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A possible edge effect in enhanced networkK-line observations of enhanced network taken with the NASA/SPO Multichannel Spectrometer on September 28, 1975, in support of OSO-8 are discussed. The data show a correlation between core brightness and asymmetry for spatial scans which cross enhanced network boundaries. The implications of this result concerning mass flow in and near supergranule boundaries are discussed.
Document ID
19770062482
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Jones, H. P.
(NASA Goddard Space Flight Center Laboratory for Solar Physics and Astrophysics, Albuquerque, N. Mex., United States)
Brown, D. R.
(NASA Goddard Space Flight Center Laboratory for Solar Physics and Astrophysics, Albuquerque; Sacramento Peak Observatory, Sunspot, N., United States)
Date Acquired
August 9, 2013
Publication Date
May 1, 1977
Publication Information
Publication: Solar Physics
Volume: 52
Subject Category
Solar Physics
Accession Number
77A45334
Distribution Limits
Public
Copyright
Other

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