找回密碼
 To register

QQ登錄

只需一步,快速開始

掃一掃,訪問微社區(qū)

打印 上一主題 下一主題

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

[復(fù)制鏈接]
查看: 29187|回復(fù): 46
樓主
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(guān)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

書目名稱Cross-Calibration of Far UV Spectra of Solar System Objects and the Heliosphere影響因子(影響力)




書目名稱Cross-Calibration of Far UV Spectra of Solar System Objects and the Heliosphere影響因子(影響力)學(xué)科排名




書目名稱Cross-Calibration of Far UV Spectra of Solar System Objects and the Heliosphere網(wǎng)絡(luò)公開度




書目名稱Cross-Calibration of Far UV Spectra of Solar System Objects and the Heliosphere網(wǎng)絡(luò)公開度學(xué)科排名




書目名稱Cross-Calibration of Far UV Spectra of Solar System Objects and the Heliosphere被引頻次




書目名稱Cross-Calibration of Far UV Spectra of Solar System Objects and the Heliosphere被引頻次學(xué)科排名




書目名稱Cross-Calibration of Far UV Spectra of Solar System Objects and the Heliosphere年度引用




書目名稱Cross-Calibration of Far UV Spectra of Solar System Objects and the Heliosphere年度引用學(xué)科排名




書目名稱Cross-Calibration of Far UV Spectra of Solar System Objects and the Heliosphere讀者反饋




書目名稱Cross-Calibration of Far UV Spectra of Solar System Objects and the Heliosphere讀者反饋學(xué)科排名




單選投票, 共有 0 人參與投票
 

0票 0%

Perfect with Aesthetics

 

0票 0%

Better Implies Difficulty

 

0票 0%

Good and Satisfactory

 

0票 0%

Adverse Performance

 

0票 0%

Disdainful Garbage

您所在的用戶組沒有投票權(quán)限
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
地板
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
5#
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
6#
發(fā)表于 2025-3-22 16:14:54 | 只看該作者
7#
發(fā)表于 2025-3-22 19:34:42 | 只看該作者
8#
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
9#
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
10#
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
 關(guān)于派博傳思  派博傳思旗下網(wǎng)站  友情鏈接
派博傳思介紹 公司地理位置 論文服務(wù)流程 影響因子官網(wǎng) 吾愛論文網(wǎng) 大講堂 北京大學(xué) Oxford Uni. Harvard Uni.
發(fā)展歷史沿革 期刊點評 投稿經(jīng)驗總結(jié) SCIENCEGARD IMPACTFACTOR 派博系數(shù) 清華大學(xué) Yale Uni. Stanford Uni.
QQ|Archiver|手機(jī)版|小黑屋| 派博傳思國際 ( 京公網(wǎng)安備110108008328) GMT+8, 2025-10-8 16:45
Copyright © 2001-2015 派博傳思   京公網(wǎng)安備110108008328 版權(quán)所有 All rights reserved
快速回復(fù) 返回頂部 返回列表
闸北区| 兴安县| 德兴市| 大足县| 始兴县| 海盐县| 石门县| 麻阳| 汕尾市| 平安县| 兰考县| 高要市| 阿克苏市| 富锦市| 庆元县| 临沂市| 项城市| 惠州市| 兴隆县| 图木舒克市| 鄂托克前旗| 青浦区| 宣城市| 周宁县| 永和县| 三亚市| 囊谦县| 公安县| 竹北市| 枣庄市| 拉孜县| 通榆县| 漳州市| 金川县| 新和县| 泗洪县| 岳阳县| 洪雅县| 上林县| 临桂县| 周宁县|