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Solar Photovoltaic Glint and Glare
Study
Richard Thomas and Co - Morfa Pingett
Solar Photovoltaic Glint and Glare Study Richard Thomas and Co - Morfa Pingett - Solar Development 2
ADMINISTRATION PAGE
Job reference: 9358A
Date: February, 2019
Author: Andrea Mariano
Telephone: 01787 319001
Email: [email protected]
Reviewer: Danny Scrivener
Second reviewer: Kai Frolic
Date: February, 2019
Telephone: 01787 319001
Email: [email protected]; [email protected]
Issue Date Detail of Changes
1 February, 2019 Initial issue
Confidential: The contents of this document may not be disclosed to others without permission.
Copyright © Pager Power Limited 2019
South Suffolk Business Centre, Alexandra Road, Sudbury, CO10 2ZX
T:+44 (0)1787 319001 E:[email protected] W: https://www.pagerpower.com/
Solar Photovoltaic Glint and Glare Study Richard Thomas and Co - Morfa Pingett - Solar Development 3
EXECUTIVE SUMMARY
Report Purpose
Pager Power has been retained to assess the possible effects of glint and glare from a proposed
solar development near Pembrey Airport in Burry Port, UK. Reflections from the solar
development towards aviation receptors at Pembrey Airport, including the approach paths and
Air Traffic Control (ATC tower) have been assessed. The potential impact on surrounding roads
has also been considered.
Pager Power
Pager Power has undertaken over 350 glint and glare assessments in the UK, Europe, India and
Australasia. The company’s own glint and glare guidance is based on industry experience and
extensive consultation with industry stakeholders including airports and aviation regulators.
Conclusion
With regard to Pembrey Airport, no significant glint and glare effects are predicted because:
• Reflections are not predicted at all towards the Air Traffic Control Tower.
• Reflections towards approaching pilots are not possible:
o Approach 04: no glint and glare predicted from the model.
o Approach 22: glint and glare are geometrically possible towards the approach path;
however the reflecting panels will be outside the pilot’s view. The effects are
therefore not significant.
With regard to nearby roads, no significant glint and glare effects are predicted:
• A low impact has been predicted for some of the receptors considered, for the others no
impact was predicted. This because one of the roads is a local road and for the other there
will be enough vegetation to screen the view of drivers.
• No mitigation requirement has been identified since drivers will not look directly in the
reflection, but effects could be reduced further via the provision of screening near the road
junction at the site boundary (receptor 5).
More exhaustive information can be found from page 37 to 46.
Solar Photovoltaic Glint and Glare Study Richard Thomas and Co - Morfa Pingett - Solar Development 4
Recommendations
The results of this assessment should be made available to Pembrey Airport.
No mitigation requirement has been identified for road users because the predicted impacts
are, at worst, low. However, further screening at the road junction immediately west of the
development (receptor 5) could reduce effects even further.
Solar Photovoltaic Glint and Glare Study Richard Thomas and Co - Morfa Pingett - Solar Development 5
LIST OF CONTENTS
Administration Page ................................................................................................................................. 2
Executive Summary ................................................................................................................................... 3
Report Purpose .............................................................................................................................................. 3
Pager Power .................................................................................................................................................... 3
Conclusion........................................................................................................................................................ 3
Recommendations ........................................................................................................................................ 4
List of Contents ........................................................................................................................................... 5
List of Figures .............................................................................................................................................. 8
List of Tables ................................................................................................................................................ 9
About Pager Power ................................................................................................................................. 10
1 Introduction................................................................................................................................. 11
1.1 Overview ........................................................................................................................................... 11
1.2 Pager Power’s Experience .......................................................................................................... 11
1.3 Glint and Glare Definition .......................................................................................................... 11
2 Proposed Development Location and Details................................................................ 12
2.1 Proposed Development Location – Aerial Image............................................................. 12
2.2 Proposed Development Layout ............................................................................................... 13
3 Glint and Glare Assessment Methodology ...................................................................... 14
3.1 Guidance and Studies.................................................................................................................. 14
3.2 Background ..................................................................................................................................... 14
3.3 Methodology .................................................................................................................................. 14
3.4 Inputs ................................................................................................................................................. 15
4 Identification of Receptors .................................................................................................... 16
4.1 Overview ........................................................................................................................................... 16
4.2 Air Traffic Control Tower ............................................................................................................ 16
Solar Photovoltaic Glint and Glare Study Richard Thomas and Co - Morfa Pingett - Solar Development 6
4.3 Approaching Aircraft ................................................................................................................... 18
4.4 Roads: A484 & road southern border................................................................................... 20
5 Modelling the Solar Development ..................................................................................... 21
5.1 Resolution ........................................................................................................................................ 21
6 Glint and Glare Assessment Results ................................................................................... 22
6.1 Overview ........................................................................................................................................... 22
6.2 Results – ATC Tower..................................................................................................................... 23
6.3 Results – Approach for Runway 04 ........................................................................................ 24
6.4 Results – Approach for Runway 22 ........................................................................................ 25
6.5 Results – Road A484 .................................................................................................................... 26
6.6 Results – Local road southern border ................................................................................... 33
7 Results Discussion ..................................................................................................................... 42
7.1 ATC Tower results ......................................................................................................................... 42
7.2 Runway 04 Approach results .................................................................................................... 42
7.3 Runway 22 Approach results .................................................................................................... 42
7.4 Road results ..................................................................................................................................... 42
7.5 Overall Conclusion ........................................................................................................................ 51
8 Overall Conclusions .................................................................................................................. 52
8.1 Analysis Results .............................................................................................................................. 52
8.2 Conclusions ..................................................................................................................................... 52
Appendix A – Overview of Glint and Glare Guidance ................................................................ 53
Overview ........................................................................................................................................................ 53
UK Planning Policy ..................................................................................................................................... 53
Assessment Process .................................................................................................................................. 54
Ground Based Assessment Guidelines .............................................................................................. 54
Aviation Assessment Guidance ............................................................................................................. 54
Appendix B – Overview of Glint and Glare Studies ..................................................................... 60
Overview ........................................................................................................................................................ 60
Solar Photovoltaic Glint and Glare Study Richard Thomas and Co - Morfa Pingett - Solar Development 7
Reflection Type from Solar Panels ....................................................................................................... 60
Solar Reflection Studies ........................................................................................................................... 61
Appendix C – Overview of Sun Movements and Relative Reflections ................................. 64
Terrain Sun Curve - From lon: -4.298671 lat: 51.721264 ............................................................ 65
Appendix D – Glint and Glare Impact Significance ..................................................................... 66
Overview ........................................................................................................................................................ 66
Impact Significance Definition .............................................................................................................. 66
Assessment Process for Road Receptors .......................................................................................... 67
Assessment Process – ATC Tower........................................................................................................ 68
Assessment Process – Approaching Aircraft ................................................................................... 69
Appendix E – Pager Power’s Reflection Calculations Methodology ..................................... 70
Appendix F – Assessment Limitations and Assumptions .......................................................... 72
Pager Power’s Model ................................................................................................................................ 72
Sandia National Laboratories’ (SGHAT) Model .............................................................................. 73
Appendix G – Coordinate Data ........................................................................................................... 74
Roads receptors .......................................................................................................................................... 74
Aviation receptors ...................................................................................................................................... 75
Modelled Reflector Area ......................................................................................................................... 76
Appendix H – Geometric Calculation Results – Pager Power Results .................................. 77
Approach 22 ................................................................................................................................................. 77
Road A484 receptors ................................................................................................................................ 78
Road south of development .................................................................................................................. 81
Solar Photovoltaic Glint and Glare Study Richard Thomas and Co - Morfa Pingett - Solar Development 8
LIST OF FIGURES
Figure 1 – Aerial image of proposed development .................................................................... 12
Figure 2 – Development details: panels height, tilt and orientation .................................... 13
Figure 3 – ATC tower image ................................................................................................................ 17
Figure 4 – ATC tower location relative to the solar development......................................... 17
Figure 5 – Approaching aircraft locations ...................................................................................... 19
Figure 6 – Aerial view of A484 (red line green points) and road southern border (blue
line red points) .......................................................................................................................................... 20
Figure 7 – Part of the path will concurrently experience low impact and low screening
from vegetation ........................................................................................................................................ 43
Figure 8 – Observer 3 A484 ................................................................................................................. 44
Figure 9 – Observer 4 A484 ................................................................................................................. 45
Figure 10 – Observer 5 A484 ............................................................................................................... 45
Figure 11 – Observer 6 A484 ............................................................................................................... 46
Figure 12 – Observer 7 A484 ............................................................................................................... 46
Figure 13 – Observer 9 southern border road .............................................................................. 47
Figure 14 – Observer 10 southern border road ........................................................................... 48
Figure 15 – Observer 11 southern border road ........................................................................... 48
Figure 16 – Observer 12 southern border road ........................................................................... 49
Figure 17 – Observer 13 southern border road ........................................................................... 49
Figure 18 – Observer 14 southern border road ........................................................................... 50
Figure 19 – Observer 15 southern border road ........................................................................... 50
Figure 20 – Observer 16 southern border road ........................................................................... 51
Solar Photovoltaic Glint and Glare Study Richard Thomas and Co - Morfa Pingett - Solar Development 9
LIST OF TABLES
Table 1 – Glare intensity designation ............................................................................................... 22
Table 2 – ATC tower results ................................................................................................................. 23
Table 3 – Runway 04 approach results ............................................................................................ 24
Table 4 – Runway 22 approach results ............................................................................................ 25
Table 5 – Road A484 results ................................................................................................................ 32
Table 6 – Local road southern border results ............................................................................... 41
Solar Photovoltaic Glint and Glare Study Richard Thomas and Co - Morfa Pingett - Solar Development 10
ABOUT PAGER POWER
Pager Power is a dedicated consultancy company based in Suffolk, UK. The company has
undertaken projects in 44 countries within Africa, Europe, America, Asia and Australasia.
