کد مقاله | کد نشریه | سال انتشار | مقاله انگلیسی | نسخه تمام متن |
---|---|---|---|---|
10705420 | 1022370 | 2005 | 8 صفحه PDF | دانلود رایگان |
عنوان انگلیسی مقاله ISI
A solar spectrum for PFS data analysis
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موضوعات مرتبط
مهندسی و علوم پایه
علوم زمین و سیارات
فیزیک زمین (ژئو فیزیک)
پیش نمایش صفحه اول مقاله
![عکس صفحه اول مقاله: A solar spectrum for PFS data analysis A solar spectrum for PFS data analysis](/preview/png/10705420.png)
چکیده انگلیسی
A measured calibrated solar radiance in the range 1.2-5μm, with the spectral sampling of 1cm-1 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-1), 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.
ناشر
Database: Elsevier - ScienceDirect (ساینس دایرکت)
Journal: Planetary and Space Science - Volume 53, Issue 10, August 2005, Pages 1009-1016
Journal: Planetary and Space Science - Volume 53, Issue 10, August 2005, Pages 1009-1016
نویسندگان
Carlo Fiorenza, Vittorio Formisano,