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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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發(fā)表于 2025-3-21 16:24:15 | 只看該作者 |倒序瀏覽 |閱讀模式
書目名稱Cross-Calibration of Far UV Spectra of Solar System Objects and the Heliosphere
編輯Eric Quémerais,Martin Snow,Roger-Maurice Bonnet
視頻videohttp://file.papertrans.cn/241/240271/240271.mp4
概述Discusses various fields of Far UV spectroscopy, ranging from a catalog of stellar spectra to detailed modeling and measurements of the interplanetary background.Presents various types of data sets an
叢書名稱ISSI Scientific Report Series
圖書封面Titlebook: Cross-Calibration of Far UV Spectra of Solar System Objects and the Heliosphere;  Eric Quémerais,Martin Snow,Roger-Maurice Bonnet Book 2013
描述This book is the result of a working group sponsored by ISSI in Bern, which was initially created to study possible ways to calibrate a Far Ultraviolet (FUV) instrument after launch. In most cases, ultraviolet instruments are well calibrated on the ground, but unfortunately, optics and detectors in the FUV are very sensitive to contaminants and it is very challenging to prevent contamination before and during the test and launch sequences of a space mission. Therefore, ground calibrations need to be confirmed after launch and it is necessary to keep track of the temporal evolution of the sensitivity of the instrument during the mission. .The studies presented here cover various fields of FUV spectroscopy, including a catalog of stellar spectra, datasets of Moon Irradiance, observations of comets and measurements of the interplanetary background. Detailed modelling of the interplanetary background 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
出版日期Book 2013
關鍵詞Lyman-alpha Comet Holmes; Lyman-alpha Models; Modeling Interplanetary Background; Moon Irradiance; UV Sp
版次1
doihttps://doi.org/10.1007/978-1-4614-6384-9
isbn_softcover978-1-4939-4709-6
isbn_ebook978-1-4614-6384-9Series ISSN 2946-1278 Series E-ISSN 2946-1286
issn_series 2946-1278
copyrightSpringer Science+Business Media New York 2013
The information of publication is updating

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沙發(fā)
發(fā)表于 2025-3-21 23:42:23 | 只看該作者
ISSI Scientific Report Serieshttp://image.papertrans.cn/d/image/240271.jpg
板凳
發(fā)表于 2025-3-22 03:53:03 | 只看該作者
Cross-Calibration of Far UV Spectra of Solar System Objects and the Heliosphere978-1-4614-6384-9Series ISSN 2946-1278 Series E-ISSN 2946-1286
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發(fā)表于 2025-3-22 07:59:18 | 只看該作者
Theoretical Foundations of the Welfare State accuracy that can be achieved, and review the different sources of emissions that can be used in that range, i.e. the interplanetary background, stars, and solar system bodies such as planets, moons, and comets. As most of the work presented here is based on comparisons with older datasets obtained
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發(fā)表于 2025-3-22 10:57:32 | 只看該作者
Summarized Findings and Conclusionhe atoms penetrate through the region of the solar wind (SW) interaction with the local interstellar medium (LISM). In the interaction region the atoms can exchange charge with both solar wind and interstellar protons disturbed in the SW/LISM interaction region. Charge exchange results in a disturba
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發(fā)表于 2025-3-23 01:08:20 | 只看該作者
Beschreibung deutscher Unternehmen in China,planetary Lyman-. data obtained in 2009–2011 on the MErcury Surface, Space ENvironment, GEochemistry, and Ranging (MESSENGER) spacecraft mission, daily all-sky Lyman-. maps were generated for use by the Lunar Reconnaissance Orbiter (LRO) LAMP Lyman-Alpha Mapping Project (LAMP) experiment. These mode
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發(fā)表于 2025-3-23 04:14:31 | 只看該作者
Beschreibung deutscher Unternehmen in China,olet spectrograph on the New Horizons spacecraft (the first new such data from outside the orbit of Saturn since the Voyager spacecraft). The observations consist of 6. ×360. great-circle swaths on the sky, centered on the ecliptic direction λ = 51. 3., . = 44. 8., which passes within ~ 33. of the u
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發(fā)表于 2025-3-23 05:35:51 | 只看該作者
,Auff?lligkeiten in H?ufigkeitsverteilungen, the ultraviolet (115–300 nm). Prior to launch, it was calibrated at the SURF-III synchrotron. Spectra from the International Ultraviolet Explorer (IUE) corrected to the white dwarf flux scale are in good agreement with SOLSTICE observations, validating the two completely independent methods of cali
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