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Energetic particles in the heliosphere

Simnett, George M.

Energetic particles in the heliosphere

紀錄類型:	書目-電子資源 : Monograph/item
正題名/作者:	Energetic particles in the heliosphereby George M. Simnett.
作者:	Simnett, George M.
出版者:	Cham :Springer International Publishing :2017.
面頁冊數:	ix, 242 p. :ill., digital ;24 cm.
Contained By:	Springer eBooks
標題:	Cosmic rays.
電子資源:	http://dx.doi.org/10.1007/978-3-319-43495-7
ISBN:	9783319434957$q(electronic bk.)

Energetic particles in the heliosphere
Simnett, George M.

Energetic particles in the heliosphere[electronic resource] /by George M. Simnett. - Cham :Springer International Publishing :2017. - ix, 242 p. :ill., digital ;24 cm. - Astrophysics and space science library,4380067-0057 ;. - Astrophysics and space science library ;379..

Introduction -- Instrumentation -- Energetic Particle Acceleration -- Solar Electrons as a Probe of the Inner Heliosphere -- Studies of Energetic Ions in the Inner Heliosphere -- Corotating Interaction Regions -- Studies onf the High Latitude Heliosphere -- The Anomalus Cosmic Ray -- Studies of the Distant Heliosphere beyond Jupiter -- Energetic Particles From Planetary Magnetospheres -- What about the Future?

This monograph traces the development of our understanding of how and where energetic particles are accelerated in the heliosphere and how they may reach the Earth. Detailed data sets are presented which address these topics. The bulk of the observations are from spacecraft in or near the ecliptic plane. It is timely to present this subject now that Voyager-1 has entered the true interstellar medium. Since it seems unlikely that there will be a follow-on to the Voyager programme any time soon, the data we already have regarding the outer heliosphere are not going to be enhanced for at least 40 years.

ISBN: 9783319434957$q(electronic bk.)

Standard No.: 10.1007/978-3-319-43495-7doiSubjects--Topical Terms:

339221
Cosmic rays.

LC Class. No.: QB526.S65

Dewey Class. No.: 523.72

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520 $a This monograph traces the development of our understanding of how and where energetic particles are accelerated in the heliosphere and how they may reach the Earth. Detailed data sets are presented which address these topics. The bulk of the observations are from spacecraft in or near the ecliptic plane. It is timely to present this subject now that Voyager-1 has entered the true interstellar medium. Since it seems unlikely that there will be a follow-on to the Voyager programme any time soon, the data we already have regarding the outer heliosphere are not going to be enhanced for at least 40 years.
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