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Solar full-disk magnetic field image receiving system and observation softwareThe paper introduces terminal hardware system of 10 cm high resolution full-disk magnetic field telescope among solar multi-channel telescope produced by Beijing Astronomical Observatory, and its software procedure by using imaging processing as well real time data collecting. These data were processed by Sun Workstation 470/4, including doing some spectrum analysis, the system is unique in the world now. It uses a set of CCD (1320 pixels plus 1035 pixels) of high resolution image explosion, also it has a set of fast and high resolution (1024 pixel plus 1024 pixel) image processor. Moreover, we can obtain higher time and space resolution about solar full-disk magnetic field and velocity field. This will provide excellent means in observation and studies of full-disk solar large-scale magnetic field and velocity field.
Document ID
19940018079
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Xu, Yan
(Academia Sinica Beijing, China)
Chang-Rong, Ming
(Academia Sinica Beijing, China)
Rong, Xing
(Academia Sinica Beijing, China)
Date Acquired
September 6, 2013
Publication Date
January 1, 1992
Publication Information
Publication: NASA, Washington, Second Annual Conference on Astronomical Data Analysis Software and Systems. Abstracts
Subject Category
Astronomy
Accession Number
94N22552
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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