Hostname: page-component-78c5997874-m6dg7 Total loading time: 0 Render date: 2024-11-19T17:59:55.875Z Has data issue: false hasContentIssue false
  • English
  • Français

Magnetic Structure Responsible for Coronal Disturbances: Observations

Published online by Cambridge University Press:  25 May 2016

Martin D. Altschuler
Martin D. Altschuler*
Affiliation:
High Altitude Observatory, National Center for Atmospheric Research*, Boulder, Colo., U.S.A.

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

Coronal disturbances are considered as consequences of the ejection of electric currents (or non-potential magnetic fields) from the photosphere and chromosphere into the corona. It may be that electric currents are generated near neutral lines in the photosphere and are later ejected into the corona.

Type
Part I Magnetic Structure Responsible for Coronal Disturbances
Information
Symposium - International Astronomical Union , Volume 57: Coronal Disturbances , 1974 , pp. 3 - 33
Copyright
Copyright © Reidel 1974 

References

Altschuler, M. D.: 1971, Sky Telesc. 41, 146.Google Scholar
Altschuler, M. D., Lilliequist, C. G., and Nakagawa, Y.: 1968, Solar Phys. 5, 366.CrossRefGoogle Scholar
Altschuler, M. D. and Newkirk, G. Jr.: 1969, Solar Phys. 9, 131.CrossRefGoogle Scholar
Altschuler, M. D. and Perry, R. M.: 1972, Solar Phys. 23, 410.CrossRefGoogle Scholar
Altschuler, M. D., Smith, D. F., Swarztrauber, P. N., and Priest, E. R.: 1973, Solar Phys. 32, 153.CrossRefGoogle Scholar
Altschuler, M. D., Trotter, D. E., and Orrall, F. Q.: 1972, Solar Phys. 26, 354.CrossRefGoogle Scholar
Anderson, G. E.: 1966, , Univ. of Colorado.Google Scholar
Anzer, U.: 1968, Solar Phys. 3, 298.CrossRefGoogle Scholar
Anzer, U. and Tandberg-Hanssen, E.: 1970, Solar Phys. 11, 61.CrossRefGoogle Scholar
Beckers, J. M.: 1968, Solar Phys. 3, 367.Google Scholar
Beckers, J. M.: 1971, in Howard, R. (ed.), ‘Solar Magnetic Fields’, IAU Symp. 43, p. 3.Google Scholar
Beckers, J. M. and Wagner, W. J.: 1971, Solar Phys. 21, 439.CrossRefGoogle Scholar
Billings, D. E.: 1966, A Guide to the Solar Corona, Academic Press, N.Y. Google Scholar
Brown, A.: 1958, Astrophys. J. 128, 646.CrossRefGoogle Scholar
Bruzek, A.: 1964, Astrophys. J. 140, 746.CrossRefGoogle Scholar
Bruzek, A. and Demastus, H. L.: 1970, Solar Phys. 12, 447.CrossRefGoogle Scholar
Bumba, V.: 1967, in Sturrock, P. A. (ed.), Plasma Astrophysics, Academic Press, p. 77.Google Scholar
Charvin, P.: 1965, Ann. Astrophys. 28, 877.Google Scholar
Charvin, P.: 1971, in Howard, R. (ed.), ‘Solar Magnetic Fields’, IAU Symp. 43, p. 580.Google Scholar
Cheng, C. C., Phillips, K. J. H., and Wilson, A. M.: 1973, Solar Phys. 29, 383.CrossRefGoogle Scholar
Coppi, B. and Friedland, A. B.: 1971, Astrophys. J. 169, 379.CrossRefGoogle Scholar
Daigne, G., Lantos-Jarry, M. F., and Pick, M.: 1971, in Howard, R. (ed.), ‘Solar Magnetic Fields’, IAU Symp. 43, p. 609.Google Scholar
Davis, H. T.: 1962, Introduction to Nonlinear Differential and Integral Equations, Dover Publ. Google Scholar
Dodson, H. W., Hedeman, E. R., and Rovira de Miceli, M.: 1972, Solar Phys. 23, 360.CrossRefGoogle Scholar
Dulk, G. A. and Altschuler, M. D.: 1971, Solar Phys. 20, 438.CrossRefGoogle Scholar