The company comprises a team of experts to provide technical expertise and guidance on a
range of planning issues for large and small developments.
Pager Power was established in 1997. Initially the company focus was on modelling the impact
of wind turbines on radar systems. Over the years, the company has expanded into numerous
fields including:
• Renewable energy projects.
• Building developments.
• Aviation and telecommunication systems.
Pager Power prides itself on providing comprehensive, understandable and accurate
assessments of complex issues in line with national and international standards. This is
underpinned by its custom software, longstanding relationships with stakeholders and active
role in conferences and research efforts around the world.
Pager Power’s assessments withstand legal scrutiny and the company can provide support for
a project at any stage.
Solar Photovoltaic Glint and Glare Study Richard Thomas and Co - Morfa Pingett - Solar Development 11
1 INTRODUCTION
1.1 Overview
Pager Power has been retained to assess the possible effects of glint and glare from a proposed
solar photovoltaic development located near Pembrey Airport in Burry Port, UK.
The assessment has considered potential impacts on aviation activity with specific reference to
Pembrey Airport and the potential impact upon surrounding roads. The report contains the
following:
• Proposed development details.
• Explanation of glint and glare.
• Overview of relevant guidance.
• Overview of relevant studies.
• Overview of Sun movement.
• Assessment methodology.
• Identification of aviation receptors including relevant approach paths.
• Identification of road receptors.
• Glint and glare assessment for identified receptors.
• Results discussion.
1.2 Pager Power’s Experience
Pager Power has undertaken over 350 Glint and Glare assessments within the UK and
internationally. The studies have included assessment civil and military aerodromes, railway
infrastructure and other ground-based receptors including roads and dwellings.
1.3 Glint and Glare Definition
The definition of glint and glare can vary however, the definition used by Pager Power is as
follows:
• Glint – a momentary flash of bright light typically received by moving receptors or from
moving reflectors.
• Glare – a continuous source of bright light typically received by static receptors or from
large reflective surfaces.
These definitions are aligned with those of the Federal Aviation Administration (FAA) in the
United States of America. The term ‘solar reflection’ is used in this report to refer to both
reflection types i.e. glint and glare.
Solar Photovoltaic Glint and Glare Study Richard Thomas and Co - Morfa Pingett - Solar Development 12
2 PROPOSED DEVELOPMENT LOCATION AND DETAILS
2.1 Proposed Development Location – Aerial Image
The location of the proposed development is shown in the aerial image1 of Figure 1 below (panel
array shown by red line).
Figure 1 – Aerial image of proposed development
1 Source: Copyright © 2019 Google.
Solar Photovoltaic Glint and Glare Study Richard Thomas and Co - Morfa Pingett - Solar Development 13
2.2 Proposed Development Layout
The following panel details (Figure 22) have been assessed:
• A vertical tilt of 20 degrees above the horizontal.
• A height above ground of 0.75 metres, a mid-height of 1.08 meters and a top height of
2.16 meters. The panel midpoint has been considered for the analysis.
• An azimuth angle of 198.6 degrees for all panels.
Figure 2 – Development details: panels height, tilt and orientation
2 Source: IKAROS SOLAR 07/08/2018.
Solar Photovoltaic Glint and Glare Study Richard Thomas and Co - Morfa Pingett - Solar Development 14
3 GLINT AND GLARE ASSESSMENT METHODOLOGY
3.1 Guidance and Studies
Guidelines exist in the UK (produced by the Civil Aviation Authority) and in the USA (produced
by the Federal Aviation Administration) with respect to solar developments and aviation activity.
Independent studies regarding the relative reflectivity of solar panels and other materials have
been undertaken (see Appendices A and B).
Pager Power’s assessment methodology is based on compiled guidance from these sources,
industry experience and consultation with the relevant bodies.
Key points from the literature are:
• Specular reflections of the Sun from solar panels are possible.
• The measured intensity of a reflection from solar panels can vary from 2% to 30%
depending on the angle of incidence.
• The intensity of reflections from solar panels are equal to or less than those from water.
Reflections from solar panels are significantly less intense than many other reflective
surfaces which are common in an outdoor environment.
3.2 Background
Details of the Sun’s movements and solar reflections are presented in Appendix C.
3.3 Methodology
The glint and glare assessment methodology has been derived from the information provided
to Pager Power through consultation with stakeholders and by reviewing the available guidance.
The methodology for the glint and glare assessment is shown below.
• Identify receptors in the area surrounding the proposed solar development.
• Consider direct solar reflections from the proposed solar development towards the
identified receptors by undertaking geometric calculations.
• Consider the visibility of the panels from the receptor’s location. If the panels are not
visible from the receptor then no reflection can occur.
• Based on the results of the geometric calculations, determine whether a reflection can
occur, and if so, at what time it will occur.
• Consider both the solar reflection from the proposed solar development and the
location of the direct sunlight with respect to the receptor’s position.
• Consider the solar reflection with respect to the published studies and guidance –
including intensity calculations for aviation receptors.
Solar Photovoltaic Glint and Glare Study Richard Thomas and Co - Morfa Pingett - Solar Development 15
• Determine whether a significant detrimental impact is expected in accordance with the
methodology presented in Appendix D.
3.4 Inputs
Within the Pager Power model, the solar development area is defined, as well as the relevant
receptor locations. The result is a chart that shows whether a reflection can occur, the duration
and the panels that can produce the solar reflection towards the receptor. See Appendix E for
technical information regarding the methodology. Solar reflection intensities are cross-checked
using external software that is aligned with the Sandia Laboratories methodology. Limitations
and assumptions are presented in Appendix F.
Solar Photovoltaic Glint and Glare Study Richard Thomas and Co - Morfa Pingett - Solar Development 16
4 IDENTIFICATION OF RECEPTORS
4.1 Overview
This assessment has been carried out with specific reference to potential impacts at Pembrey
Airport (ATC tower and runaways), in accordance with the recommended guidance, and ground
level road receptors including the A484 road and the local road situated to the development’s
southern border, in accordance with Pager Power guidance.
There is no formal guidance with regard to the maximum distance at which glint and glare
should be assessed. From a technical perspective, there is no maximum distance for potential
reflections.
However, the significance of a solar reflection decreases with distance. This is because the
proportion of an observer’s field of vision that is taken up by the reflecting area diminishes as
the separation distance increases.
Terrain and shielding by vegetation are also more likely to obstruct an observer’s view at longer
distances for ground-based receptors.
4.2 Air Traffic Control Tower
The ATC tower is located to the east of the runway at Pembrey Airport, approximately 1.15 km
southwest of the proposed development.
The tower co-ordinates have been extrapolated from aerial imagery (Figure3 3 and 4 on the
following page) and are shown in Appendix G. The tower height has been estimated to be 5
meters above ground level.
