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Titlebook: Magnetospheric Imaging — The Image Prime Mission; J. L. Burch Book 2003 Springer Science+Business Media Dordrecht 2003 Heliosphere.Planet.

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發(fā)表于 2025-3-21 17:50:14 | 只看該作者 |倒序?yàn)g覽 |閱讀模式
書目名稱Magnetospheric Imaging — The Image Prime Mission
編輯J. L. Burch
視頻videohttp://file.papertrans.cn/622/621451/621451.mp4
圖書封面Titlebook: Magnetospheric Imaging — The Image Prime Mission;  J. L. Burch Book 2003 Springer Science+Business Media Dordrecht 2003 Heliosphere.Planet.
描述The Imager for Magnetopause-to-Aurora Global Exploration (IMAGE) is a NASA Explorer mission that is the first space mission dedicated to imaging of the Earth‘s magnetosphere. IMAGE was launched from Vandenberg AFB into an elliptical polar orbit by a Delta II launch vehicle on March 25, 2000. The two-year prime sci- entific mission of IMAGE began on May 25, 2000 after instrument commissioning was successfully completed. IMAGE has now been approved for operation until October 1,2005, and an additional two-year extension is now being considered by NASA. The papers in this volume represent many of the scientific results obtained dur- ing the IMAGE prime mission and include some of the early correlative research with ground-based measurements, measurements from other spacecraft such as Cluster II, and relevant theory and modeling programs. All of the reported work is related to the overall IMAGE science objective: How does the magnetosphere respond globally to the changing conditions in the solar wind? IMAGE addresses this question with multi-spectral imaging of most of the important plasma pop- ulations of the inner magnetosphere, combined with radio sounding of gradients of total plas
出版日期Book 2003
關(guān)鍵詞Heliosphere; Planet; Solar wind; magnetic field; solar
版次1
doihttps://doi.org/10.1007/978-94-010-0027-7
isbn_softcover978-94-010-4000-6
isbn_ebook978-94-010-0027-7
copyrightSpringer Science+Business Media Dordrecht 2003
The information of publication is updating

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Quantifying Global Plasmaspheric Images with , Observations,ellites are combined to understand plasmaspheric behavior and to quantify the global images. A brief review of the understanding of the plasmasphere as learned from in situ observations prior to the launch of IMAGE is given to place the results presented here into context.
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https://doi.org/10.1007/978-94-010-0027-7Heliosphere; Planet; Solar wind; magnetic field; solar
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Extreme Ultraviolet Imager Observations of the Structure and Dynamics of the Plasmasphere,nance line. The images reveal the details of a highly structured and dynamic entity. Comparing EUV images and selected . observations has helped to validate the remote sensing measurements. The brightness in the EUV images is heavily weighted by the He. density near the plane of the magnetic equator
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Quantifying Global Plasmaspheric Images with , Observations,ellites are combined to understand plasmaspheric behavior and to quantify the global images. A brief review of the understanding of the plasmasphere as learned from in situ observations prior to the launch of IMAGE is given to place the results presented here into context.
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