Observational study of the origin and acceleration mechanism of the solar win
Project/Area Number |
19540474
|
Research Category |
Grant-in-Aid for Scientific Research (C)
|
Allocation Type | Single-year Grants |
Section | 一般 |
Research Field |
Space and upper atmospheric physics
|
Research Institution | Kyoto University |
Principal Investigator |
KITAI Reizaburo Kyoto University, 理学研究科, 准教授 (40169850)
|
Co-Investigator(Kenkyū-buntansha) |
NISHIKAWA Takara 京都経済短期大学, 経営情報, 教授 (10172636)
SHIBATA Kazanari 京都大学, 理, 教授 (70144178)
NAGATA Shin'ichi 京都大学, 理, 助教 (30362437)
UENO Satoru 京都大学, 理, 助教 (70303807)
|
Project Period (FY) |
2007 – 2009
|
Project Status |
Completed (Fiscal Year 2009)
|
Budget Amount *help |
¥4,420,000 (Direct Cost: ¥3,400,000、Indirect Cost: ¥1,020,000)
Fiscal Year 2009: ¥1,040,000 (Direct Cost: ¥800,000、Indirect Cost: ¥240,000)
Fiscal Year 2008: ¥1,430,000 (Direct Cost: ¥1,100,000、Indirect Cost: ¥330,000)
Fiscal Year 2007: ¥1,950,000 (Direct Cost: ¥1,500,000、Indirect Cost: ¥450,000)
|
Keywords | 太陽風 / 彩層ジェット / 太陽活動領域 / 太陽 / 太陽プラージュ / 磁気再結合 / 磁気リコネクション |
Research Abstract |
Driving mechanisms of solar jet phenomena such as Ellerman bomb, spicules and surges are clarified by the analysis of the cooperative observation between the satellite HINODE and the ground-based solar telescopes at Hida Observatory, Kyoto University. Besides, we have got the detailed observational results on the behavior of emerging flux regions and the fine structure of sunspot umbrae.
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Report
(4 results)
Research Products
(42 results)