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Institut für Umweltphysik Universität Heidelberg High resolution spectroscopy of the Oxygen A-band in zenith-scattered light; Implications for cloudy sky photon path length T.Scholl, U.Nägele , U.Platt, and K.Pfeilsticker nstitut für Umweltphysik, Universität Heidelberg, INF 229, D-69120 Heidelber Overview: -Instrumentation -Method -Evaluation Example -Summary / Outlook

Institut für Umweltphysik Universität Heidelberg High resolution spectroscopy of the Oxygen A-band in zenith-scattered light; Implications for cloudy sky

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Page 1: Institut für Umweltphysik Universität Heidelberg High resolution spectroscopy of the Oxygen A-band in zenith-scattered light; Implications for cloudy sky

Institut für Umweltphysik Universität Heidelberg

High resolution spectroscopy of the Oxygen A-band in zenith-scattered light; Implications for cloudy sky photon

path length

T.Scholl, U.Nägele , U.Platt, and K.Pfeilsticker

Institut für Umweltphysik, Universität Heidelberg, INF 229, D-69120 Heidelberg

Overview:

-Instrumentation

-Method

-Evaluation Example

-Summary / Outlook

Page 2: Institut für Umweltphysik Universität Heidelberg High resolution spectroscopy of the Oxygen A-band in zenith-scattered light; Implications for cloudy sky

Institut für Umweltphysik Universität Heidelberg

Setup / Geometry

ANDO R C C D C AM ERA(2048 x 512 p ixe l)

Ground

v

FOV = 1°

RT SmoothingH

H

H: vertical cloud extension

Short integration time required:

Previous measurements: 900 sec

BBC measurements: ~ 2 sec

Page 3: Institut für Umweltphysik Universität Heidelberg High resolution spectroscopy of the Oxygen A-band in zenith-scattered light; Implications for cloudy sky

Institut für Umweltphysik Universität Heidelberg

Spectrograph CCD Detector

•Sopra UHRS 1500 Fastie-Ebert

•F = 1500 mm

•110 x 220 mm2, 316 g/mm Echelle

•f/13.5

•Temp. const. +/- 1K

•ca. 500 kg

Resolution(@770nm): 9.6 pm (5ch, 1.93pm/ch)

Spectral Range: ca. 4 nm

•2048x512 pixel

•27.6 x 6.9 mm2 (13.5 m)

•QE ca. 45% @ 770nm

•R/O noise 2e-/pixel

•FI, Marconi (EEV)

•TE cooling –90°C

Page 4: Institut für Umweltphysik Universität Heidelberg High resolution spectroscopy of the Oxygen A-band in zenith-scattered light; Implications for cloudy sky

Institut für Umweltphysik Universität Heidelberg

Setup / Geometry

ANDO R C C D C AM ERA(2048 x 512 p ixe l)

Ground

v

FOV = 1°

RT SmoothingH

H

H: vertical cloud extension

Short integration time required:

Previous measurements: 900 sec

BBC measurements: ~ 2 sec

Page 5: Institut für Umweltphysik Universität Heidelberg High resolution spectroscopy of the Oxygen A-band in zenith-scattered light; Implications for cloudy sky

Institut für Umweltphysik Universität Heidelberg

Radiative Smoothing Scales

08:00 10:00 12:00 14:000

1x104

2x104

3x104

4x104

5x104

6x104a) October 08, 98

-1 1 3 5 7 9 11 13 15

2-12

2-10

2 -8

2 -6

2 -4

2 -2

20

L = 17-25 kmSmoothing

regime

Large scale

regime

Intermediate

regime

=1.64

2=0.48

a) October 08, 98

<|

(r

;n)|

2>

2 22 2 2 2 2 2 2

Savigny et al. , 2002Scale parameter rTime (UTC)

Radiometer HDRAD (760nm)

Page 6: Institut für Umweltphysik Universität Heidelberg High resolution spectroscopy of the Oxygen A-band in zenith-scattered light; Implications for cloudy sky

Institut für Umweltphysik Universität Heidelberg

Lévy Indices

 

α: Lévy (transport) index; α = 1 direct transmission, 1< α < 2 anomalous diffusion, α = 2 classical diffusion  Observables are: <L> (oxygen A band spectroscopy), H radar/Lidar, Inferred quantities: τ and α  

ergo transport index α (describing a mean) can be inferred !