Dulk, G. A., Altschuler, M. D., and Smerd, S. F.: 1971, Astrophys. Letters 8, 235.Google Scholar
Dunn, R.: 1960, , Harvard Univ. Google Scholar
Dunn, R. B.: 1971, in Macris, C. J. (ed.), Physics of the Solar Corona, D. Reidel Publ., p. 114.Google Scholar
Eddy, J. A., Lee, R. H., and Emerson, J. P.: 1973, Solar Phys. 30, 351.CrossRefGoogle Scholar
Eddy, J. A. and Malville, J. M.: 1967, Astrophys. J. 150, 289.CrossRefGoogle Scholar
Engvold, O.: 1972, Solar Phys. 23, 346.CrossRefGoogle Scholar
Foukal, H. and Zirin, H.: 1972, Solar Phys. 26, 148.CrossRefGoogle Scholar
Frazier, E. N.: 1972a, Solar Phys. 24, 98.CrossRefGoogle Scholar
Frazier, E. N.: 1972b, Solar Phys. 26, 142.CrossRefGoogle Scholar
Frazier, E. N. and Stenflo, J. O.: 1972, Solar Phys. 27, 330.CrossRefGoogle Scholar
Gold, T.: 1964, in Hess, W. N. (ed.), The Physics of Solar Flares, NASA SP-50, p. 389.Google Scholar
Gold, T.: 1968, in Öhman, Y. (ed.), ‘Mass Motions in Solar Flares and Related Phenomena’, Nobel Symp. 9, p. 205.Google Scholar
Harvey, J. W.: 1969, , Univ. of Colorado.Google Scholar
Harvey, J. W.; 1972, in McIntosh, P. and Dryer, M. (eds.), Solar Activity Observations and Predictions, MIT Press, p. 51.Google Scholar
Harvey, K. L., Livingston, W. C., Harvey, J. W., and Slaughter, C. D.: 1971, in Howard, R. (ed.), ‘Solar Magnetic Fields’, IAU Symp. 43, p. 422.Google Scholar
Hildner, E.: 1971, , Univ. of Colorado.Google Scholar
House, L. L.: 1972, Solar Phys. 23, 103.CrossRefGoogle Scholar
Howard, R.: 1971, Solar Phys. 16, 21.CrossRefGoogle Scholar
Howard, R., Bumba, V., and Smith, S. F.: 1967, Atlas of Solar Magnetic Fields, Carnegie Inst. of Washington, Publication 626.Google Scholar
Howard, R. and Harvey, J. W.: 1964, Astrophys. J. 139, 1328.CrossRefGoogle Scholar
Howard, R. and Stenflo, J. O.: 1972, Solar Phys. 22, 402.CrossRefGoogle Scholar
Hyder, C. L.: 1965, Astrophys. J. 141, 1382.CrossRefGoogle Scholar
Hyder, C. L.: 1966, in Atti del Convegno sui Campi Magnetici Solari, Rome Obs., p. 110.Google Scholar
Hyder, C. L.: 1967, Solar Phys. 2, 49.CrossRefGoogle Scholar
Hyder, C. L., Mauter, H. A., and Shutt, R. L.: 1968, Astrophys. J. 154, 1039.CrossRefGoogle Scholar
Jefferies, J. T. and Orrall, F. Q.: 1964, in Hess, W. N. (ed.), The Physics of Solar Flares, NASA SP-50, p. 71.Google Scholar
Kippenhahn, R. and Schluter, A.: 1957, Z. Astrophys. 43, 36.Google Scholar
Kleczek, J.: 1964, in Hess, W. N. (ed.), The Physics of Solar Flares, NASA SP-50, p. 77.Google Scholar
Kopecky, M. and Kuklin, G. V.: 1971, in Howard, R. (ed.), ‘Solar Magnetic Fields’, IAU Symp. 43, p. 534.Google Scholar
Krieger, A. S., Vaiana, G. S., and Van Speybroeck, L. P.: 1971, in Howard, R. (ed.), ‘Physics of the Solar Corona’, IAU Symp. 43, p. 397.Google Scholar
Kuiper, T. B. H.: 1973, Solar Phys. 33, 461.CrossRefGoogle Scholar
Kundu, M. R.: 1971, in Howard, R. (ed.), ‘Solar Magnetic Fields’, IAU Symp. 43, p. 642.Google Scholar
Kuperus, M. and Athay, R. G.: 1967, Solar Phys. 1, 361.CrossRefGoogle Scholar
Levine, R. and Nakagawa, Y.: 1974, Astrophys. J., in press.Google Scholar
Macris, C. J.: 1971, in Macris, C. J. (ed.), Physics of the Solar Corona, D. Reidel Publ., p. 168.Google Scholar
