10月31日（火）13：30～15：00 太陽系小天体セミナー 南棟２階会議室
Oct 31 tue Solar System Minor Body Seminar Conference Room, South Bldg.2F
11月1日（水）10：30～12：00 総研大コロキウム 講義室
Nov 1 wed SOKENDAI colloquium Lecture Room
11月2日（木）11：00～12：00 太陽天体プラズマセミナー 院生セミナー室
Nov 2 thu Solar and Space Plasma Seminar Student Seminar Room, Subaru Bldg.
11月2日（木）13：30～14：30 理論コロキウム コスモス会館会議室
Nov 2 thu DTA colloquium Conference Room, Cosmos Lodge
詳細は以下をご覧下さい。
10月31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
- 10月31日（火曜日）13時30分～15時
- 場所
- 南棟２階会議室
- 講演者
- 大坪貴文
- 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
- Campus
- Mitaka
- Seminar
- SOKENDAI colloquium
- Regularly Scheduled/Sporadic
- Regular
- Date and time
- November 1, 2017, 10:30 -12:00
- Place
- Lecture Room
- Speaker1
- Hiroyuki Ishikawa
- Affiliation
- SOKENDAI: M2 (Supervisor : Takayuki Kotani, Tomonori Usuda, Saeko Hayashi)
- Title
- NIR Spectra of M Dwarfs Obtained by IRD Engineering Run
- Speaker2
- Ko Hosokawa
- Affiliation
- SOKENDAI: M2 (Supervisor :Takayuki Kotani, Tomonori Usuda, Hideki Takami)
- Title
- High Resolution Spectrometer by Applying Static Fourier Transform Method
- Facilitator
- -Name：Nagaaki Kambara
- Comment
- TV conference system is available connecting from Nobeyama, Hawaii, Mizusawa, and Okayama.
- Campus
- Mitaka
- Seminar
- Solar and Space Plasma Seminar
- Regularly Scheduled/Sporadic
- Sporadic
- Date and time
- 2 November (Thu), 11:00-12:00
- Place
- Student Seminar Room, Subaru Bldg.
- Speaker
- Wenda Cao
- Affiliation
- New Jersey Institute of Technology
- Title
- Big Bear Solar Observatory – Cool Toys for Observing Our Warm Star
- Abstract
-
Fundamental discoveries in solar physics rely on advances of instrumentation. This includes observations that advance the state of the art in resolution and cadence, and open new wavelength domains. NJIT (New Jersey Institute of Technology) has built, and now operates the highest-resolution solar telescope ever built ? the Goode Solar Telescope (GST, formerly the New Solar Telescope, NST) at Big Bear Solar Observatory (BBSO), California. This 1.6-meter clear aperture, off-axis GST is the first facility class solar telescope built in the U.S. in a generation and will dominate U.S. ground-based solar observations until the 4-meter DKIST comes online. Benefitting from the long periods of local excellent seeing at Big Bear Lake, the GST, equipped with high-order adaptive optics (AO), routinely collects diffraction-limited spatial resolution (~ 0.1″) photometric, spectroscopic and/or polarimetric data, with a high cadence, across the spectrum from 0.4 –
5.0 μm. Since its regular operation in 2010, it has provided the community with open access to observations of the photosphere, chromosphere and up to the base of the corona with the unprecedented resolution, targeting at the fundamental nature of solar activity and the origin of space weather. This presentation reviews the process of design, construction and commissioning of the GST, and reports the up-to-date progress on its next generation instruments including the AO systems (AO-308, GLAO & MCAO), the Near-InfraRed Imaging Spectro-polarimeter (NIRIS), the Visible Imaging Spectrometer (VIS), the Broad-band Filter Imager (BFI), and the Cryogenic Infrared Spectrograph (CYRA). Some significant scientific results from GST will be highlighted. - Facilitator
- -Name：Shin Toriumi
- Comment
- Campus
- Mitaka
- Seminar
- DTA colloquium
- Regularly Scheduled/Sporadic
- Sporadic
- Date and time
- November 2 2017, 13:30-14:30
- Place
- Conference Room, Cosmos Lodge
- Speaker
- Wanggi Lim
- Affiliation
- NAOJ
- Title
- TBA
- Abstract
- Facilitator
- -Name：Tomoya Takiwaki
- Comment
- in English