Upload
prue
View
78
Download
1
Tags:
Embed Size (px)
DESCRIPTION
GNSS ionosphere research activities at FCT/UNESP João Francisgo Galera Monico , Paulo De Oliveira Camargo FCT/UNESP - Presidente Prudente , SP. Outline. Introduction Developments on GNSS/Ionosphere Brazilian Ionospheric Model Mod_ION Mod_ION_FK /IG Rinex_HO GNSS demands in Brazil - PowerPoint PPT Presentation
Citation preview
GNSS ionosphere research activities at FCT/UNESP
João Francisgo Galera Monico, Paulo De Oliveira Camargo
FCT/UNESP - Presidente Prudente, SP.
Outline• Introduction• Developments on GNSS/Ionosphere
– Brazilian Ionospheric Model• Mod_ION• Mod_ION_FK/IG• Rinex_HO
• GNSS demands in Brazil• CIGALA & CALIBRA Projects• Final Comments
Ionosphere and GNSS• Ionospheric effects (delay and frequency dispersion & phase
scintillation and amplitude fading) are one of the main barriers to achieve high accuracy GNSS positioning and navigation.
• It affects the quality of positioning and navigation: PPP, relative carrier phase based positioning, DGNSS, GBAS and SBAS, mainly for users of one frequency receiver.
• Measurements made on two different frequencies allow the correction of the first order ionospheric delay by means of the widely used ionospheric-free linear combination (2nd order still has to be corrected).
Ionosphere and GNSS• Effects as ionospheric scintillations, may cause problems
such as:– signal power fading, – phase cycle slips, – receiver loss of lock, etc.,
• Such effects degrade the position quality provided by the satellite navigation systems (GNSS). This problem is still to be solved !
Developments on GNSS/Ionosphere at FCT/UNESP
• A Ion-model based on GNSS data has been under development since 1997;–Mod_Ion (in-house iono model) initially generated
coefficients for L1 users (Camargo et al., 2000)
• Mod_Ion expanded to generate Ionex files and Ionospheric maps from Brazilian GNSS data
• Real time: Mod_Ion_FK to generate the biases and a IG with respective GIVE are provided (Aguiar 2010).
n 4 m 4s s s s s s
1 2 j j 1 n*2 3 j j 1i 1 i 1j 2i 1 j 2i 10
VTEC a a B {a cos(i h ) a sin(i h )} a h {a cos(i B ) a sin(i B )}
2 2 2i 2i 1i 2iF f /(f f )
n 4s s s s s s s2 1 r r 1 2 j j 1 n*2 3
i 1j 2i 1
m 4s s s s
j j 1 P2 P1 r P2 P1 P21i 1j 2i 10
F(P P ) SF (a a B {a cos(i h ) a sin(i h )} a h
{a cos(i B ) a sin(i B )} F(R R ) F(S S ) F .
TEC s s TEC s s TECi 2r 1r i p2 p1 p2 p1 r i P21s
r
VTECF (P P ) + F [(S -S ) + (R -R ) ] + Fcos(z )
MOD_Ion - Fundamental (GPS & GLONASS)
Mod_Ion with inequality equation
• Problem: at some situations, even with calibrated equipments, negative values of TEC may be obtained.
• One solution: to apply inequality equation as follows:n 4
s s s1 2 j j 1
i 1j 2i 1
m 4s s s
n*2 3 j j 1 i 1j 2i 10
VTEC a a B {a cos(i h ) a sin(i h )}
a h {a cos(i B ) a sin(i B )} 0
GNSS Ionospheric Products
• TEC Maps
-75 -70 -65 -60 -55 -50 -45 -40 -35 -30
Longitude G eográfica (graus) + E stações G PS da RB M C
M apa do VTEC - 06/10/2001 - 01:00 U T
-35
-30
-25
-20
-15
-10
-5
0
5
Latit
ude
Geo
gráf
ica
(gra
us)
VTE
C (x
10E
+16
el/m
2)
0
10
20
30
40
50
60
70
80
90
100
110
120
130
140
BNC
ALDAR
Kalman Filter
Ionosphere Model:Polynomial
Function
Coeficients: dss and drr
Ionosphere Monitoring
dss, drr
VTEC, ROT, IPP
Real time ionosphere maps
GMT
IG & GIVE
Mod_ION_FK/IG (Aguiar, 2010)
BNC
Mod_ION_FK/IG
ALDAR
Kalman Filter
Ionosphere Model:Polynomial
Function
Coeficients: dss and drr
Ionosphere Monitoring
dss, drr
VTEC, ROT, IPP
Real time ionosphere maps
GMT
IG & GIVE
Grid Maps and GIVE/ Brazil
GIVEL1 Ionospheric Delay (m)
• November 22, 2009;• Real time processing;• 29 NTRIP stations.