McLean, D. J.: 1967, Proc. Astron. Soc. Australia 1, 47.CrossRefGoogle Scholar
Meyer, F.: 1968, in Kiepenheuer, K. O. (ed.), ‘Structure and Development of Solar Active Regions’, IAU Symp. 35, p. 485.Google Scholar
Meyer, F. and Schmidt, H. U.: 1968, Mitt. Astron. Ges. 25, 194.Google Scholar
Moreton, G. E. and Ramsey, H. E.: 1960, Publ. Astron. Soc. Pacific 72, 357.CrossRefGoogle Scholar
Nakagawa, Y. and Malville, J. M.: 1969, Solar Phys. 9, 102.CrossRefGoogle Scholar
Nakagawa, Y. and Raadu, M. A.: 1972, Solar Phys. 25, 127.CrossRefGoogle Scholar
Neupert, W. M.: 1971, in Macris, C. J. (ed.), Physics of the Solar Corona, D. Reidel Publ. Co., Dordrecht, p. 237.Google Scholar
Neupert, W. M., Thomas, R. J., and Chapman, R. D.: 1974, Solar Phys. 34, 349.CrossRefGoogle Scholar
Newkirk, G. Jr.: 1971, in Macris, C. J. (ed.), Physics of the Solar Corona, D. Reidel Publ. Co., Dordrecht, p. 66.Google Scholar
Newkirk, G. Jr. and Altschuler, M. D.: 1970, Solar Phys. 13, 131.CrossRefGoogle Scholar
Newkirk, G. Jr., Altschuler, M. D., and Harvey, J.: 1968, in Kiepenheuer, K. O. (ed.), ‘Structure and Development of Solar Active Regions’, IAU Symp. 35, p. 379.Google Scholar
Newkirk, G. Jr., Trotter, D. E., Altschuler, M. D., and Howard, R.: 1972, A Microfilm Atlas of Magnetic Fields in the Solar Corona, NCAR-TN/STR-85.CrossRefGoogle Scholar
Öhman, Y. (ed.): 1968, ‘Mass Motions in Solar Flares and Related Phenomena’, Nobel Symp. 9.Google Scholar
Orrall, F. Q.: 1971, in Howard, R. (ed.), ‘Solar Magnetic Fields’, IAU Symp. 43, p. 30.Google Scholar
Parker, E. N.: 1955, Astrophys. J. 121, 491.CrossRefGoogle Scholar
Perry, R. M. and Altschuler, M. D.: 1973, Solar Phys. 28, 435.CrossRefGoogle Scholar
Petschek, H. E.: 1964, in Hess, W. N. (ed.), The Physics of Solar Flares, NASA SP-50, p. 425.Google Scholar
Piddington, J. H.: 1972, Solar Phys. 27, 402.CrossRefGoogle Scholar
Pikelner, S. B.: 1966, Fundamentals of Cosmic Electrodynamics (2nd ed.), Nauka, Moscow.Google Scholar
Pikelner, S. B.: 1969, Astron. Zh. 46, 328 (Soviet Astron. 13, 259).Google Scholar
Pneuman, G. W.: 1967, Solar Phys. 2, 462.CrossRefGoogle Scholar
Pneuman, G. W. and Kopp, R. A.: 1971, Solar Phys. 18, 258.CrossRefGoogle Scholar
Querfeld, C. W.: 1974 in Gehrels, T. (ed.), Planets, Stars, and Nebulae Studied with Photopolarimetry, Univ. of Ariz. Press, p. 264.Google Scholar
Raadu, M. A. and Kuperus, M.: 1973, Solar Phys. 28, 77.CrossRefGoogle Scholar
Rayrole, J. and Semel, M.: 1968, in Kiepenheuer, K. O. (ed.), ‘Structure and Development of Solar Active Regions’, IAU Symp. 35, p. 134.Google Scholar
Riddle, A. C.: 1970, Solar Phys. 13, 448.CrossRefGoogle Scholar
Roy, J. R.: 1972, Solar Phys. 26, 418.CrossRefGoogle Scholar
Roy, J. R.: 1973, Solar Phys. 28, 95.CrossRefGoogle Scholar
Rust, D. M.: 1966, , Univ. of Colorado.Google Scholar
Rust, D. M.: 1967, Astrophys. J. 150, 313.CrossRefGoogle Scholar
Rust, D. M.: 1968, in Kiepenheuer, K. O. (ed.), ‘Structure and Development of Solar Active Regions’, IAU Symp. 35, p. 77.Google Scholar
Rust, D. M.: 1970, Astrophys. J. 160, 315.CrossRefGoogle Scholar
Rust, D. M. and Roy, J. R.: 1971, in Howard, R. (ed.), ‘Physics of the Solar Corona’, IAU Symp. 43, p. 569.Google Scholar
