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Observations of the Coronal Network

Published online by Cambridge University Press:  14 August 2015

George W. Simon  and
Robert W. Noyes
George W. Simon
Affiliation:
Sacramento Peak Observatory, Sunspot, N. Mex. 88349, U.S.A.
Robert W. Noyes
Affiliation:
Harvard College Observatory, Cambridge, Mass. 02138, U.S.A.

Abstract

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Spectroheliograms of quiet regions obtained by the OSO-G satellite in chromospheric, transition zone, and coronal lines indicate that the chromospheric network as seen in Ca K can be resolved despite the low resolution (30 arc s) of OSO-G. The network pattern becomes more diffuse with increasing height, indicating that the magnetic field pattern spreads with height.

Type
Part VI: Optical and Radio Observations of Large Scale Magnetic Fields on the Sun
Information
Symposium - International Astronomical Union , Volume 43: Solar Magnetic Fields , 1971 , pp. 663 - 666
Copyright
Copyright © Reidel 1971