Home > Solar and Space Plasma (SSP) Seminar | 太陽系小天体セミナー | 理論コロキウム | 総研大コロキウム > 2017.10.30-11.5

2017.10.30-11.5

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

11月1日(水)

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.

11月2日(木)

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

11月2日(木)

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

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