Schatten, K. H.: 1970, Solar Phys. 12, 484.CrossRefGoogle Scholar
Schatten, K. H.: 1971a, Cosmic Electrodyn. 2, 232.Google Scholar
Schatten, K. H.: 1971b, in Howard, R. (ed.), ‘Solar Magnetic Fields’, IAU Symp. 43, p. 595.Google Scholar
Schatten, K. H., Wilcox, J. M., and Ness, N. F.: 1969, Solar Phys. 6, 442.CrossRefGoogle Scholar
Scherrer, P. H., Wilcox, J. M., and Howard, R.: 1972, Solar Phys. 22, 418.CrossRefGoogle Scholar
Schmidt, H. U.: 1964, in Hess, W. N. (ed.), The Physics of Solar Flares, NASA SP-50, p. 107.Google Scholar
Severny, A. B.: 1969, in de Jager, C. and Švestka, Z. (eds.), ‘Solar Flares and Space Research’, COSPAR Symp., p. 38.Google Scholar
Simon, G. W. and Weiss, N. O.: 1968, in Kiepenheuer, K. O. (ed.), ‘Structure and Development of Solar Active Regions’, IAU Symp. 35, p. 108.Google Scholar
Smerd, S. F. and Dulk, G. A.: 1971, in Howard, R. (ed.), ‘Solar Magnetic Fields’, IAU Symp. 43, p. 616.Google Scholar
Smith, S. F. and Harvey, K. L.: 1971, in Macris, C. J. (ed.), Physics of the Solar Corona, D. Reidel Publ., p. 156.Google Scholar
Smith, H. and Smith, E. v. P.: 1963, Solar Flares, Macmillan Co. Google Scholar
Stenflo, J. O.: 1969, Solar Phys. 8, 115.CrossRefGoogle Scholar
Stenflo, J. O.: 1971, in Howard, R. (ed.), ‘Solar Magnetic Fields’, IAU Symp. 43, p. 101.Google Scholar
Sturrock, P. A.: 1968, in Kiepenheuer, K. O. (ed.), ‘Structure and Development of Solar Active Regions’, IAU Symp. 35, p. 471.Google Scholar
Sturrock, P. A. and Coppi, B.: 1966, Astrophys. J. 143, 3.CrossRefGoogle Scholar
Švestka, Z.: 1969, in de Jager, C. and Švestka, Z. (eds.), ‘Solar Flares and Space Research’, COSPAR Symp., 16.Google Scholar
Sweet, P. A.: 1958, in Lehnert, B., ‘Electromagnetic Phenomena in Cosmical Physics’, IAU Symp. 6, p. 123.Google Scholar
Tandberg-Hanssen, E.: 1971, in Howard, R. (ed.), ‘Solar Magnetic Fields’, IAU Symp. 43, p. 192.Google Scholar
Tandberg-Hanssen, E. (ed.): 1974, Solar Prominences, D. Reidel Publ. Co., Dordrecht-Holland.CrossRefGoogle Scholar
Thomas, R. J. and Neupert, W. M.: 1971, Bull. Am. Astron. Soc. 3, p. 7.Google Scholar
Uchida, Y.: 1968, Solar Phys. 4, 30.CrossRefGoogle Scholar
Uchida, Y.: 1970, Publ. Astron. Soc. Japan 22, 341.Google Scholar
Uchida, Y., Altschuler, M. D., and Newkirk, G. Jr.: 1973, Solar Phys. 28, 495.CrossRefGoogle Scholar
Vaiana, G. S. and Giacconi, R.: 1969, in Wentzel, D. G. and Tidman, D. A. (eds.), Plasma Instabilities in Astrophysics, Gordon and Breach, Publ., p. 91.Google Scholar
Valdez, J. and Altschuler, M. D.: 1970, Solar Phys. 15, 446.CrossRefGoogle Scholar
Valnicek, B.: 1968, in Kiepenheuer, K. O. (ed.), ‘Structure and Development of Solar Active Regions’, IAU Symp. 35, p. 282.Google Scholar
Veeder, G. J. and Zirin, H.: 1970, Solar Phys. 12, 391.CrossRefGoogle Scholar
Wilcox, J. M. and Ness, N. F.: 1965, J. Geophys. Res. 70, 5793.CrossRefGoogle Scholar
Wild, J. P.: 1970, Proc. Astron. Soc. Australia 1, 365.CrossRefGoogle Scholar
Wilson, P. R.: 1972, Proc. Astron. Soc. Australia 2, 144.CrossRefGoogle Scholar
Yoshimura, H.: 1971, Solar Phys. 18, 417.CrossRefGoogle Scholar
Zirin, H.: 1972, Solar Phys. 26, 145.CrossRefGoogle Scholar
Zirin, H. and Tanaka, K.: 1973, Solar Phys. 32, 173.CrossRefGoogle Scholar