3 Source: Copyright © 2019 Google.
Solar Photovoltaic Glint and Glare Study Richard Thomas and Co - Morfa Pingett - Solar Development 17
Figure 3 – ATC tower image
Figure 4 – ATC tower location relative to the solar development
Solar Photovoltaic Glint and Glare Study Richard Thomas and Co - Morfa Pingett - Solar Development 18
4.3 Approaching Aircraft
It is Pager Power’s methodology to assess whether a solar reflection can be experienced on the
approach paths for the associated runways. Pembrey Airport has approach paths for one
runaway.
A geometric glint and glare assessment has been undertaken for both aircraft approach paths
for the runway. This is considered the most critical stage of the flight. The Pager Power approach
for determining receptor (aircraft) locations on the approach path is to select locations along
the extended runway centre line from 50ft above the runway threshold out to a distance of 2
miles. The height of the aircraft is determined by using a 3-degree descent path relative to the
runway threshold height. The Sandia Laboratories methodology, recommended by the USA’s
Federal Aviation Administration, uses the same criteria. Figure 54 in the following page shows
the assessed aviation receptors overlaid on aerial imagery of the airport.
4 Source: Copyright © 2019 Google.
Solar Photovoltaic Glint and Glare Study Richard Thomas and Co - Morfa Pingett - Solar Development 19
Figure 5 – Approaching aircraft locations
Solar Photovoltaic Glint and Glare Study Richard Thomas and Co - Morfa Pingett - Solar Development 20
4.4 Roads: A484 & road southern border
The analysis has considered through-roads that:
• Are within, or close to one kilometre of the proposed development; and
• Have a potential view of the panels.
The assessed roads receptor points are shown as green and red icons in Figure 65 below. The
A484 is located 55 meters (at its closest point) west of the solar development (green icons) while
the road at the southern border is located at 20 meters from the site boundary (red line). The
direction of the A484 North-South while for the local road the direction is East-West. A height
above ground level of 1.5 metres has been taken as typical eye level for a road user for both
roads. The co-ordinates of the receptor points are presented in Appendix G.
Figure 6 – Aerial view of A484 (red line green points) and road southern border (blue line red points)
5 Source: Copyright © 2019 Google.
Solar Photovoltaic Glint and Glare Study Richard Thomas and Co - Morfa Pingett - Solar Development 21
5 MODELLING THE SOLAR DEVELOPMENT
5.1 Resolution
A number of representative panel locations are selected within the proposed solar development
site boundary. The number of locations is determined by the size of the proposed solar
development and the assessment resolution. The bounding co-ordinates for the proposed solar
development have been extrapolated from the available site maps. The assessment is considered
conservative and robust. All ground heights have been taken from Pager Power’s database.
Boundary coordinate data is shown in Appendix G.
A resolution of 1m has been chosen for this assessment (Pager Power model). This means that
a geometric calculation is undertaken for each identified receptor every 1m from within the
defined solar development area. This resolution is sufficiently high to maximise the accuracy of
the results – increasing the resolution further would not significantly change the modelling
output. If a reflection is experienced from an assessed panel location, then it is likely that a
reflection will be viewable from similarly located panels within the development.
Solar Photovoltaic Glint and Glare Study Richard Thomas and Co - Morfa Pingett - Solar Development 22
6 GLINT AND GLARE ASSESSMENT RESULTS
6.1 Overview
The Pager Power model has been used to identify whether reflections are possible, and when
they would occur. Where solar reflections have been predicted, intensity calculations in
accordance with Sandia National Laboratories’ methodology have been undertaken.
Where glare is predicted, the intensity model calculates the expected intensity of a reflection
with respect to the potential for an after-image (or worse) occurring. The designation used by
the model is presented in Table 1 below along with the associated colour coding.
Coding Used Intensity Key
Glare beyond 50°
Low potential
Potential
Potential for
permanent eye
damage
Table 1 – Glare intensity designation
This coding has been used in the table where a reflection has been calculated and is in
accordance with Sandia National Laboratories’ methodology.
In addition, the intensity model allows for assessment of a variety of solar panel surface
materials. In the first instance, a surface material of ‘smooth glass without an anti-reflective
coating’ is assessed. This is the most reflective surface and allows for a ‘worst case’ assessment.
Other surfaces that could be modelled include:
• Smooth glass with an anti-reflective coating;
• Light textured glass without an anti-reflective coating;
• Light textured glass with an anti-reflective coating; or
• Deeply textured glass.
If significant glare is predicted, modelling of less reflective surfaces could be undertaken.
The tables in the following subsections summarise the results of the assessment.
Solar Photovoltaic Glint and Glare Study Richard Thomas and Co - Morfa Pingett - Solar Development 23
6.2 Results – ATC Tower
Receptor
Pager Power Results
Glare Type Comment Theoretical reflection times towards ATC tower, GMT (approx.)
am pm
ATC None. None. N/A – No glare predicted.
No reflections are
predicted towards the
ATC tower.
Table 2 – ATC tower results
Solar Photovoltaic Glint and Glare Study Richard Thomas and Co - Morfa Pingett - Solar Development 24
6.3 Results – Approach for Runway 04
Receptor
Pager Power Results
Glare Type Comment Theoretical reflection times towards Runway 04, GMT (approx.)
am pm
Threshold
up to 2
miles
None. None. N/A – No glare predicted.
No reflections are
predicted towards pilots
approaching within 2
miles of the threshold.
Table 3 – Runway 04 approach results
Solar Photovoltaic Glint and Glare Study Richard Thomas and Co - Morfa Pingett - Solar Development 25
6.4 Results – Approach for Runway 22
Receptor
Pager Power Results
Glare Type Comment Theoretical reflection times towards Runway 22, GMT (approx.)
am pm
Threshold None.
None.
Not applicable because
the viewer will be at an
angle of more than 50°
compared to the solar
panels’ location.
No visible reflections are
predicted towards pilots
approaching within 2
miles of the threshold.
0.25 miles Between 6.50 and 7.20 from May to
early August
0.50 miles
Between 8.00 and 8.50 from mid-
January to mid-February and
between 7.30 to 8.10 mid-October
to mid-November
0.75 – 2
miles None.
Table 4 – Runway 22 approach results
Solar Photovoltaic Glint and Glare Study Richard Thomas and Co - Morfa Pingett - Solar Development 26
6.5 Results – Road A484
Receptor
Pager Power Results
Comment Theoretical reflection times towards Road A484, GMT (approx.)
am pm
1-2 None. None. None.
Solar Photovoltaic Glint and Glare Study Richard Thomas and Co - Morfa Pingett - Solar Development 27
Receptor
Pager Power Results
Comment Theoretical reflection times towards Road A484, GMT (approx.)
am pm
3
Reflection are possible between 7:00 and 7:40
from late February to early April. It is also
expected between 6:50 and 7:10 from
September until mid-October.
None.
Reflections would occur from
the northern portion of
development. The analysis
shows that there is line of sight
between drivers travelling
south and the panels, however
the panels will be outside the
drivers’ view and existing
vegetation will screen
completely the site (Figure 8).
Also, the solar reflection and
direct sunlight will originate
from the same location during
that time of the year.
Effects are possible.
Solar Photovoltaic Glint and Glare Study Richard Thomas and Co - Morfa Pingett - Solar Development 28
Receptor
Pager Power Results
Comment Theoretical reflection times towards Road A484, GMT (approx.)
am pm
4 Reflection are possible between 6:40 and 7:30
from late February to late October. None.
Reflections would occur from
almost all development area.
The analysis shows that there is
line of sight between drivers
travelling south and the panels,
however the panels will be
outside the drivers’ view and
existing vegetation will
completely screen the site
(Figure 9). Also, the solar
reflection and direct sunlight
will originate from the same
location during that time of the
year.
Effects are possible.
Solar Photovoltaic Glint and Glare Study Richard Thomas and Co - Morfa Pingett - Solar Development 29
Receptor
Pager Power Results
Comment Theoretical reflection times towards Road A484, GMT (approx.)
am pm
5 Reflection are possible between 6:40 and 7:30
from late February to late October. None.
Reflections would occur from
the south eastern portion of
development. The analysis
shows that there is line of sight
between drivers travelling
south and the panels, however
the panels will be outside the
drivers’ view and existing
vegetation will completely
screen the site (Figure 10). Also,
the solar reflection and direct
sunlight will originate from the
same location during that time
of the year.
