Abstract
Solar coronal mass ejections (CMEs) observed in 1980 with the HAO Coronagraph/Polarimeter on the Solar Maximum Mission (SMM) satellite are compared with other forms of solar activity that might be physically related to the ejections. The solar phenomena checked and the method of association used were intentionally patterned after those of Munro et al.'s (1979) analysis of mass ejections observed with the Skylab coronagraph to facilitate comparison of the two epochs. Comparison of the results reveals that the types and degree of CME associations are similar near solar activity minimum and at maximum. For both epochs, most CMEs with associations had associated eruptive prominences and the proportions of association of all types of activity were similar. We also found a high percentage of association between SMM CMEs and X-ray long duration events (LDEs), in agreement with Skylab results. We conclude that most CMEs are the result of the destabilization and eruption of a prominence and its overlying coronal structure, or of a magnetic structure capable of supporting a prominence.
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Anzer, U. and Pneuman, G. W.: 1982, Solar Phys. 79, 129.
Csoeke-Poeckh, A., Lee, R. H., Wagner, W. J., House, L. L., Hildner, E., and Sawyer, C.: 1982, J. Spacecraft 19, 345.
Forbes, T. G. and Priest, E. R.: 1983, Solar Phys. 84, 169.
Hildner, E.: 1977, in M. A. Shea et al. (eds.), Study of Travelling Interplanetary Phenomena, D. Reidel Publ. Co., Dordrecht, Holland, p. 3.
Howard, R. A., Sheeley, N. R., Jr., Koomen, M. J., and Michels, D. J.: 1985, J. Geophys. Res. 90, 8173.
Howard, R. A., Sheeley, N. R., Jr., Koomen, M. J., and Michels, D. J.: 1986, in R. G. Marsden (ed.), The Sun and the Heliosphere in Three Dimensions, D. Reidel Publ. Co., Dordrecht, Holland, p. 107.
Hundhausen, A. J.: 1987, J. Geophys. Res. (submitted).
Hundhausen, A. J., Sawyer, C. S., House, L., Illing, R. M. E., and Wagner, W. J.: 1984, J. Geophys. Res. 89, 2639.
Kahler, S.: 1977, Astrophys. J. 214, 891.
Low, B. C., Munro, R. H., and Fisher, R. R.: 1982, Astrophys. J. 254, 335.
MacQueen, R. M.: 1980, Phil. Trans. R. Soc. London 297, 605.
MacQueen, R. M.: 1985, Solar Phys. 95, 359.
MacQueen, R. M. and Fisher, R. R.: 1983, Solar Phys. 89, 89.
MacQueen, R. M., Csoeke-Poeckh, A., Hildner, E., House, L., Reynolds, R., Stanger, A., TePoel, H., and Wagner, W.: 1980, Solar Phys. 65, 91.
Munro, R., Hildner, E. and Roach, G.: 1976, ‘Revised Transient List (as of 15 June 1976)’ (unpublished).
Munro, R. H., Gosling, J. T., Hildner, E., MacQueen, R. M., Poland, A. E., and Ross, C. L.: 1979, Solar Phys. 61, 201.
Pallavicini, R., Serio, S., and Vaiana, G. S.: 1977, Astrophys. J. 216, 108.
Poland, A. I., Howard, R. A., Koomen, M. J., Michels, D. J., and Sheeley, N. R., Jr.: 1981, Solar Phys. 69, 169.
Robinson, R. D., Tuxford, J. M., Sheridan, K. V., and Stewart, R. T.: 1983, Proc. Astron. Soc. Aust. 5, 84.
Rock, K., Fisher, R., Garcia, C., and Yasukawa, E.: 1983, A Summary of Solar Activity Observed at the Mauna Loa Solar Observatory: 1980–1983, NCAR TN-221, Boulder, CO.
Rust, D. M., Hildner, E. and 11 co-authors: 1980, in P. Sturrock (ed.), Solar Flares, Colorado Assoc. Univ. Press, Boulder, CO, p. 273.
Sheeley, N. R. Jr., and 12 co-authors: 1975, Solar Phys. 45, 377.
Sheeley, N. R., Jr., Howard, R. A., Koomen, M. J., Michels, D. J., Harvey, K. L., and Harvey, J. W.: 1982, Space Sci. Rev. 33, 219.
Sheeley, N. R., Jr., Howard, R.., Koomen, M. J., and Michels, D. J.: 1983, Astrophys. J. 272, 349.
Tandberg-Hanssen, E., Martin, S. A., and Hansen, R. T.: 1980, Solar Phys. 65, 357.
Wagner, W. J.: 1984, Ann. Rev. Astron. Astrophys. 22, 267.
Wagner, W. J.: 1985, in C. de Jager and C. Biao (eds.), Proc. of Kunming Workshop on Solar Physics and Interplanetary Travelling Phenomena, Vol. 2, Science Press, Beijing, China, p. 969.
Webb, D. F.: 1986, in M. R. Kundu et al. (eds.), Solar Terrestrial Physics: Proc. of Second Indo-US Workshop on Solar-Terrestrial Physics, Nat. Physical Lab, New Delhi, India, p. 283.
Webb, D. F.: 1987, ‘SMM I (1980) List of CME Associations’, NCAR Technical Report (to be published).
Webb, D. F., Krieger, A. S., and Rust, D. M.: 1976, Solar Phys. 48, 159.
Wolfson, R. L. T.: 1982, Astrophys. J. 255, 774.
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Much of this work was performed as a Visiting Scientist at the High Altitude Observatory/NCAR.
The National Center for Atmospheric Research is sponsored by the National Science Foundation.
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Webb, D.F., Hundhausen, A.J. Activity associated with the solar origin of coronal mass ejections. Sol Phys 108, 383–401 (1987). https://doi.org/10.1007/BF00214170
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DOI: https://doi.org/10.1007/BF00214170