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Observations of the Coronal Network
Published online by Cambridge University Press: 14 August 2015
Abstract
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
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