Observational Study of Solar Magnetic Field and Eruption Phenomena at Huairou Solar Observing Station

Details Observational Study of Solar Magnetic Field and Eruption Phenomena at Huairou Solar Observing Station Observational Study of Solar Magnetic Field and Eruption Phenomena at Huairou Solar Observing Station

Aug 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006iaujd...3e..28z&link_type=abstract

Solar Active Regions and 3D Magnetic Structure, 26th meeting of the IAU, Joint Discussion 3, 16-17 August, 2006, Prague, Czech R

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We present the observational study of vector magnetic field and also the development of new optical instrumentations at Huairou Solar Observing Station, National Astronomical Observatories of China. The presentations are following: 1.The synthetical analysis between photospheric vector magnetic field and the morphological configuration in solar atmosphere provides the essential information on the developments of magnetic energy in source regions of Flare-CME Eruptions. The observational study on the evolution of photospheric vector magnetic field provides the basic information for the emergence, storage, relaxes of non-potential magnetic energy in solar active regions (such as, NOAA 9077, 10488 and 10720) and the relationship with the trigger of solar flare-CMEs. The photospheric vector magnetic field also provides the possible forming mechanism of helical magnetic configuration and transferring form in the solar atmosphere into the interplanetary space inferred from the observational vector magnetic field. 2. A brief introduction of new full disk vector magnetograph on the study of large-scale properties of solar magnetic field, which has been operated at Huairou since end of 2005 gradually.

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