Physics
Scientific paper
Aug 2005
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005p%26ss...53.1009f&link_type=abstract
Planetary and Space Science, Volume 53, Issue 10, p. 1009-1016.
Physics
16
Scientific paper
A measured calibrated solar radiance in the range 1.2 5μm, with the spectral sampling of 1cm does not exist. When studying the measured Planetary Fourier Spectrometer (PFS) spectra of the Earth's or Mars's atmosphere we discover that the most used solar spectrum contains several important errors. Here we present a “calibrated” solar radiance in the wavelength range 1.2 5μm, with the spectral resolution of PFS (1.3cm), which we are going to use for studying Martian spectra. This spectrum has been assembled using measurements from Kitt Peak and from ATMOS Spacelab experiment (uncalibrated high resolution) and theoretical results, together with low resolution calibrated continuum. This is the best we can have in this moment to be used with PFS, while waiting to have good solar calibrated radiances. Examples of solar lines at Mars are given.
Fiorenza Carlo
Formisano Vittorio
No associations
LandOfFree
A solar spectrum for PFS data analysis does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with A solar spectrum for PFS data analysis, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and A solar spectrum for PFS data analysis will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-797687