Effects are possible.
Solar Photovoltaic Glint and Glare Study Richard Thomas and Co - Morfa Pingett - Solar Development 30
Receptor
Pager Power Results
Comment Theoretical reflection times towards Road A484, GMT (approx.)
am pm
6 Reflection are possible between 6:40 and 7:10
from early April September. None.
Reflections would be from the
south-eastern portion of
development. The analysis
shows that there is line of sight
between drivers travelling
south and the panels, however
the panels will be outside the
drivers’ view. In this case
existing vegetation will not
completely screen the site
(Figure 11). Also, the solar
reflection and direct sunlight
will originate from the same
location during that time of the
year.
Effects are possible.
Solar Photovoltaic Glint and Glare Study Richard Thomas and Co - Morfa Pingett - Solar Development 31
Receptor
Pager Power Results
Comment Theoretical reflection times towards Road A484, GMT (approx.)
am pm
7 Reflection are possible between 6:40 and 7:10
from June to early July. None.
Reflections would be from the
south-eastern portion of
development. The analysis
shows that there is line of sight
between drivers travelling
south and the panels, however
the panels will be outside the
drivers’ view. In this case
existing vegetation will not
completely screen the site
(Figure 12). Also, the solar
reflection and direct sunlight
will originate from the same
location during that time of the
year.
Effects are possible.
Solar Photovoltaic Glint and Glare Study Richard Thomas and Co - Morfa Pingett - Solar Development 32
Receptor
Pager Power Results
Comment Theoretical reflection times towards Road A484, GMT (approx.)
am pm
8 None. None. None.
Table 5 – Road A484 results
Solar Photovoltaic Glint and Glare Study Richard Thomas and Co - Morfa Pingett - Solar Development 33
6.6 Results – Local road southern border
Receptor
Pager Power Results
Comment Theoretical reflection times towards Local road southern border, GMT (approx.)
am pm
9 Reflection are possible between 6:40 due 7:10
from mid-March to end of September. None.
Reflections would be from the
south eastern position of
development. The analysis
shows that there is line of sight
between drivers travelling east
and the panels. However,
existing vegetation will
completely screen the site
(Figure 13). Also, the solar
reflection and direct sunlight
will originate from the same
location during that time of the
year.
Effects are possible.
Solar Photovoltaic Glint and Glare Study Richard Thomas and Co - Morfa Pingett - Solar Development 34
Receptor
Pager Power Results
Comment Theoretical reflection times towards Local road southern border, GMT (approx.)
am pm
10 Reflection are possible between 6:30 and 7:10
from early April to early September. None.
Reflections would be from the
south eastern position of
development. The analysis
shows that there is line of sight
between drivers travelling east
and the panels. In this case
existing vegetation will not
completely screen the site
(Figure 14). Also, the solar
reflection and direct sunlight
will originate from the same
location during that time of the
year.
Effects are possible.
Solar Photovoltaic Glint and Glare Study Richard Thomas and Co - Morfa Pingett - Solar Development 35
Receptor
Pager Power Results
Comment Theoretical reflection times towards Local road southern border, GMT (approx.)
am pm
11 Reflection is expected between 6:40 until 7:10
from early May to early August.
Reflection is expected between 19:20 until
19:40 from early May to late July.
Reflections would be from the
south eastern and western
position of development. The
analysis shows that there is line
of sight between drivers
travelling both direction and
the panels. In this case existing
vegetation will not completely
screen the site (Figure 15). Also,
the solar reflection and direct
sunlight will originate from the
same location during that time
of the year.
Effects are possible.
Solar Photovoltaic Glint and Glare Study Richard Thomas and Co - Morfa Pingett - Solar Development 36
Receptor
Pager Power Results
Comment Theoretical reflection times towards Local road southern border, GMT (approx.)
am pm
12 None. Reflection is expected between 19:10 until
19:30 from early May to mid-August.
Reflections would be from the
south western position of
development. The analysis
shows that there is line of sight
between drivers travelling west
and the panels. However,
existing vegetation will
completely screen the site
(Figure 16). Also, the solar
reflection and direct sunlight
will originate from the same
location during that time of the
year.
Effects are possible.
Solar Photovoltaic Glint and Glare Study Richard Thomas and Co - Morfa Pingett - Solar Development 37
Receptor
Pager Power Results
Comment Theoretical reflection times towards Local road southern border, GMT (approx.)
am pm
13 None. Reflection is expected between 19:05 until
19:30 from early May to mid-August.
Reflections would be from the
south western position of
development. The analysis
shows that there is line of sight
between drivers travelling west
and the panels. However,
existing vegetation will
completely screen the site
(Figure 17). Also, the solar
reflection and direct sunlight
will originate from the same
location during that time of the
year.
Effects are possible.
Solar Photovoltaic Glint and Glare Study Richard Thomas and Co - Morfa Pingett - Solar Development 38
Receptor
Pager Power Results
Comment Theoretical reflection times towards Local road southern border, GMT (approx.)
am pm
14 None. Reflection is expected between 19:05 until
19:30 from early May to mid-August.
Reflections would be from the
south western position of
development. The analysis
shows that there is line of sight
between drivers travelling west
and the panels. However,
existing vegetation will
completely screen the site
(Figure 18). Also, the solar
reflection and direct sunlight
will originate from the same
location during that time of the
year.
Effects are possible.
Solar Photovoltaic Glint and Glare Study Richard Thomas and Co - Morfa Pingett - Solar Development 39
Receptor
Pager Power Results
Comment Theoretical reflection times towards Local road southern border, GMT (approx.)
am pm
15 None. Reflection is expected between 19:05 until
19:30 from early May to mid-August.
Reflections would be from the
south western position of
development. The analysis
shows that there is line of sight
between drivers travelling west
and the panels. However,
existing vegetation will
completely screen the site
(Figure 19). Also, the solar
reflection and direct sunlight
will originate from the same
location during that time of the
year.
Effects are possible.
Solar Photovoltaic Glint and Glare Study Richard Thomas and Co - Morfa Pingett - Solar Development 40
Receptor
Pager Power Results
Comment Theoretical reflection times towards Local road southern border, GMT (approx.)
am pm
16 None. Reflection is expected between 19:05 until
19:30 from early May to mid-August.
Reflections would be from the
south western position of
development. The analysis
shows that there is line of sight
between drivers travelling west
and the panels. However,
existing vegetation will
completely screen the site
(Figure 20). Also, the solar
reflection and direct sunlight
will originate from the same
location during that time of the
year.
Effects are possible.
Solar Photovoltaic Glint and Glare Study Richard Thomas and Co - Morfa Pingett - Solar Development 41
Receptor
Pager Power Results
Comment Theoretical reflection times towards Local road southern border, GMT (approx.)
am pm
17 – 23 None. None.
No impact predicted. Existing
vegetation will screen the site
from all of these receptors.
Table 6 – Local road southern border results
Solar Photovoltaic Glint and Glare Study Richard Thomas and Co - Morfa Pingett - Solar Development 42
7 RESULTS DISCUSSION
7.1 ATC Tower results
None of the models predicted solar reflections at the ATC tower.
No impacts are predicted.
7.2 Runway 04 Approach results
None of the models predicted solar reflection at the Approach Runway 04.
No impacts are predicted.
7.3 Runway 22 Approach results
The Pager Power model predicts reflections at receptor 0.25 and 0.50 miles. However, during
landing operation a pilot would not be looking towards the panel area since the PV arrays are
located North of the receptor point while the plane’s landing direction will be South-West.
No effects are predicted.
7.4 Road results
Based on the review of the analysis and available imagery, at 13 of the 23 points assessed a solar
reflection is geometrically possible. This is equivalent to 0.6km of road. However, when existing
screening is considered the solar reflection zone is reduced to approximately 170m. This is
presented in Figure 76 (orange lines) on the following page.
6 Source: Copyright © 2019 Google.
Solar Photovoltaic Glint and Glare Study Richard Thomas and Co - Morfa Pingett - Solar Development 43
Figure 7 – Part of the path will concurrently experience low impact and low screening from vegetation
7.4.1 A484 Road
Up to 0.3km of this road will experience a solar reflection. The speed limit on this road is 50mph
and it is likely that drivers will travel at such speed. The solar reflection will last 20 minutes per
day. Its duration would depend on the speed of the car travelling through the solar reflection
zone. Note that not all the solar panels will be producing a reflection at the same time. The Pager
Power model predicts a solar reflection at receptors 3, 4, 5, 6 and 7 for a considerable amount
of time throughout the majority of the year.
