Imaging Plasma Density Structures in the Soft X-Rays Generated by Solar Wind Charge Exchange with Neutrals
Autor David G. Sibecken Limba Engleză Hardback – 10 mai 2019
Originally published in Space Science Reviews, Volume 214, Issue 4, Article 79, 2018
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Specificații
ISBN-13: 9789402416916
ISBN-10: 9402416919
Pagini: 124
Ilustrații: XIX, 124 p. 101 illus., 87 illus. in color.
Dimensiuni: 155 x 235 mm
Greutate: 0.36 kg
Ediția:1st ed. 2019
Editura: SPRINGER NETHERLANDS
Colecția Springer
Locul publicării:Dordrecht, Netherlands
ISBN-10: 9402416919
Pagini: 124
Ilustrații: XIX, 124 p. 101 illus., 87 illus. in color.
Dimensiuni: 155 x 235 mm
Greutate: 0.36 kg
Ediția:1st ed. 2019
Editura: SPRINGER NETHERLANDS
Colecția Springer
Locul publicării:Dordrecht, Netherlands
Cuprins
About the Authors.- Foreword.- Imaging Plasma Density Structures in the Soft X-Rays Generated by Solar Wind Charge Exchange with Neutrals.
Notă biografică
D. G. Sibeck is NASA’s Mission Scientist for the THEMIS and Van Allen Probes missions. He has extensive experience in analyzing and interpreting plasma, magnetic field, and energetic particle observations from the IMP-8, AMPTE, Geotail, Interball, Wind, GOES, THEMIS, Van Allen Probes, and MMS missions, as well as from ground-based magnetometers and numerical simulations. His research interests focus upon the interaction of the solar wind with the Earth’s magnetosphere, including processes at the magnetopause, in the magnetosheath, outer dayside magnetosphere, and high latitude ionosphere. He has both led and convened numerous NASA and NSF review panels, served as President of the NSF’s GEM Steering Committee, and served as President of the AGU’s SPA Section. He is the author or coauthor of over 350 publications in refereed scientific journals and has served as editor or associate editor for EOS, Advances in Space Research, GRL, and JASTP. Hereceived the AGU’s MacElwane award in 1992.
Caracteristici
Reviews past observations, numerical simulations, and the theory of soft X-rays Details the instrumentation needed to study soft X-rays emitted from planetary obstacles Describes unsolved problems in the solar wind's interaction with Solar System obstacles