Abstract
New measurements of the velocities of moving magnetic features (MMFs) are made from spectroheliograms and filtergrams. The sample includes 200 MMFs found in the moats surrounding 7 different sunspots. Our data are compiled with the data from other authors to uncover common properties of moats. The moat radius is roughly twice the penumbral radius. No significant correlation between the average moat velocity or angular extent and any noted property of the spot or moat (size, age, stage of development) is found. Individual MMFs move radially outward with a constant speed, but nearby MMFs may have quite different speeds. The average moat speed is twice the supergranule flow speed. The speed of MMFs in moats is equal on average to the surface gas flow speed. A large bias is found in much of the existing observations of moat speeds from MMFs.
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Allen, R., Edberg, S., LaBonte, B., and Sheeley, N. R.: 1973, Bull. Am. Astron. Soc. 5, 268.
Biermann, L.: 1941, Vierteljahrsch. Astrophys. Gesellsch. 76, 194.
Cimino, M. (ed.): 1968–1974, Suppl. to Monthly Bull. Solar Phenomena, Osservatorio Astronomico di Roma, Roma.
Clark, A.: 1979, Solar Phys. 62, 305.
Foukal, P., Fowler, L. A., and Livshits, M.: 1983, Astrophys. J. 267, 863.
Fowler, L. A., Foukal, P., and Duvall, T.: 1983, Solar Phys. 84, 33.
Giovanelli, R. G.: 1980, Solar Phys. 67, 211.
Harvey, K. and Harvey, J.: 1973, Solar Phys. 28, 61.
Houtgast, J. and van Sluiters, A.: 1948, Bull. Astron. Inst. Neth. 10, 325.
Küveler, G.: 1983, Solar Phys. 88, 13.
Küveler, G. and Wiehr, E.: 1985, Astron. Astrophys. 142, 205.
Meyer, F., Schmidt, H. U., Weiss, N. O., and Wilson, P. R.: 1974, Monthly Notices Roy. Astron. Soc. 169, 35.
Meyer, F., Schmidt, H. U., Simon, G. W., and Weiss, N. O.: 1979, Astron. Astrophys. 76, 35.
Michalitsanos, A. G. and Bhatnagar, A.: 1975, Astrophys. J. 285, L381.
Nye, A. H., Thomas, J. H., and Cram, L. E.: 1984, Astrophys. J. 285, 381.
Pardon, L., Worden, S. P., and Schneeberger, T. J.: 1979, Solar Phys. 63, 247.
Roy, J. R. and Michalitsanos, A. G.: 1974, Solar Phys. 35, 47.
Schmidt, H. U., Simon, G. W., and Weiss, N. O.: 1985, Astron. Astrophys. 148, 191.
Sheeley, N. R.: 1969, Solar Phys. 9, 347.
Sheeley, N. R.: 1972, Solar Phys. 25, 98.
Sheeley, N. R.: 1981, in F. Q. Orrall (ed.), Solar Active Regions, Colorado Associated University Press, Boulder, Colorado, p. 28.
Shine, R. A., Title, A., Tarbell, T., and the SOUP Team: 1986, Contributed Paper to the Second Workshop on Problems in High Resolution Solar Observations, Boulder, Colorado.
Simon, G., Ferfuson, S., Tarbell, T., Title, A., Topka, K., November, L., and Zirin, H.: 1987, preprint.
Singh, J. and Sappu, M. K. V.: 1981, Solar Phys. 71, 161.
Solar Geophysical Data: 1968–1985, Part 1, U.S. Department of Commerce, Boulder, Colorado.
Spruit, H. C.: 1977, Solar Phys. 55, 3.
Spruit, H. C.: 1981, in L. Cram and J. Thomas (eds.), The Physics of Sunspots, Sacramento Peak Observatory, Sunspot, New Mexico, p. 480.
Spruit, H. C.: 1982a, Astron. Astrophys. 108, 348.
Spruit, H. C.: 1982b, Astron. Astrophys. 108, 356.
Stix, M.: 1981, Astron. Astrophys. 93, 339.
Wiehr, E., Stellmacher, G., Knolker, M., and Grosser, H.: 1986, Astron. Astrophys. 155, 402.
Vrabec, D.: 1974, in Grant Athay (ed.), ‘The Chromospheric Fine Structure’, IAU Symp. 56, 201.
Wallenhorst, S. G. and Topka, K. P.: 1982, Solar Phys. 81, 33.
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Brickhouse, N.S., Labonte, B.J. Mass and energy flow near sunspots. Sol Phys 115, 43–60 (1988). https://doi.org/10.1007/BF00146229
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DOI: https://doi.org/10.1007/BF00146229