Glint and glare will not be an issue for people travelling in North-South direction, however solar
reflection might be visible for people travelling in the opposite direction since the solar panels
may be visible. Available imagery shows that significant screening in the form of vegetation
would shield the view of the reflecting solar panels especially for receptors 6 and 7 (Figures7 11
and 12 on the following pages).
7 Source: Copyright © 2019 Google.
Solar Photovoltaic Glint and Glare Study Richard Thomas and Co - Morfa Pingett - Solar Development 44
However, the vegetation is not consistent throughout all the road bordering, from receptors 3,
4 and 5 (Figures8 8 to 108 on the following pages). The view of the proposed solar development
from the vehicle will be at a lower height (1.5 metres) compared to the imagery provided from
the Google camera (2.5 metres) resulting in lower chances of establishing a line of sight with the
site.
Figure 8 – Observer 3 A484
8 Source: Copyright © 2019 Google.
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Figure 9 – Observer 4 A484
Figure 10 – Observer 5 A484
Solar Photovoltaic Glint and Glare Study Richard Thomas and Co - Morfa Pingett - Solar Development 46
Figure 11 – Observer 6 A484
Figure 12 – Observer 7 A484
Solar Photovoltaic Glint and Glare Study Richard Thomas and Co - Morfa Pingett - Solar Development 47
7.4.2 Local road southern border
Only 0.75km of this road will experience solar reflection. At this point the speed limit will be
60mph and it is extremely unlikely that drivers will travel at such speed due to the size of the
carriage. The solar reflection will last 20 minutes per day. Its duration would depend on the
speed of the car travelling through the solar reflection zone. Note that not all the solar panels
will be producing a reflection at the same time. The Pager Power model predicts a solar reflection
at receptors location 9 to 16 for a considerable amount of time throughout the majority of the
year.
Glint and glare will can be an issue for people travelling in both direction since the solar panels
will be visible. However, available imagery shows that significant screening in the form of
vegetation which would shield the view of the reflective solar panels especially for receptors
location 9,12,13,14,15 and 16 (Figures9 13, 14, 17, 18, 19 and 20 on the following pages).
However, the vegetation is not consistent throughout all the road section, from receptors 10
and 11 (Figures10 14 to 15 on the following pages). The view of the proposed solar development
from the vehicle will be at a lower height (1.5 metre) compared to the imagery provided from
the Google camera (2.5 metre) resulting in lower chances of establishing a line of sight with the
site.
Figure 13 – Observer 9 southern border road
9 Source: Copyright © 2019 Google.
10 Source: Copyright © 2019 Google.
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Figure 14 – Observer 10 southern border road
Figure 15 – Observer 11 southern border road
Solar Photovoltaic Glint and Glare Study Richard Thomas and Co - Morfa Pingett - Solar Development 49
Figure 16 – Observer 12 southern border road
Figure 17 – Observer 13 southern border road
Solar Photovoltaic Glint and Glare Study Richard Thomas and Co - Morfa Pingett - Solar Development 50
Figure 18 – Observer 14 southern border road
Figure 19 – Observer 15 southern border road
Solar Photovoltaic Glint and Glare Study Richard Thomas and Co - Morfa Pingett - Solar Development 51
Figure 20 – Observer 16 southern border road
7.5 Overall Conclusion
7.5.1 Aviation receptors
No significant impact has been highlighted based on the results of the analysis carried out with
Pager Power software.
7.5.2 Road receptors
In accordance with Pager Power methodology set out in Section 3 and Appendix D, the impact
upon road users with respect to safety is therefore classified as low where the reflecting solar
panels are visible and there is no requirement for mitigation based on Pager Power’s assessment
guidance. This is because for both roads the reflection will not originate in front of the road user
and/or it is significantly screened considering existing screening. However, despite low impact
predicted, for receptor 5 (Figure 10) glint and glare effects can be reduced further via the
provision of screening near the junction.
Solar Photovoltaic Glint and Glare Study Richard Thomas and Co - Morfa Pingett - Solar Development 52
8 OVERALL CONCLUSIONS
8.1 Analysis Results
The analysis has shown that:
• No significant reflections predicted:
o Runaway 04: no reflection predicted
o Runway 22: reflection predicted but outside pilot sight range
• No reflections towards the Air Traffic Control tower at Pembrey Airport is expected.
• The impact of reflection on the receptors analysed for both roads is considered low.
8.2 Conclusions
• No significant impact upon aviation operations at Pembrey Airport are anticipated
• Low impact predicted for both the A484 and the local road which runs alongside the
southern border. No mitigation requirement has been identified, but effects could be
reduced further via the provision of screening near the road junction at the site
boundary.
Solar Photovoltaic Glint and Glare Study Richard Thomas and Co - Morfa Pingett - Solar Development 53
APPENDIX A – OVERVIEW OF GLINT AND GLARE GUIDANCE
Overview
This section presents details regarding the relevant guidance and studies with respect to the
considerations and effects of solar reflections from solar panels, known as ‘Glint and Glare’ .
This is not a comprehensive review of the data sources, rather it is intended to give an overview
of the important parameters and considerations that have informed this assessment.
UK Planning Policy
UK National Planning Practice Guidance dictates that in some instances a glint and glare
assessment is required however, there is no specific guidance with respect to the methodology
for assessing the impact of glint and glare.
The planning policy from the Department for Communities and Local Government (paragraph
2711) states:
‘Particular factors a local planning authority will need to consider include… the effect on landscape
of glint and glare and on neighbouring uses and aircraft safety.’
The National Planning Policy Framework for Renewable and Low Carbon Energy12 (specifically
regarding the consideration of solar farms) states:
‘What are the particular planning considerations that relate to large scale ground-mounted solar
photovoltaic Farms?
The deployment of large-scale solar farms can have a negative impact on the rural environment,
particularly in undulating landscapes. However, the visual impact of a well-planned and well-
screened solar farm can be properly addressed within the landscape if planned sensitively.
Particular factors a local planning authority will need to consider include:
• the proposal’s visual impact, the effect on landscape of glint and glare (see guidance on
landscape assessment) and on neighbouring uses and aircraft safety;
• the extent to which there may be additional impacts if solar arrays follow the daily
movement of the sun;
11 http://planningguidance.planningportal.gov.uk/blog/guidance/renewable-and-low-carbon-energy/ 12Reference ID: 5-013-20140306, paragraph 13-13,http://planningguidance.planningportal.gov.uk/blog/guidance/
renewable-and-low-carbon-energy/particular-planning-considerations-for-hydropower-active-solar-technology-solar-
farms-and-wind-turbines/
Solar Photovoltaic Glint and Glare Study Richard Thomas and Co - Morfa Pingett - Solar Development 54
The approach to assessing cumulative landscape and visual impact of large scale solar farms is
likely to be the same as assessing the impact of wind turbines. However, in the case of ground-
mounted solar panels it should be noted that with effective screening and appropriate land
topography the area of a zone of visual influence could be zero.’
Assessment Process
No process for determining and contextualising the effects of glint and glare are, however,
provided. Therefore, the Pager Power approach is to determine whether a reflection from the
proposed solar development is geometrically possible and then to compare the results against
the relevant guidance/studies to determine whether the reflection is significant.
Ground Based Assessment Guidelines
There are no specific guidelines for assessing the impact of solar reflections upon surrounding
roads and dwellings. Therefore, the Pager Power approach has been informed by the policy
presented above, current studies (presented in Appendix B) and stakeholder consultation.
Aviation Assessment Guidance
The UK Civil Aviation Authority (CAA) issued interim guidance relating to Solar Photovoltaic
Systems (SPV) on 17 December 2010 and was subject to a CAA information alert 2010/53. The
formal policy was cancelled on September 7th, 201213 however the advice is still applicable14 until
a formal policy is developed. The relevant aviation guidance from the CAA is presented in the
section below.
CAA Interim Guidance
This interim guidance makes the following recommendations (p.2-3):
‘8. It is recommended that, as part of a planning application, the SPV developer provide safety
assurance documentation (including risk assessment) regarding the full potential impact of the
SPV installation on aviation interests.
