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Titlebook: Cross-Calibration of Far UV Spectra of Solar System Objects and the Heliosphere; Eric Quémerais,Martin Snow,Roger-Maurice Bonnet Book 2013

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樓主: 搖尾乞憐
31#
發(fā)表于 2025-3-26 23:14:32 | 只看該作者
32#
發(fā)表于 2025-3-27 02:44:54 | 只看該作者
33#
發(fā)表于 2025-3-27 08:28:04 | 只看該作者
34#
發(fā)表于 2025-3-27 10:04:18 | 只看該作者
Absolute Ultraviolet Irradiance of the Moon from the LASP Lunar Albedo Measurement and Analysis frommajority of the previous work on characterizing the lunar reflectance has been in the visible part of the spectrum using ground-based lunar images. The SOLar-STellar Irradiance Comparison Experiment (SOLSTICE) on the SOlar Radiation and Climate Experiment (SORCE) can be used to extend the lunar spec
35#
發(fā)表于 2025-3-27 13:38:52 | 只看該作者
Lyman-α Observations of Comet Holmes from SORCE SOLSTICE and SOHO SWANison Experiment (SOLSTICE) on the SOlar Radiation and Climate Experiment (SORCE) both made observations of comet 17P/Holmes at Lyman-α wavelengths. The intent of these observations was to compare the calibration of SWAN and SOLSTICE, rather than to study the properties of comets. The two datasets re
36#
發(fā)表于 2025-3-27 21:13:45 | 只看該作者
Book 2013ackground is presented as well. This work also includes comparisons of older datasets with current ones.? This raises the question of the consistency of the existing datasets. Previous experiments have been calibrated independently and comparison of the datasets may lead to inconsistencies. The auth
37#
發(fā)表于 2025-3-28 01:40:42 | 只看該作者
38#
發(fā)表于 2025-3-28 05:52:02 | 只看該作者
39#
發(fā)表于 2025-3-28 08:34:07 | 只看該作者
Lyman-, Models for LRO LAMP from MESSENGER MASCS and SOHO SWAN Data represents a failure of the model or a decline in sensitivity in SWAN in 2010 and 2011. MESSENGER MASCS and SOHO SWAN Lyman-. calibrations systematically differ in comparison with the model, with MASCS reporting Lyman-. values some 30 % lower than SWAN.
40#
發(fā)表于 2025-3-28 12:46:41 | 只看該作者
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