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书目名称The Reuven Ramaty High Energy Solar Spectroscopic Imager (RHESSI) - Mission Description and Early Re影响因子(影响力)<br>        http://impactfactor.cn/if/?ISSN=BK0918587<br><br>        <br><br>书目名称The Reuven Ramaty High Energy Solar Spectroscopic Imager (RHESSI) - Mission Description and Early Re影响因子(影响力)学科排名<br>        http://impactfactor.cn/ifr/?ISSN=BK0918587<br><br>        <br><br>书目名称The Reuven Ramaty High Energy Solar Spectroscopic Imager (RHESSI) - Mission Description and Early Re网络公开度<br>        http://impactfactor.cn/at/?ISSN=BK0918587<br><br>        <br><br>书目名称The Reuven Ramaty High Energy Solar Spectroscopic Imager (RHESSI) - Mission Description and Early Re网络公开度学科排名<br>        http://impactfactor.cn/atr/?ISSN=BK0918587<br><br>        <br><br>书目名称The Reuven Ramaty High Energy Solar Spectroscopic Imager (RHESSI) - Mission Description and Early Re被引频次<br>        http://impactfactor.cn/tc/?ISSN=BK0918587<br><br>        <br><br>书目名称The Reuven Ramaty High Energy Solar Spectroscopic Imager (RHESSI) - Mission Description and Early Re被引频次学科排名<br>        http://impactfactor.cn/tcr/?ISSN=BK0918587<br><br>        <br><br>书目名称The Reuven Ramaty High Energy Solar Spectroscopic Imager (RHESSI) - Mission Description and Early Re年度引用<br>        http://impactfactor.cn/ii/?ISSN=BK0918587<br><br>        <br><br>书目名称The Reuven Ramaty High Energy Solar Spectroscopic Imager (RHESSI) - Mission Description and Early Re年度引用学科排名<br>        http://impactfactor.cn/iir/?ISSN=BK0918587<br><br>        <br><br>书目名称The Reuven Ramaty High Energy Solar Spectroscopic Imager (RHESSI) - Mission Description and Early Re读者反馈<br>        http://impactfactor.cn/5y/?ISSN=BK0918587<br><br>        <br><br>书目名称The Reuven Ramaty High Energy Solar Spectroscopic Imager (RHESSI) - Mission Description and Early Re读者反馈学科排名<br>        http://impactfactor.cn/5yr/?ISSN=BK0918587<br><br>        <br><br>

感激小女 发表于 2025-3-21 21:07:20

nergy release and particle acceleration in solar flares through observations of X-rays and gamma rays. Two novel technologies are combined to obtain both spectra and images over a broad energy range. For the spectroscopy, cooled hyperpure germanium detectors are used to cover the energy range from 3

notion 发表于 2025-3-22 01:13:09

Book 2003se new instrumental techniques require equally innovative software to reconstruct X-ray and gamma-ray spectra and images from the observations. .Ample solar activity, abundant observations, and an open data policy have attracted many researchers. Astronomers face in the RHESSI mission an exciting ne

Conjuction 发表于 2025-3-22 07:32:38

efore. These new instrumental techniques require equally innovative software to reconstruct X-ray and gamma-ray spectra and images from the observations. .Ample solar activity, abundant observations, and an open data policy have attracted many researchers. Astronomers face in the RHESSI mission an exciting ne978-90-481-6212-3978-94-017-3452-3

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The Reuven Ramaty High Energy Solar Spectroscopic Imager (RHESSI) - Mission Description and Early Re978-94-017-3452-3

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查看完整版本: Titlebook: The Reuven Ramaty High Energy Solar Spectroscopic Imager (RHESSI) - Mission Description and Early Re; Robert P. Lin,Brian R. Dennis,Arnold