9. Guidance on safeguarding procedures at CAA licensed aerodromes is published within CAP 738
Safeguarding of Aerodromes and advice for unlicensed aerodromes is contained within CAP 793
Safe Operating Practices at Unlicensed Aerodromes.
10. Where proposed developments in the vicinity of aerodromes require an application for planning
permission the relevant LPA normally consults aerodrome operators or NATS when aeronautical
interests might be affected. This consultation procedure is a statutory obligation in the case of
certain major airports, and may include military establishments and certain air traffic surveillance
13 http://www.caa.co.uk/docs/697/srg_asd_solarphotovoltaicsystguidance.pdf
14 Reference email from the CAA dated 19.05.2014.
Solar Photovoltaic Glint and Glare Study Richard Thomas and Co - Morfa Pingett - Solar Development 55
technical sites. These arrangements are explained in Department for Transport Circular 1/2003
and for Scotland, Scottish Government Circular 2/2003.
11. In the event of SPV developments proposed under the Electricity Act, the relevant government
department should routinely consult with the CAA. There is therefore no requirement for the CAA
to be separately consulted for such proposed SPV installations or developments.
12. If an installation of SPV systems is planned on-aerodrome (i.e. within its licensed boundary)
then it is recommended that data on the reflectivity of the solar panel material should be included
in any assessment before installation approval can be granted. Although approval for installation
is the responsibility of the ALH15, as part of a condition of a CAA Aerodrome Licence, the ALH is
required to obtain prior consent from CAA Aerodrome Standards Department before any work is
begun or approval to the developer or LPA is granted, in accordance with the procedures set out
in CAP 791 Procedures for Changes to Aerodrome Infrastructure.
13. During the installation and associated construction of SPV systems there may also be a need
to liaise with nearby aerodromes if cranes are to be used; CAA notification and permission is not
required.
14. The CAA aims to replace this informal guidance with formal policy in due course and reserves
the right to cancel, amend or alter the guidance provided in this document at its discretion upon
receipt of new information.
15. Further guidance may be obtained from CAA’s Aerodrome Standards Department via
FAA Guidance
The most comprehensive guidelines available for the assessment of solar developments near
aerodromes were produced initially in November 2010 by the United States Federal Aviation
Administration (FAA) and updated in 2013.
The 2010 document is entitled ‘Technical Guidance for Evaluating Selected Solar Technologies on
Airports’16 and the 2013 update is entitled ‘Interim Policy, FAA Review of Solar Energy System
Projects on Federally Obligated Airports’17.
Key points from the 2010 FAA guidance are presented below.
15 Aerodrome Licence Holder.
16 http://www.faa.gov/airports/environmental/policy_guidance/media/airport_solar_guide_print.pdf
17 http://www.gpo.gov/fdsys/pkg/FR-2013-10-23/pdf/2013-24729.pdf
Solar Photovoltaic Glint and Glare Study Richard Thomas and Co - Morfa Pingett - Solar Development 56
• The potential impacts of reflectivity are glint and glare (referred to henceforth just as glare)
which can cause a brief loss of vision (also known as flash blindness).
• Reflectivity from solar panels could cause flash blindness18 episodes on pilots or air traffic
controllers when 7-11 W/m2 reaches the eye.
• Today’s solar panels reflect as little as 2% of the incoming sunlight meaning roughly 20 W/m2
are reflected off a typical PV panel.
• PV solar panels reflect less light than other substances such as snow, vegetation and water.
• Reflections from PV panels are specular because of their smooth surfaces – meaning that
reflected light from a specific source is reflected in a single direction.
• Glare analysis can include one or more of:
o A qualitative analysis of potential impact in consultation with the Control Tower,
pilots and airport officials;
o A demonstration field test with solar panels at the proposed site in coordination with
FAA Tower personnel;
o A geometric analysis to determine days and times when an impact is predicted.
• The extent of reflectivity analysis required to assess potential impacts will depend on the
specific project site and system design.
• Reflection in the form of glare is present in current aviation operations. The existing sources
of glare come from glass windows, auto surface parking, rooftops, and water bodies. Figure 16
(not shown) shows the percent of incoming sunlight that is reflected off of a variety of surfaces.
At airports, existing reflecting surfaces may include hangar roofs, surface parking, and glassy
office buildings. To minimize unexpected glare, windows of air traffic control towers and
airplane cockpits are coated with anti-reflective glazing and operators will wear polarized eye
wear. Potential glare from solar panels should be viewed in this context. Any airport
considering a PV installation should first review existing sources of glare at the airport and the
effectiveness of measures used to mitigate that glare.
• Geometric studies are the most technical approach for reflectivity issues that are difficult to
assess. Studies of glare can employ geometry and the known path of the sun to predict when
sunlight will reflect off of a fixed surface (like a solar panel) and contact a fixed receptor (e.g.,
control tower). At any given site, the sun not only moves across the sky every day, but its path
18 Flash Blindness, as described in the FAA guidelines, can be described as a temporary visual interference effect that
persists after the source of illumination has ceased. This occurs from many reflective materials in the ambient
environment.
Solar Photovoltaic Glint and Glare Study Richard Thomas and Co - Morfa Pingett - Solar Development 57
in the sky changes during various times of year. This in turn alters the destination of the
resultant reflections since the angle of reflection for the solar panels will be the same as the
angle at which the sun hits the panels. The larger the reflective surface, the greater the
likelihood of glare impacts.
• Solar installations are presently operating at a number of airports including megawatt-sized
solar facilities covering multiple acres. Project managers from six airports where solar has been
operational for one to three years were asked about glare complaints. Air traffic controllers
were contacted from three of those airports and asked to comment on the effect of glare on
their daily operations. To date, there have been no serious complaints from pilots or air traffic
control due to glare impacts from existing airport solar PV installations.
Any potential problems in this area have apparently been resolved prior to construction
through one or a combination of the strategies described above. The anecdotal evidence
suggests that either considerable glare is not occurring during times of operation or if glare is
occurring, it is not a negative effect and is a minor part of the landscape to which pilots and
tower personnel are exposed.
From October 2013, the FAA is reviewing multiple sections of the guidance based on new
information and field experience. An overview of the 2013 FAA interim guidance is presented
below.
• Solar energy systems located on an airport that is not federally-obligated or located outside
the property of a federally-obligated airport are not subject to this policy.
• Proponents of solar energy systems located off-airport property or on non-federally-obligated
airports are strongly encouraged to consider the requirements of this policy when siting such
system.
• FAA adopts the Solar Glare Hazard Analysis Plot shown…below as the standard for measuring
the ocular impact of any proposed solar energy system on a federally-obligated airport. This
is shown in the figure below.
Solar Photovoltaic Glint and Glare Study Richard Thomas and Co - Morfa Pingett - Solar Development 58
Solar Glare Hazard Analysis Plot (FAA)
• No potential for glint or glare in the existing or planned Airport Traffic Control Tower
(ATC) cab, and
• No potential for glare or ‘‘low potential for after-image’’ … along the final approach
path for any existing landing threshold or future landing thresholds (including any
planned interim phases of the landing thresholds) as shown on the current FAA-
approved Airport Layout Plan (ALP). The final approach path is defined as two (2)
miles from fifty (50) feet above the landing threshold using a standard three (3) degree
glidepath.
• Ocular impact must be analysed over the entire calendar year in one (1) minute intervals from
when the sun rises above the horizon until the sun sets below the horizon.
The two bullets highlighted above state there should be ‘no potential for glare’ at that ATC
Tower and ‘no’ or ‘low potential for glare’ on the approach paths.
Solar Photovoltaic Glint and Glare Study Richard Thomas and Co - Morfa Pingett - Solar Development 59
Air Navigation Order (ANO) 2009
In some instances, an aviation stakeholder can refer to the ANO 2009 with regard to
safeguarding. Key points from the document are presented below.
Endangering safety of an aircraft
137. A person must not recklessly or negligently act in a manner likely to endanger an aircraft, or
any person in an aircraft.
Lights liable to endanger
221.
(1) A person must not exhibit in the United Kingdom any light which—
(a) by reason of its glare is liable to endanger aircraft taking off from or landing at an
aerodrome; or
(b) by reason of its liability to be mistaken for an aeronautical ground light is liable to endanger
aircraft.
