Frontier of solar observation. Solar activity observed by 'HINODE' mission
Creators
- 1. National Astronomical Observatory of Japan, Hinode Science Center, Mitaka, Tokyo (Japan)
Description
After launched in September 2006, solar observation satellite 'HINODE' has been a solar observatory on orbit with the scientific instruments well operated and its continuous observation was conducted steadily on almost all solar atmospheres from photosphere to corona. 'HINODE' was equipped with the solar optical telescope, extreme-ultraviolet imaging spectrometer and x-ray telescope and aimed at clarifying the mystery of solar physics related with coronal heating and magnetic reconnection. Present state of 'HINODE' was described from observations made in initial observation results, which have made several discoveries, such as Alfven waves in the corona, unexpected dynamics in the chromosphere and photosphere, continuous outflowing plasma as a possible source of solar wind, and fine structures of magnetic field in sunspots and solar surface. (T. Tanaka)
Additional details
Publishing Information
- Journal Title
- Purazuma, Kaku Yugo Gakkai-Shi
- Journal Volume
- 84
- Journal Issue
- 3
- Journal Page Range
- p. 147-154
- ISSN
- 0918-7928
INIS
- Country of Publication
- Japan
- Country of Input or Organization
- Japan
- INIS RN
- 39087447
- Subject category
- S46: INSTRUMENTATION RELATED TO NUCLEAR SCIENCE AND TECHNOLOGY;
- Descriptors DEI
- MAGNETIC FIELDS; MAGNETIC RECONNECTION; ORBITING SOLAR OBSERVATORIES; PHOTOSPHERE; SOLAR ACTIVITY; SOLAR CORONA; SOLAR FLARES; SOLAR RADIATION; SOLAR WIND; SOLAR X-RAY BURSTS; TELESCOPES; ULTRAVIOLET SPECTROMETERS
- Descriptors DEC
- ATMOSPHERES; MEASURING INSTRUMENTS; RADIATIONS; SATELLITES; SOLAR ACTIVITY; SOLAR ATMOSPHERE; SPECTROMETERS; STELLAR ACTIVITY; STELLAR ATMOSPHERES; STELLAR CORONAE; STELLAR FLARES; STELLAR RADIATION; STELLAR WINDS
Optional Information
- Notes
- 10 refs., 19 figs., 1 tab.