Abstract
Force-free magnetic field extrapolation for region McMath 12417 on 4 July 1973 corroborates a suggestion by Roy and Michalitsanos (1974): A large moving magnetic feature presses together opposite fluxes to form an X-type neutral sheet; the supposed geometry of the field as derived from chromospheric activity (subflares, ejections) is confirmed by the calculated lines of force.
Similar content being viewed by others
References
Altschuler, M. D., Levine, R. H., Stix, M., and Harvey, J.: 1977, Solar Phys. 51, 345.
Bachmann, G.: 1978, Bull. Astron. Inst. Czech. 29, 180
Bachmann, G., Jäger, F. W., Künzel, H., Pflug, K., and Staude, J.: 1975, HHI-STP Report No. 4, Zentralinstitut für solar-terrestrische Physik, Berlin-Adlershof.
Bray, R. J.: 1974, Solar Phys. 38, 377.
Howard, R. and Švestka, Z.: 1977, Solar Phys. 54, 65.
Loughhead, R. E.: 1974, Solar Phys. 38, 77.
Maltby, P.: 1975, Solar Phys. 43, 91.
Roy, J.-R. and Michalitsanos, A. G.: 1974, Solar Phys. 35, 47.
Seehafer, N.: 1978, Solar Phys. 58, 215.
Seehafer, N. and Staude, J.: 1979, Astron. Nachr. 300, 151.
Švestka, Z., Solodyna, C. V., Howard, R., and Levine, R. H.: 1977, Solar Phys. 55, 359.
Tang, F.: 1978, Solar Phys. 60, 119.
Zirin, H.: 1974a, in R. G. Athay (ed.), ‘Chromospheric Fine Structure’, itIAU Symp. 56, 161.
Zirin, H.: 1974b, Solar Phys. 38, 91.
Author information
Authors and Affiliations
Rights and permissions
About this article
Cite this article
Seehafer, N., Staude, J. Evidence for an X-type neutral sheet producing chromospheric activity. Sol Phys 67, 121–125 (1980). https://doi.org/10.1007/BF00146688
Received:
Issue Date:
DOI: https://doi.org/10.1007/BF00146688