Energetic Particles in the Heliosphere
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 chromo...
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| Định dạng: | Sách |
| Ngôn ngữ: | English |
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Springer
2018
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| Truy cập trực tuyến: | http://thuvien.ued.udn.vn/handle/TVDHSPDN_123456789/54258 |
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oai:localhost:TVDHSPDN_123456789-542582022-10-14T03:12:50Z Energetic Particles in the Heliosphere Simnett, George M. Energetic Particles Solar Electrons Energetic Ions Planetary Magnetospheres 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”. 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? 2018-06-21T04:11:20Z 2018-06-21T04:11:20Z 2017 Book 978-3-319-43495-7 http://thuvien.ued.udn.vn/handle/TVDHSPDN_123456789/54258 en Astrophysics and Space Science Library;438 Springer |
| institution |
Trung tâm Học liệu và E-Learning, Trường Đại học Sư phạm – Đại học Đà Nẵng |
| collection |
Thư viện số |
| language |
English |
| topic |
Energetic Particles Solar Electrons Energetic Ions Planetary Magnetospheres |
| spellingShingle |
Energetic Particles Solar Electrons Energetic Ions Planetary Magnetospheres Simnett, George M. Energetic Particles in the Heliosphere |
| description |
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”. |
| format |
Book |
| author |
Simnett, George M. |
| author_facet |
Simnett, George M. |
| author_sort |
Simnett, George M. |
| title |
Energetic Particles in the Heliosphere |
| title_short |
Energetic Particles in the Heliosphere |
| title_full |
Energetic Particles in the Heliosphere |
| title_fullStr |
Energetic Particles in the Heliosphere |
| title_full_unstemmed |
Energetic Particles in the Heliosphere |
| title_sort |
energetic particles in the heliosphere |
| publisher |
Springer |
| publishDate |
2018 |
| url |
http://thuvien.ued.udn.vn/handle/TVDHSPDN_123456789/54258 |
| _version_ |
1766670435366207488 |