11

11

HL

MFP

Lgg

HMFP

Page 7: Institut für Umweltphysik Universität Heidelberg High resolution spectroscopy of the Oxygen A-band in zenith-scattered light; Implications for cloudy sky

Institut für Umweltphysik Universität Heidelberg

Inferred Lévy Indices(Pfeilsticker, JGR, 1999)

Page 8: Institut für Umweltphysik Universität Heidelberg High resolution spectroscopy of the Oxygen A-band in zenith-scattered light; Implications for cloudy sky

Institut für Umweltphysik Universität Heidelberg

Measurement

768.0 768.5 769.0 769.5 770.0 770.50.0

0.2

0.4

0.6

0.8

1.0

K I

Mg ISi I

Tra

nsm

issi

on

Wavelength (nm)

Sept.17, 2001 10:30:32 UTC

=14 pm, integration time = 1.5 sec

- Data available from Sept.6 – 25, 2001- ~ 150.000 spectra were measured (~9GB)- Integration time ranging from 0.5 - 5 sec (variable light intensity)

Page 9: Institut für Umweltphysik Universität Heidelberg High resolution spectroscopy of the Oxygen A-band in zenith-scattered light; Implications for cloudy sky

Institut für Umweltphysik Universität Heidelberg

Data Analysis

High Spectral Resolution

Searched quantityp(l) ?

Spectrum

Measurement withgiven spectral

resolution

Measured Spectrum

Nonlinear Least

Square Fit (10min, 1GHz)

Modeled Spectrum

Spectroscopic Model Temp., Pressure Profile

x T(p(aj), i ( )

Solar Fraunhofer p(l) Model Oxygen Absorption Spectrum Lines (VOD)

Low Spectral ResolutionBest estimate p(l)

Convolution with instrument function

768.0 768.5 769.0 769.5 770.0 770.5 771.0 771.50.0

0.2

0.4

0.6

0.8

1.0

Ni I

(?)

Ni I

Co

IF

e II

Fe

I

K I

Si I

Si I

Mg

I

Si I

Si IS

i IC I

Si I

I 0

Wavelength / nm

-1.5 -1.0 -0.5 0.0 0.5 1.0 1.50

10

20

30

40

50

60

70

767.20 767.25 767.30 767.35 767.40 767.45 767.500.00E+000

2.00E-024

4.00E-024

6.00E-024

Wavelength (nm)

Page 10: Institut für Umweltphysik Universität Heidelberg High resolution spectroscopy of the Oxygen A-band in zenith-scattered light; Implications for cloudy sky

Institut für Umweltphysik Universität Heidelberg

Evaluation Example

768.0 768.5 769.0 769.5 770.0 770.50.0

0.2

0.4

0.6

0.8

1.0

Tra

nsm

issio

n

Wavelength (nm)

MEASUREMENT Model (Fit)

768.0 768.5 769.0 769.5 770.0 770.5

-0.02

-0.01

0.00

0.01

0.02

0.03

0.04

Re

sid

ua

l

Wavelength (nm)

Model

Residual

Page 11: Institut für Umweltphysik Universität Heidelberg High resolution spectroscopy of the Oxygen A-band in zenith-scattered light; Implications for cloudy sky

Institut für Umweltphysik Universität Heidelberg

Sensitivity Test

1 2 3 4 5 6 7

0.0

0.5

1.0

1.5

2.0

2.5

?

?

model: Gamma <l> = 2.615 +/- 0.039

<l2> = 9.177 +/- 0.717<l> = 2.682 +/- 0.038

<l2> = 7.227 +/- 0.223p(l

)

Pathlengths l

free Fraunhofercoefficient fixed Fraunhofercoefficient

768.0 768.5 769.0 769.5 770.0 770.5

-0.03

-0.02

-0.01

0.00

0.01

0.02

0.03

0.04

Re

sid

ua

l

Wavelength (nm)

Page 12: Institut für Umweltphysik Universität Heidelberg High resolution spectroscopy of the Oxygen A-band in zenith-scattered light; Implications for cloudy sky

Institut für Umweltphysik Universität Heidelberg

Summary

• Spectral retrieval software works, but needs some improvements (wavelength dependent convolution)

• Better time resolution (15 min few seconds) and better spectroscopical resolution ( 20pm 9.5 pm)

• Better understanding and sensitivity test for retrieval method necessary • Determination of <L>, <L2>, ...• Combination with , LWC, H, ...• ..............

Outlook