IONEX Files
2nd and 3rd order Ionosphere corrections• In-house software was developed (RINEX_HO)
• GPS Solutions, Online First: 21 April 2011, DOI: 10.1007/s10291-011-0220-1, "RINEX_HO: second- and third-order ionospheric corrections for RINEX observation files" by H. A. Marques, J. F. G. Monico and M. Aquino
2nd and 3rd order Ionosphere corrections• The earth’s magnetic field
– Dipolar Approximation– International Geomagnetic Reference Field (IGRF) model
(IGRF11 model)– Corrected Geomagnetic Model from PIM (Parameterized
Ionospheric Model)
• TEC– From raw pseudoranges, from pseudoranges smoothed by
phase, or from Global Ionosphere Maps (GIM).
2nd order Ionosphere correctionsDipolar – IGRF and Differences
RECIFE/PE – RECF (28/10/2003)
Ionosphere irregularities Index (Fp )
Estação RECIFE/PE – RECF (21/11/2007)
Ionosphere irregularities Index (Fp )
GNSS demands in Brazil
Off shore applicationsAir Navigation
Positioning in generalPrecision agriculture
Rural Cadastre (50 cm or better – 1 sigma)
….
PA in Brazil is demanding 24 hours RTK service
Concerning Air Navigation, Brazilian authorities decided to invest in GBAS
instead of SBAS.
A system from Honeywell Aerospace is under certification at Rio de Janeiro
Airport (Galeão). (Cosendey presentation on Nov 09).
Challenges for such GNSS applications
Ionospheric Scintillation!
CIGALA Project“Concept for Ionospheric scintillation mitiGAtion for professional GNSS in Latin America”
Goal: Understand the cause and implication of IS disturbances at low latitudes, model their effects and develop mitigations through:– Research of the underlying causes of IS and the development of state-of-the-art models
capable of predicting signal propagation and tracking perturbations– Field measurement via the deployment in close collaboration with local academic and
industrial partners of multi-frequency multi-constellation Ionospheric Scintillation Monitoring (ISM) network
– Design and implementation of novel IS mitigation techniques in state-of-the-art GNSS receivers
– Field testing the mitigation techniques, leveraging the same partnership as during the measurement campaign.
CIGALA partners
CIGALA IS Monitoring Network in Brazil
Continuous recording of :• Amplitude scintillation index S4 : standard deviation of received power
normalized by its mean value• Phase scintillation index σΦ : standard deviation of
de-trended carrier phase, with Phi60 its 60” version• TEC (Total Electron Content)• Lock time• Code – Carrier Divergence• Spectral parameters of phase Power Spectral Density:
– Spectral slope p– Spectral strength T
• Raw high-rate I&Q correlation values (50Hz)
• 8 ISM stations• Latitudinal and longitudinal
distribution over Brazil• Two stations at São José dos
Campos (crest of EIA) and Pres. Prudente
• Data stored locally and sent to repository at UNESP, Pres. Prudente
• Data mirrored at INGV, Rome• Ended on Feb 2012, but the
network is still collecting data.
IS Monitoring Network in Brazil
ISMR Query Tool was developed
CALIBRA PROJECT• A follow up of the CIGALA Project
– Countering GNSS high Accuracy applications Limitations due to Ionospheric disturbances in BRAzil
Focus on high accuracy GNSS
positioning techniques
Better than 10cm
CIGALA/CALIBRA Network• Stations
equipped GNSS receivers PolaRxS-PRO,
• Five new stations will be installed for the CALIBRA Project.
• GNSS/Ionosphere developments at FCT/UNESP were presented;
• Brazil is a very challenge place for GNSS applications, mainly due to the Ionosphere behavior in the equatorial region;
• Several applications have suffered of the effects of such problem (IS);
• In the PA and aviation there is a need for more developments and tests;
• CIGALA/CALIBRA is collecting data that may provide more data for scientific and operational purposes.
Final comments
More information?http://gege.fct.unesp.br