A new view of the particle acceleration theory for the neutron star magnetosphere
| Project/Area Number |
22540244
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| Research Category |
Grant-in-Aid for Scientific Research (C)
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| Allocation Type | Single-year Grants |
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| Section | 一般 |
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| Research Field |
Astronomy
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| Research Institution | Yamagata University |
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Principal Investigator |
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| Project Period (FY) |
2010 – 2012
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| Project Status |
Completed (Fiscal Year 2012)
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| Budget Amount *help |
¥4,290,000 (Direct Cost: ¥3,300,000、Indirect Cost: ¥990,000)
Fiscal Year 2012: ¥1,300,000 (Direct Cost: ¥1,000,000、Indirect Cost: ¥300,000)
Fiscal Year 2011: ¥1,300,000 (Direct Cost: ¥1,000,000、Indirect Cost: ¥300,000)
Fiscal Year 2010: ¥1,690,000 (Direct Cost: ¥1,300,000、Indirect Cost: ¥390,000)
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| Keywords | 高エネルギー天文学 / プラズマ物理学 / パルサー / 宇宙物理学 |
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| Research Abstract |
Fermi gamma-ray observatory yields a great expansion of data and new fact on the pulsar magnetosphere. This situation of these days, together with variety of observational results in other wave length, requires new theories and models. In this project, we are attempting to construct such a new view and a new theory for the particle acceleration in the pulsar magnetosphere.
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Report
(4 results)
Research Products
(27 results)
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[Journal Article]2012
Author(s)
Kouzu T., Terada Y., Tashiro M. S., Yamada S., Bamba A., Yuasa T., Mori K., Fukazawa Y., Enoto T., Tanaka Y. T., Shibata S., Makishima K.
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Journal Title
American Institute of Physics Conference Series
Volume: 1427
Pages: 265-265
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