CCD polarimetry of the solar corona at the 1997-03-09 solar eclipse |
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| Institution: | 1. Key Laboratory of Middle Atmosphere and Global Environment Observation, Institute of Atmospheric Physics, Chinese Academy of Sciences, Beijing 100029, China;2. University of Chinese Academy of Sciences, Beijing 100049, China;3. Earth and Atmospheric Sciences, University of Nebraska-Lincoln, 303 Bessey Hall, Lincoln, NE 68588, USA;4. Center for Global and Regional Environmental Research, Department of Chemical and Biochemical Engineering, The University of Iowa, 4133 Seamans Center, Iowa City, IA 52242, USA;5. Changchun Institute of Optics, Fine Mechanics and Physics, Chinese Academy of Sciences, Changchun 130033, China;6. National Centre for Earth Observation, School of GeoSciences, University of Edinburgh, UK;1. Institute of Astronomy, Kharkov V.N. Karazin National University, Kharkov 61022, Ukraine;2. School of Natural Sciences, Far Eastern Federal University, Vladivostok 690950 Russia;3. Space Science Institute, 4750 Walnut St. Suite 205, Boulder, CO 80301, USA;1. CSRE, Indian Institute of Technology Bombay, India;2. IETR, University of Rennes 1, France |
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| Abstract: | We give the treated results of our CCD polarimetric data of the solar corona obtained during the 1997-03-09 total eclipse, including the profiles of absolute brightness and degree of polarization along 12 directions (including the two equatorial and two polar directions) in the middle corona (1.6?3.2 R⊙) |
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