Energetic Particles in the Heliosphere

Please use this identifier to cite or link to this item: http://thuvien.ued.udn.vn/handle/TVDHSPDN_123456789/54258

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DC Field	Value	Language
dc.contributor.author	Simnett, George M.	-
dc.date.accessioned	2018-06-21T04:11:20Z	-
dc.date.available	2018-06-21T04:11:20Z	-
dc.date.issued	2017	-
dc.identifier.isbn	978-3-319-43495-7	-
dc.identifier.uri	http://thuvien.ued.udn.vn/handle/TVDHSPDN_123456789/54258	-
dc.description.abstract	Thermal ionization can only be an approximation as the source at the Sun is almost certainly not in equilibrium and probably never has been. Nonthermal ionization is virtually unknown as it requires knowledge of the energy spectrum and elemental composition of the interacting particles in the chromosphere/corona. There are so many unknown parameters that understanding the truth is just like a “can of worms”.	vi
dc.description.tableofcontents	1 Introduction; 2 Instrumentation; 3 Energetic Particle Acceleration; 4 Solar Electrons as a Probe of the Inner Heliosphere; 5 Studies of Energetic Ions in the Inner Heliosphere; 6 Corotating Interaction Regions; 7 Studies of the High Latitude Heliosphere; 8 The Anomalous Cosmic Rays; 9 Studies of the Distant Heliosphere Beyond Jupiter; 10 Energetic Particles from Planetary Magnetospheres; 11 What About the Future?	vi
dc.language.iso	en	vi
dc.publisher	Springer	vi
dc.relation.ispartofseries	Astrophysics and Space Science Library;438	-
dc.subject	Energetic Particles	vi
dc.subject	Solar Electrons	vi
dc.subject	Energetic Ions	vi
dc.subject	Planetary Magnetospheres	vi
dc.title	Energetic Particles in the Heliosphere	vi
dc.type	Book	vi
Appears in Collections:	Physics

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