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A possible edge effect in enhanced network
Authors:Harrison P Jones  Douglas R Brown
Institution:(1) NASA/GSFC, Laboratory for Solar Physics and Astrophysics, New Mexico Station, 800 Yale Blvd. N.E., 87131 Albuquerque, New Mexico, USA;(2) NASA/GSFC, Laboratory for Solar Physics and Astrophysics, Solar Spectrometer Group, Sacramento Peak Observatory, 88349 Sunspot, New Mexico, USA
Abstract:K-line observations of enhanced network taken with the NASA/SPO Multichannel Spectrometer on 28 September 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.
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