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| Paper: |
Instrument Design of the Large Aperture Solar UV Visible and
IR Observing Telescope (SUVIT) for the SOLAR-C Mission |
| Volume: |
463, 2nd ATST-EAST Workshop in Solar Physics: Magnetic Fields from the Photosphere to the Corona |
| Page: |
439 |
| Authors: |
Suematsu, Y.; Katsukawa, Y.; Shimizu, T.; Ichimoto, K.; Takeyama, N. |
| Abstract: |
We present an instrumental design of one major solar observation
payload planned for the SOLAR-C mission: the Solar Ultra-violet Visible
and near IR observing Telescope (SUVIT).
The SUVIT is designed to provide high-angular-resolution investigation
of the lower solar atmosphere, from the photosphere to the uppermost
chromosphere, with enhanced spectroscopic and spectro-polarimetric
capability in wide wavelength regions from 280 nm
(Mg II h&k lines) to 1100 nm (He I 1083 nm line) with 1.5 m class
aperture and filtergraphic and spectrographic instruments. |
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