| Project/Area Number |
02044074
|
|---|
| Research Category |
Grant-in-Aid for international Scientific Research
|
| Allocation Type | Single-year Grants |
|---|
| Section | Joint Research |
|---|
| Research Institution | Kyoto University |
|---|
Principal Investigator |
MAKITA Mitugu Kyoto University, Prof., 理学部, 教授 (90012806)
|
|---|
| Co-Investigator(Kenkyū-buntansha) |
方 成 南京大学, 天文系, 教授
丁 有済 中国科学院, 雲南天文台, 教授
艾 国祥 中国科学院, 北京天文台, 教授
TSUBAKI Tokio Shiga University, Prof., 教育学部, 教授 (10040700)
KUBOTA Jun Osaka Keizai University, Prof., 経済学部, 教授 (30066815)
ICHIMOTO Kiyoshi National Astronomical Observatory, Res. Assoc., 太陽物理学研究系, 助手 (70193456)
SUEMATSU Yoshinori National Astronomical Observatory, Res. Assoc., 太陽物理学研究系, 助手 (50171111)
SAKURAI Takashi National Astronomical Observatory, A. Prof., 太陽物理学研究系, 助教授 (40114491)
HIRAYAMA Tadashi National Astronomical Observatory, Prof., 太陽物理学研究系, 教授 (20012841)
HIEI Eijiro National Astronomical Observatory, Prof., 太陽物理学研究系, 教授 (60012796)
KUROKAWA Hiroki Kyoto University, A. Prof., 理学部, 助教授 (80135508)
DING Youji Yunnan Observatory, Prof.
AI Guoxiang Beijing Astronomical Observatory, Prof.
FANG Cheng Nanjing University, Prof.
|
|---|
| Project Period (FY) |
1990
|
| Project Status |
Completed (Fiscal Year 1990)
|
| Budget Amount *help |
¥3,000,000 (Direct Cost: ¥3,000,000)
Fiscal Year 1990: ¥3,000,000 (Direct Cost: ¥3,000,000)
|
|---|
| Keywords | Solar Activity / Magnetic Field / Simultaneous Observation |
|---|
| Research Abstract |
The progress made under this project is as in the following ;
(1) Coordinated simultaneous observation.
We, Japanese and Chinese observers, have recently completed a network system for the coordinated simultaneous observations. With the use of this system the coordinated observation was made from Aug. 19 to Sep. 2, 1990. The target active region was NOAA 6233.
(2) Cooperative analysis.
Cooperative analysis has just begun. Rather fragmental studies, such as comparison of the Hida H-alpha photos with the Huairou magnetograms, are performed. It is obvious that non-potential magnetic fields are clearly related to active phenomenae on the sun. However, we need more accumulation of the data before predicting when and where the active phenomena occurs in the active region.
(3) Exchange visit program.
The project invited 2 Chinese scientist to the Solar-A Science Meeting in October, 1990, and sent 7 Japanese scientist to the 1st Sino-Japan Seminar on Solar Physics in March, 1991. These two opportunities were invaluable to increase mutual collaborations.
Reports produced by this project will appear in the Proceedings of the two scientific meetings.
|
