Abstract
We are now at both the maximum of the solar activity cycle and at the most populated part of the saros. I discuss the solar corona over the recent saros and its changes with the solar activity cycle. We consider the scientific value of eclipse studies and how they relate to other ongoing coronal studies on the sun and other stars.
References
Chandrasekhar, T., Desai, J.N., Ashok, N.M., Pasachoff, J.M.: 1991, Solar Phys., in press
Pasachoff, J.M.: 1991a, Eclipses of the Sun in The Reference Encyclopedia of Astronomy a and Astrophysics, in press
Pasachoff, J.M.: 1991b, Proc. Heidelberg Conf. on Mechanisms of Chrom. and Coronal Heating, ed. by P. Ulmschneider, E. Priest, R. Rosner (Springer-Verlag), in press
Pasachoff, J.M., Landman, D.A.: 1984, Solar Phys. 90, 325
Pasachoff, J.M., Ladd, E.F.: 1987, Solar Phys. 109, 365; 110, 412
Pasachoff, J.M., Sandford, II, M.T., Keller, Jr., C. F., Jr.: 1978, Bull. Am. Astron. Soc. 10,431
Author information
Authors and Affiliations
Editor information
Rights and permissions
Copyright information
© 1991 Springer-Verlag
About this paper
Cite this paper
Pasachoff, J.M. (1991). The solar corona over the recent saros. In: Tuominen, I., Moss, D., Rüdiger, G. (eds) The Sun and Cool Stars: activity, magnetism, dynamos. Lecture Notes in Physics, vol 380. Springer, Berlin, Heidelberg. https://doi.org/10.1007/3-540-53955-7_144
Download citation
DOI: https://doi.org/10.1007/3-540-53955-7_144
Published:
Publisher Name: Springer, Berlin, Heidelberg
Print ISBN: 978-3-540-53955-1
Online ISBN: 978-3-540-46483-9
eBook Packages: Springer Book Archive