Hinode Discovers the Origin of White Light Flare
November 27, 2012
A joint Japan-United States research team has identified the origin of the white light emission in solar flares. The team, led by Dr. Kyoko Watanabe, an aerospace project research associate at the Japan Aerospace Exploration Agency, made its discovery by quantitatively analyzing an X-class solar flare, which was observed by two successive, solar-observing satellites: Hinode and the NASA SMEX mission RHESSI. The origin of the white light emission had not been clarified since its first discovery about 150 years ago. A solar flare is the most energetic explosion observed in the solar system. Different ways of viewing solar flares include X-rays, radio and chromospheric spectral lines. A large percentage of flares are recognized as a result of associated brightening in the visible light spectrum, and thus are called white light flares. British astronomer Richard Carrington made the first observation of solar flares in 1859 by sketching details of sunspots, including bright features that at times corresponded to white light emissions. However, the occurrence of such emissions is infrequent, leaving the mechanism for their creation unclear. The Solar Optical Telescope, aboard the solar observing satellite Hinode, provides the white light images, allowing scientists for the first time to accurately study the brightness and its time variations. The Hinode observations completed so far indicate that many solar flares are accompanied by white light emissions. Hinode was launched on Sept. 23, 2006 by JAXA, in partnership with NASA and in collaboration with space-agency partners in the United Kingdom, Norway, Europe and Japan's National Astronomical Observatory. White light emissions were observed by the Solar Optical Telescope during an X-class flare that occurred at 22:09 UT on Dec. 14, 2006 (see Fig. 1). The RHESSI satellite simultaneously recorded hard X-ray emissions, an indicator of non-thermal electrons accelerated by solar flares. The team found that the spatial location and temporal change of white light emissions are correlated with those of hard X-ray emissions (see Fig. 2). Moreover, the energy of white light emissions is equivalent to the energy supplied by all the electrons accelerated to above 40 keV (~40 percent of the light speed). This finding strongly suggests that highly accelerated electrons are responsible for producing white light emissions. Hard X-rays are emitted when accelerated electrons impact the dense atmosphere near the solar surface. Normally, white light emissions primarily come from the solar surface, whereas 40 keV electrons can penetrate into the atmosphere about 1,000 km above the solar surface, i.e., the chromosphere. Fig.2: White light emission, left, taken by Hinode/SOT, and the difference image of white light emission and RHESSI hard X-ray contours at 22:09 UT. The background image is the differential white light image (the average of the images taken at 22:07 UT and 22:17 UT is subtracted). Blue contours show 40-100 keV emission. Image credit: NASA/JAXA View large image Particle acceleration is one of the many mysteries surrounding solar flares. Modeling energy transfer of high-energy particles in the solar atmosphere is an important subject for further improving human understanding of particle acceleration. Highly accelerated particles may travel toward the Earth and cause geomagnetic storms, resulting in impacts to Earth-orbiting hardware and human activity on the surface. Now, as solar activity gradually increases after a very long period of minimal high energy activity, solar physicists are hoping the increased solar activity will provide Hinode with additional opportunities to observe solar flares and extend its observations. Hinode is a collaborative mission with NASA and the space agencies of Japan, the United Kingdom, Norway and Europe and Japan's National Astronomical Observatory. NASA's Marshall Space Flight Center in Huntsville, Ala., manages Hinode science operations and oversaw development of the scientific instrumentation provided for the mission by NASA, industry and other federal agencies. The Lockheed Martin Advanced Technology Center in Palo Alto, Calif., is the lead U.S. investigator for the Solar Optical Telescope. The Smithsonian Astrophysical Observatory in Cambridge, Mass., is the lead American investigator for the X-ray Telescope. To view images about these findings and learn more about Hinode, visit: http://www.nasa.gov/hinode Published paper information: Title: “G-band and Hard X-ray Emissions of the 2006 December 14 Flare Observed by Hinode/SOT and RHESSI” by Kyoko Watanabe (Institute of Space and Astronautical Science, JAXA), Säm Krucker, Hugh Hudson (Space Science Laboratories, University of California, Berkeley), Toshifumi Shimizu (ISAS/JAXA), Satoshi Masuda (Nagoya University), Kiyoshi Ichimoto（Kyoto University). The Astrophysical Journal, No.715, pp. 651-655, 2010.
Topics: Environment, Technology Internet, Space, Astronomy, Plasma physics, Japan Aerospace Exploration Agency, X-ray astronomy, Reuven Ramaty High Energy Solar Spectroscopic Imager, Hinode, Solar flare, Space telescopes, Japanese space program, X-ray telescopes, Space plasmas, Japan, National Aeronautics and Space Administration