Abstract
I have studied the observed concentrations of vertical velocity and vertical magnetic field in the corners of the coarse network. Using a horizontal velocity inferred from the vertical velocity, I have computed the possible rate of concentration of the field. The rate turns out to be much higher than observed. I conclude that the observed motions in supergranules are not concentrating the observed field at the corners of the network. I have suggested four possible alternate situations consistent with the observations.
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© 1971 International Astronomical Union
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Musman, S. (1971). Observations and Interpretation of Supergranule Velocity and Magnetic Fields. In: Howard, R. (eds) Solar Magnetic Fields. International Astronomical Union / Union Astronomique Internationale, vol 43. Springer, Dordrecht. https://doi.org/10.1007/978-94-010-3117-2_39
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DOI: https://doi.org/10.1007/978-94-010-3117-2_39
Publisher Name: Springer, Dordrecht
Print ISBN: 978-94-010-3119-6
Online ISBN: 978-94-010-3117-2
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