uv-vis remote sensing instruments nasa/goddard space

22
UV-Vis remote sensing instruments - From L0 to L1 Alexander Cede LuftBlick, Austria NASA/Goddard Space Flight Center, USA

Upload: others

Post on 07-Jan-2022

2 views

Category:

Documents


0 download

TRANSCRIPT

UV-Vis remote sensing instruments

- From L0 to L1

Alexander CedeLuftBlick, Austria

NASA/Goddard Space Flight Center, USA

ESA-EUM, 2 School and Atmospheric Composition, 19 November 2020

From photons to digital number

Readout electronics (ROE)

Telescope

Fiber optics

Spectrometer

ESA-EUM, 2 School and Atmospheric Composition, 19 November 2020

L0 to L1 correction steps

ESA-EUM, 2 School and Atmospheric Composition, 19 November 2020

Dark correction

ESA-EUM, 2 School and Atmospheric Composition, 19 November 2020

Effect of Dark correction

Spectrum shown in this presentation is direct sun at noon (SZA=56°) on 17 Oct 2019 at Innsbruck.

ESA-EUM, 2 School and Atmospheric Composition, 19 November 2020

Non linearity

ESA-EUM, 2 School and Atmospheric Composition, 19 November 2020

Effect of Non-linearity correction

ESA-EUM, 2 School and Atmospheric Composition, 19 November 2020

Latency

ESA-EUM, 2 School and Atmospheric Composition, 19 November 2020

Latency

ESA-EUM, 2 School and Atmospheric Composition, 19 November 2020

Effect of latency correction

ESA-EUM, 2 School and Atmospheric Composition, 19 November 2020

Pixel response non uniformity

ESA-EUM, 2 School and Atmospheric Composition, 19 November 2020

Conversion to count rates

ESA-EUM, 2 School and Atmospheric Composition, 19 November 2020

Temperature correction

ESA-EUM, 2 School and Atmospheric Composition, 19 November 2020

Stray light correction

Slit function looks tame on the linear scale, but reveals all kind of structures on the log scale → spectral stray light

ESA-EUM, 2 School and Atmospheric Composition, 19 November 2020

Stray light correction

ESA-EUM, 2 School and Atmospheric Composition, 19 November 2020

Full slit function

Video compiled and thankfully provided by● Julian Gröbner and● Natalia Kouremeti

ESA-EUM, 2 School and Atmospheric Composition, 19 November 2020

Effect of Stray light correction

ESA-EUM, 2 School and Atmospheric Composition, 19 November 2020

Spectral Sensitivity

●●●●

ESA-EUM, 2 School and Atmospheric Composition, 19 November 2020

Effect of Sensitivity correction

ESA-EUM, 2 School and Atmospheric Composition, 19 November 2020

Wavelength correction

●squeeze

shift

Solar reference

ESA-EUM, 2 School and Atmospheric Composition, 19 November 2020

Effect of Wavelength correction

Here the wavelength shift was about 0.01nm.

ESA-EUM, 2 School and Atmospheric Composition, 19 November 2020

From photons to digital number

Readout electronics (ROE)

Telescope

Fiber optics

Spectrometer