(2) If any light which appears to the CAA to be a light described in paragraph (1) is exhibited, the
CAA may direct the person who is the occupier of the place where the light is exhibited or who
has charge of the light, to take such steps within a reasonable time as are specified in the
direction—
(a) to extinguish or screen the light; and
(b) to prevent in the future the exhibition of any other light which may similarly endanger
aircraft.
(3) The direction may be served either personally or by post, or by affixing it in some conspicuous
place near to the light to which it relates.
(4) In the case of a light which is or may be visible from any waters within the area of a general
lighthouse authority, the power of the CAA under this article must not be exercised except with
the consent of that authority.
Lights which dazzle or distract
222. A person must not in the United Kingdom direct or shine any light at any aircraft in flight so
as to dazzle or distract the pilot of the aircraft.’
The document states that no ‘light’, ‘dazzle’ or ‘glare’ should be produced which will create a
detrimental impact upon aircraft safety.
Solar Photovoltaic Glint and Glare Study Richard Thomas and Co - Morfa Pingett - Solar Development 60
APPENDIX B – OVERVIEW OF GLINT AND GLARE STUDIES
Overview
Studies have been undertaken assessing the type and intensity of solar reflections from various
surfaces including solar panels and glass. An overview of these studies is presented below.
The guidelines presented are related to aviation safety. The results are applicable for the purpose
of this analysis.
Reflection Type from Solar Panels
Based on the surface conditions reflections from light can be specular and diffuse. A specular
reflection has a reflection characteristic similar to that of a mirror; a diffuse will reflect the
incoming light and scatter it in many directions. The figure below, taken from the FAA
guidance19, illustrates the difference between the two types of reflections. Because solar panels
are flat and have a smooth surface most of the light reflected is specular, which means that
incident light from a specific direction is reradiated in a specific direction.
Specular and diffuse reflections
19Source: Technical Guidance for Evaluating Selected Solar Technologies on Airports, Federal Aviation Administration,
November 2010.
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Solar Reflection Studies
An overview of content from identified solar panel reflectivity studies is presented in the
subsections below.
Evan Riley and Scott Olson, “A Study of the Hazardous Glare Potential to Aviators from
Utility-Scale Flat-Plate Photovoltaic Systems”
Evan Riley and Scott Olson published in 2011 their study titled: A Study of the Hazardous Glare
Potential to Aviators from Utility-Scale Flat-Plate Photovoltaic Systems20”. They researched the
potential glare that a pilot could experience from a 25 degree fixed tilt PV system located outside
of Las Vegas, Nevada. The theoretical glare was estimated using published ocular safety metrics
which quantify the potential for a postflash glare after-image. This was then compared to the
postflash glare after-image caused by smooth water. The study demonstrated that the
reflectance of the solar cell varied with angle of incidence, with maximum values occurring at
angles close to 90 degrees. The reflectance values varied from approximately 5% to 30%. This is
shown on the figure below.
Total reflectance % when compared to angle of incidence
The conclusions of the research study were:
• The potential for hazardous glare from flat-plate PV systems is similar to that of smooth
water;
20 Evan Riley and Scott Olson, “A Study of the Hazardous Glare Potential to Aviators from Utility-Scale Flat-Plate
Photovoltaic Systems,” ISRN Renewable Energy, vol. 2011, Article ID 651857, 6 pages, 2011. doi:10.5402/2011/651857
Solar Photovoltaic Glint and Glare Study Richard Thomas and Co - Morfa Pingett - Solar Development 62
• Portland white cement concrete (which is a common concrete for runways), snow, and
structural glass all have a reflectivity greater than water and flat plate PV modules.
FAA Guidance- “Technical Guidance for Evaluating Selected Solar Technologies on
Airports”21
The 2010 FAA Guidance included a diagram which illustrates the relative reflectance of solar
panels compared to other surfaces. The figure shows the relative reflectance of solar panels
compared to other surfaces. Surfaces in this figure produce reflections which are specular and
diffuse. A specular reflection (those made by most solar panels) has a reflection characteristic
similar to that of a mirror. A diffuse reflection will reflect the incoming light and scatter it in many
directions. A table of reflectivity values, sourced from the figure within the FAA guidance, is
presented below.
Surface Approximate Percentage of Light Reflected22
Snow 80
White Concrete 77
Bare Aluminium 74
Vegetation 50
Bare Soil 30
Wood Shingle 17
Water 5
Solar Panels 5
Black Asphalt 2
Relative reflectivity of various surfaces
Note that the data above does not appear to consider the reflection type (specular or diffuse).
An important comparison in this table is the reflectivity compared to water which will produce
a reflection of very similar intensity when compared to that from a solar panel. The study by
21 Source: Technical Guidance for Evaluating Selected Solar Technologies on Airports, Federal Aviation Administration,
November 2010. 22 Extrapolated data, baseline of 1,000 W/m2 for incoming sunlight.
Solar Photovoltaic Glint and Glare Study Richard Thomas and Co - Morfa Pingett - Solar Development 63
Riley and Olsen study (2011) also concludes that still water has a very similar reflectivity to solar
panels.
SunPower Technical Notification (2009)
SunPower published a technical notification23 to ‘increase awareness concerning the possible
glare and reflectance impact of PV Systems on their surrounding environment’.
The figure presented below shows the relative reflectivity of solar panels compared to other
natural and manmade materials including smooth water, standard glass and steel.
Common reflective surfaces
The results, similarly to those from Riley and Olsen study (2011) and the FAA (2010), show that
solar panels produce a reflection that is less intense than those of ‘standard glass and other
common reflective surfaces’.
With respect to aviation and solar reflections observed from the air, SunPower has developed
several large installations near airports or on Air Force bases. It is stated that these developments
have all passed FAA or Air Force standards with all developments considered “No Hazard to Air
Navigation”. The note suggests that developers discuss any possible concerns with stakeholders
near proposed solar farms.
23 Source: Technical Support, 2009. SunPower Technical Notification – Solar Module Glare and Reflectance.
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APPENDIX C – OVERVIEW OF SUN MOVEMENTS AND RELATIVE
REFLECTIONS
The Sun’s position in the sky can be accurately described by its azimuth and elevation. Azimuth
is a direction relative to true north (horizontal angle i.e. from left to right) and elevation describes
the Sun’s angle relative to the horizon (vertical angle i.e. up and down).
The Sun’s position can be accurately calculated for a specific location. The following data being
used for the calculation:
• Time;
• Date;
• Latitude;
• Longitude.
The combination of the Sun’s azimuth angle and vertical elevation will affect the direction and
angle of the reflection from a reflector.
The following is true at the location of the solar development:
• The Sun is at its highest around midday and is to the south at this time;
• The Sun rises highest on 21 June reaching a maximum elevation of approximately 60-
65 degrees (longest day);
• On 21 December, the maximum elevation reached by the Sun is approximately 10-
15 degrees (shortest day).
The combination of the Sun’s azimuth angle and vertical elevation will affect the direction and
angle of the reflection from a reflector. The figure on the following page shows terrain at the
horizon as well as the sunrise and sunset curves throughout the year.
Solar Photovoltaic Glint and Glare Study Richard Thomas and Co - Morfa Pingett - Solar Development 65
Terrain Sun Curve - From lon: -4.298671 lat: 51.721264
Solar Photovoltaic Glint and Glare Study Richard Thomas and Co - Morfa Pingett - Solar Development 66
APPENDIX D – GLINT AND GLARE IMPACT SIGNIFICANCE
Overview
The significance of glint and glare will vary for different receptors. The following section presents
a general overview of the significance criteria with respect to experiencing a solar reflection.
Impact Significance Definition
The table below presents the recommended definition of ‘impact significance’ in glint and glare
terms and the requirement for mitigation under each.
Impact
Significance Definition Mitigation Requirement
No Impact
A solar reflection is not geometrically
possible or will not be visible from the
assessed receptor.
No mitigation required.
Low
A solar reflection is geometrically
possible however any impact is
considered to be small such that
mitigation is not required e.g.
intervening screening will limit the
view of the reflecting solar panels.
No mitigation required.
Moderate
A solar reflection is geometrically
possible and visible however it occurs
under conditions that do not represent
a worst-case.
Whilst the impact may be
acceptable, consultation
and/or further analysis should
be undertaken to determine
the requirement for mitigation.
