Hinode: A New Solar Observatory in Space
スポンサーリンク
概要
- 論文の詳細を見る
The third Japanese solar observing satellite, SOLAR-B, was launched on 2006 Sep 23 from the Uchinoura Space Center of JAXA and it was named "Hinode" (sunrise). Hinode carries three major telescopes: Solar Optical Telescope (SOT), X-Ray Telescope (XRT), and Extreme-ultraviolet Imaging Spectrometer (EIS). These telescopes have been built in an international collaboration of Japan, US, and UK for understanding the formation mechanism of the solar corona, mechanism of dynamic events such as solar flares and coronal mass ejection, and general magnetic activities on the sun. All telescopes have started their commissioning activities after the successful launch of the spacecraft. The performance of the spacecraft that supports the diffraction-limited SOT observations and the first-light observation of each telescope are briefly introduced.
- 社団法人 プラズマ・核融合学会の論文
著者
-
Hara Hirohisa
National Astoronomical Observatory Of Japan
-
HARA Hirohisa
National Astronomical Observatory of Japan, Mitaka, Tokyo 181-8588
関連論文
- EUV Emission Lines and Diagnostics Observed with Hinode/EIS
- 2006 December 17 Long Duration Flare Observed with the Hinode EUV Imaging Spectrometer
- On Connecting the Dynamics of the Chromosphere and Transition Region with Hinode SOT and EIS
- Hinode EUV Imaging Spectrometer Observations of Solar Active Region Dynamics
- Observations of Transient Active Region Heating with Hinode
- Wavelength Determination for Solar Features Observed by the EUV Imaging Spectrometer on Hinode
- Discovery of a Temperature-Dependent Upflow in the Plage Region during a Gradual Phase of the X-Class Flare
- Velocity Structure of Jets in a Coronal Hole
- Solar Transition Region Features Observed with Hinode/EIS
- Hot and Cool Loops Composing the Corona of the Quiet Sun
- Temperature and Density Structures of Solar Corona : A Test of Iron Line Diagnostic Capability of EIS Instrument on Board Hinode
- Coronal Dimming Observed with Hinode : Outflows Related to a Coronal Mass Ejection
- Vertical Temperature Structures of the Solar Corona Derived with the Hinode X-Ray Telescope
- A High-Temperature Component in Coronal Holes as Confirmed by a Partial-Eclipse Observation
- On the Detection of Solar Coronal High-Velocity Fields Using the XUV Doppler Telescope
- Hard X-Ray Sources and the Primary Energy-Release Site in Solar Flares
- Hinode: A New Solar Observatory in Space