1月29日（火）13：30～15：00 太陽系小天体セミナー 南棟２階会議室
Jan 29 Tue Solar System Minor Body Seminar Conference Room, South Bldg.2F
1月30日（水）10：30～12：00 総研大コロキウム 講義室
Jan 30 Wed SOKENDAI colloquium Lecture Room
1月31日（木）15：00～16：30 太陽天体プラズマセミナー 中央棟（北）113号室
Jan 31 Thu Solar and Space Plasma Seminar Room 113, Central Bldg. (North)
1月31日（木）15：30～17：00 太陽系小天体セミナー 南棟２階会議室
Jan 31 Thu Solar System Minor Body Seminar Conference Room, South Bldg.2F
詳細は以下をご覧下さい。
1月29日（火）
- キャンパス
- 三鷹
- セミナー名
- 太陽系小天体セミナー
- 定例・臨時の別
- 定例
- 日時
- 1月29日（火曜日）13時30分～15時
- 場所
- 南棟２階会議室
- 講演者
- 藤原康徳
- 連絡先
- 名前：渡部潤一
- 備考
- テレビ会議またはスカイプによる参加も可
1月30日（水）
- Campus
- Mitaka
- Seminar
- SOKENDAI colloquium
- Regularly Scheduled/Sporadic
- Regular
- Date and time
- January 30, 2019, 10:30 -12:00
- Place
- Lecture Room
- Speaker
- Jungha Kim
- Affiliation
- SOKENDAI 4th year (D2)(Supervisor:,,)
- Title
- TBD
- Abstract
- (optional)
- Speaker
- Yuhang Zhao
- Affiliation
- SOKENDAI 4th year (D2)(Supervisor: MatteoLeonardi,RaffaeleFlaminio,RyotaroTakahashi)
- Title
- Status of Frequency Dependent Squeezing Experiment at TAMA
- Abstract
- (optional)
Please note that the presenter information posted here is not necessarily listed in order of presentation.
- Facilitator
- -Name：Yoshiki Hatta
- Comment
- TV conference system is available connecting from Nobeyama, Hawaii, Mizusawa, and Okayama.
1月31日（木）
- Campus
- Mitaka
- Seminar
- Solar and Space Plasma Seminar
- Regularly Scheduled/Sporadic
- Sporadic
- Date and time
- 31 January (Thu), 15:00-16:30
- Place
- Room 113, Central Bldg. (North)
- Speaker
- Haosheng Lin
- Affiliation
- Hawaii University
- Title
- A Space Solar Magnetometry Mission
- Abstract
- Comprehensive understanding of the physics of solar eruptions requires knowledge of the 3-dimensional magnetic and thermodynamic structures of the solar atmosphere, from the photosphere to the corona, and how these structures evolve before, during and after the eruptions. A critical requirement for the observation of the 3D magnetic, temperature, and density structures is that their temporal resolution need to be high enough to resolve the dynamic time scale of the eruptions. This knowledge can only be obtained from a space mission consists of a constellation of spacecraft in circumsolar orbits, with each spacecraft performing tomographic observations of the sun using spectroscopic and spectropolarimetric diagnostics of spectral lines with magnetic, temperature, and density sensitivities from different layer of the solar atmosphere. We will present the mission concept and the designs of a compact multi-slit disk spectrograph/spectropolarimeter, and an integral-field coronal spectropolarimeter optimized for deployment in a deep space mission. Simultaneous observations of the photospheric, chromosphere, and corona from multiple sight lines from such a space mission will provide the data needed for 3D tomographic reconstruction of the magnetic and thermodynamic structure of the solar atmosphere. New numerical studies of the efficacy of vector tomographic inversion strategies utilizing only linear polarization measurements of coronal emission lines, as well as vector tomographic inversion utilizing the full-Stokes data will be presented also.
- Facilitator
- -Name：Shin Toriumi
- Comment
1月31日（木）
- キャンパス
- 三鷹
- セミナー名
- 太陽系小天体セミナー
- 定例・臨時の別
- 定例
- 日時
- 1月31日（木曜日）15時30分～17時
- 場所
- 南棟２階会議室
- 講演者
- 小島悠人
- 所属
- 東京大学
- 連絡先
- 名前：渡部潤一
- 備考
- テレビ会議またはスカイプによる参加も可