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@ARTICLE{Kaufmann:842032,
author = {Kaufmann, Martin and Olschewski, Friedhelm and Mantel,
Klaus and Solheim, Brian and Shepherd, Gordon and Deiml,
Michael and Liu, Jilin and Song, Rui and Chen, Qiuyu and
Wroblowski, Oliver and Wei, Daikang and Zhu, Yajun and
Wagner, Friedrich and Loosen, Florian and Froehlich, Denis
and Neubert, Tom and Rongen, Heinz and Knieling, Peter and
Toumpas, Panos and Shan, Jinjun and Tang, Geshi and
Koppmann, Ralf and Riese, Martin},
title = {{A} highly miniaturized satellite payload based on a
spatial heterodyne spectrometer for atmospheric temperature
measurements in the mesosphere and lower thermosphere},
journal = {Atmospheric measurement techniques discussions},
volume = {437},
issn = {1867-8610},
address = {Katlenburg-Lindau},
publisher = {Copernicus},
reportid = {FZJ-2018-00316},
pages = {1 - 19},
year = {2017},
abstract = {A highly miniaturized limb sounder for the observation of
the O2 A-Band to derive temperatures in the mesosphere and
lower thermosphere is presented. The instrument consists of
a monolithic spatial heterodyne spectrometer (SHS), which is
able to resolve the rotational structure of the R-branch of
that band. The relative intensities of the emission lines
follow a Boltzmann distribution and the ratio of the lines
can be used to derive the kinetic temperature. The SHS
operates at a Littrow wavelength of 761.8 nm and
heterodynes a wavelength regime between 761.9 nm and
765.3 nm with a resolving power of about 8000 considering
apodization effects. The size of the SHS is
38 × 38 × 27 mm3 and its acceptance angle is
±5°. It has an etendue of 0.014 cm2 sr. Complemented
by a front optics with a solid angle of 0.65° and a
detector optics, the entire optical system fits into a
volume of about 1.5 liters. This allows to fly this
instrument on a 3 or 6 unit CubeSat. The vertical field of
view of the instrument is about 60 km at the Earth's limb
if operated in a typical low Earth orbit. Integration times
to obtain an entire altitude profile of nighttime
temperatures are in the order of one minute for a vertical
resolution of 1.5 km and a random noise level of 1.5 K.
Daytime integration times are one order of magnitude
shorter. This work presents the design parameters of the
optics and a radiometric assessment of the instrument.
Furthermore it gives an overview of the required
characterization and calibration steps. This includes the
characterization of image distortions in the different parts
of the optics, flat fielding and the spectral power
estimation.},
cin = {IEK-7},
ddc = {550},
cid = {I:(DE-Juel1)IEK-7-20101013},
pnm = {244 - Composition and dynamics of the upper troposphere and
middle atmosphere (POF3-244) / HITEC - Helmholtz
Interdisciplinary Doctoral Training in Energy and Climate
Research (HITEC) (HITEC-20170406)},
pid = {G:(DE-HGF)POF3-244 / G:(DE-Juel1)HITEC-20170406},
typ = {PUB:(DE-HGF)16},
doi = {10.5194/amt-2017-437},
url = {https://juser.fz-juelich.de/record/842032},
}