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Full-Disk solar Dopplergrams observed with a 1024 × 1024-Pixel CCD Camera

Published online by Cambridge University Press:  03 August 2017

Edward J. Rhodes Jr. ,
Alessandro Cacciani  and
Steven Tomczyk
Edward J. Rhodes Jr.
Affiliation:
University of Southern California Los Angeles, California 90089-1342 Jet Propulsion Laboratory California Institute of Technology Pasadena, California 91109
Alessandro Cacciani
Affiliation:
University of Rome, Rome, Italy
Steven Tomczyk
Affiliation:
University of California at Los Angeles, Los Angeles, California 90024

Abstract

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We present here the first full-disk solar Dopplergram obtained with the new 1024 × 1024-pixel CCD camera which has recently been installed at the 60-Foot Tower Telescope of the Mt. Wilson Observatory. This Dopplergram has a spatial resolution of 2.2 arcseconds and was obtained in less than one minute of time. The Dopplergram was obtained with a magneto-optical filter which was designed to obtain images in the two Na D lines. The filter and the camera were operated together as part of the development of a Solar Oscillations Imager (SOI) esperiment which is currently being designed at JPL for the joint NASA/ESA Solar and Heliospheric Observatory (SOHO) mission.

Type
Chapter 8: Techniques for Observing Solar Oscillations
Information
Symposium - International Astronomical Union , Volume 123: Advances In Hello- and Asteroseismology , 1988 , pp. 471 - 474
Copyright
Copyright © Reidel 1988 

References

Rhodes, E. J. Jr., Bursch, T. K., Ulrich, R. K., and Tomczyk, S. ‘A one megapixel image acquisition and processing system for Solar Oscillation Studies,1 to appear in Proceedings of Instrumentation in Astronomy VI, SPIE, in press, 1986.CrossRefGoogle Scholar