Major
A solar reflection is geometrically
possible and visible under conditions
that will produce a significant impact.
Mitigation and consultation is
recommended.
Mitigation will be required if
the proposed development is
to proceed.
Impact significance definition
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The flow charts presented in the following sub-sections have been followed when determining
the mitigation requirement for roads and aviation receptors.
Assessment Process for Road Receptors
The flow chart presented below has been followed when determining the mitigation
requirement for road receptors.
Road receptor mitigation requirement flow chart
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Assessment Process – ATC Tower
The charts relate to the determining the potential impact upon the ATC Tower.
ATC Tower mitigation requirement flow chart
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Assessment Process – Approaching Aircraft
The charts relate to the determining the potential impact upon approaching aircraft.
Approaching aircraft receptor mitigation requirement flow chart
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APPENDIX E – PAGER POWER’S REFLECTION CALCULATIONS
METHODOLOGY
The calculations are three dimensional and complex, accounting for:
• The Earth’s orbit around the Sun;
• The Earth’s rotation;
• The Earth’s orientation;
• The reflector’s location;
• The reflector’s 3D Orientation.
Reflections from a flat reflector are calculated by considering the normal which is an imaginary
line that is perpendicular to the reflective surface and originates from it. The diagram below may
be used to aid understanding of the reflection calculation process.
Illustration of calculation process
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The following process is used to determine the 3D Azimuth and Elevation of a reflection:
• Use the Latitude and Longitude of reflector as the reference for calculation purposes;
• Calculate the Azimuth and Elevation of the normal to the reflector;
• Calculate the 3D angle between the source and the normal;
• If this angle is less than 90 degrees a reflection will occur. If it is greater than 90 degrees
no reflection will occur because the source is behind the reflector;
• Calculate the Azimuth and Elevation of the reflection in accordance with the following:
o The angle between source and normal is equal to angle between normal and
reflection;
o Source, Normal and Reflection are in the same plane.
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APPENDIX F – ASSESSMENT LIMITATIONS AND ASSUMPTIONS
Pager Power’s Model
It is assumed that the panel elevation angle provided by the developer represents the elevation
angle for all of the panels within the solar development.
It is assumed that the panel azimuth angle provided by the developer represents the azimuth
angle for all of the panels within the solar development.
Only a reflection from the face of the panel has been considered. The frame or the reverse of
the solar panel has not been considered.
The model assumes that a receptor can view the face of every panel within the proposed
development area whilst in reality this, in the majority of cases, will not occur.
Therefore any predicted reflection from the face of a solar panel that is not visible to a receptor
will not occur.
A finite number of points within the proposed development are chosen based on an assessment
resolution so we can build a comprehensive understanding of the entire development. This will
determine whether a reflection could ever occur at a chosen receptor. The calculations do not
incorporate all of the possible panel locations within the development outline.
A single reflection point on the panel has been chosen for the geometric calculations. This will
suitably determine whether a reflection can be experienced at a location and the general time
of year and duration of this reflection. Increased accuracy could be achieved by increasing the
number of heights assessed however this would only marginally change the results and is not
considered significant.
Whilst line of sight to the development from receptors has been considered, only available street
view imagery and satellite mapping has been used. In some cases this imagery may not be up
to date and may not give the full perspective of the installation from the location of the assessed
receptor.
Any screening in the form of trees, buildings etc. that may obstruct the Sun from view of the
solar panels is not considered unless stated.
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Sandia National Laboratories’ (SGHAT) Model
The following text is taken from the Solar Glare Hazard Analysis Tool (SGHAT) Technical
Reference Manual24 which was previously freely available. The following is presented for
reference.
24 https://share.sandia.gov/phlux/static/references/glint-glare/SGHAT_Technical_Reference-v5.pdf
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APPENDIX G – COORDINATE DATA
Roads receptors
The table below presents the assessed roads’ receptor locations (A484 and local road southern
border). All the road receptors were considered at a height of 1.5 metre.
ID Longitude (°) Latitude (°) Ground
Elevation (amsl)
Overall height
(amsl)
01 -4.30126 51.72294 2.0 3.5
02 -4.30118 51.72248 2.0 3.5
03 -4.3011 51.72204 2.9 4.4
04 -4.30103 51.7216 3.0 4.5
05 -4.30096 51.72117 3.0 4.5
06 -4.30091 51.7207 3.0 4.5
07 -4.30086 51.72024 3.0 4.5
08 -4.30081 51.7198 3.0 4.5
09 -4.30025 51.72097 3.0 4.5
10 -4.29956 51.72081 2.8 4.3
11 -4.29889 51.72066 3.0 4.5
12 -4.29822 51.7205 3.0 4.5
13 -4.29753 51.72034 3.0 4.5
14 -4.29686 51.72019 2.2 3.7
15 -4.29618 51.72003 2.0 3.5
16 -4.29551 51.71987 2.0 3.5
17 -4.29482 51.71971 2.0 3.5
18 -4.29414 51.71955 2.0 3.5
19 -4.29346 51.71939 2.0 3.5
20 -4.29279 51.71923 2.0 3.5
21 -4.29211 51.71907 2.0 3.5
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ID Longitude (°) Latitude (°) Ground
Elevation (amsl)
Overall height
(amsl)
23 -4.29155 51.71893 1.7 3.2
24 -4.29092 51.71879 1.3 2.8
Aviation receptors
ATC tower
Longitude (°) Latitude (°) Ground
Elevation
ATC Tower
Height25
Overall Assessed
Height 26
-4.31081 51.71329 3.0m 5.0m 8.0m
Runways 04 and 22
The table below presents the assessed 2-miles approach for 22 and 04 runaways’ receptor
locations.
ID Longitude
(°)
Latitude
(°)
Height
(amsl) ID
Longitude
(°)
Latitude
(°)
Height
(amsl)
Runway 04 Runway 22
0 -4.31536 51.71086 19.8 0 -4.30922 51.71696 19.5
¼ -4.31845 51.7078 40. 9 ¼ -4.30613 51.72002 40.6
½ -4.32154 51.70473 62.0 ½ -4.30304 51.72309 61.7
¾ -4.32463 51.70167 83.1 ¾ -4.29994 51.72615 82.8
1 -4.32772 51.6986 104.2 1 -4.29685 51.72921 103.8
1 ¼ -4.33081 51.69554 125.2 1 ¼ -4.29376 51.73228 124.9
1 ½ -4.3339 51.69247 146.3 1 ½ -4.29067 51.73534 146.0
1 ¾ -4.33699 51.68941 167.4 1 ¾ -4.28757 51.73841 167.1
2 -4.34007 51.68634 188.5 2 -4.28448 51.74147 188.2
Assessed receptor locations
25 Estimated based on altitude of the ATC tower listed within the AIP and ground level at the tower’s location.
26 Maximum height of the tower is 160m amsl however 3m has been deducted to account for the cab viewing height.
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Modelled Reflector Area
ID Longitude (°) Latitude (°) ID Longitude (°) Latitude (°)
1 -4.300309 51.721105 6 -4.297876 51.720775
2 -4.299903 51.722049 7 -4.298499 51.720882
3 -4.298699 51.721854 8 -4.298461 51.721148
4 -4.297092 51.721704 9 -4.299136 51.721258
5 -4.297431 51.720929 10 -4.299303 51.720938
Modelled reflector area
Image of reflector area
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APPENDIX H – GEOMETRIC CALCULATION RESULTS – PAGER
POWER RESULTS
The charts for the receptors are shown on the following pages. Each chart shows:
• The receptor (observer) location – top right image. This also shows the azimuth range
of the Sun itself at times when reflections are possible. If sunlight is experienced from
the same direction as the reflecting panels, the overall impact of the reflection is reduced
as discussed within the body of the report;
• The reflecting panels – bottom right image. The reflecting area is shown in yellow. If the
yellow panels are not visible from the observer location, no issues will occur in practice.
Additional obstructions which may obscure the panels from view are considered
separately within the analysis;
• The reflection date/time graph – left hand side of the page. The blue line indicates the
dates and times at which geometric reflections are possible. This relates to reflections
from the yellow areas.
Charts are only shown for aircraft approaching runway 22, road A484 receptors 3 – 7 and local
road southern border receptors 9 – 16 as no other reflections are predicted.
Approach 22
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Road A484 receptors
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Road south of development
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