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Magnetic Fields in the Solar Atmosphere
This paper describes the magnetic field configurations observed in the solar atmosphere including the corona and the solar wind. The techniques for observing solar magnetic fields are briefly reviewed. The significance of Alfven waves in transporting energy is stressed. (Author).
Exploring the Unknown
NASA SP-2004-4407. NASA History Series. Edited by John M. Logsdon, et al. 6th in a series containing a selection of key documents in the history of the United States civil space program. Includes chapters on solar physics, space physics, life sciences, and Earth science. LC. card 96-9066.
Solar and Stellar Granulation
Robert J. Rutten Sterrekundig Instituut Utrecht, The Netherlands Why this workshop? Why this workshop? Or rather, since the real question that arose about a year ago was not whether there should be another OAC workshop, but only what it should be about: why a workshop on granulation? To answer this question I will play an unfair trick on you. I will simply present the scientific justification which I included last autumn in a grant application to NATO's Scientific Affairs Division. It lists the reasons why I thought a workshop on this particular topic and at this particular moment ought to be worthwhile. There must be something in its reasoning, because NATO has indeed agreed to co-sponsor t...
A Table of Zeeman Multiplets
The table lists the Zeeman multiplets for transitions of astrophysical interest assuming Russell-Saunders (LS) coupling. (Author).
Motions in the Solar Atmosphere
The report presents two papers on observational evidence for large and small scale motions in the solar atmosphere.
Solar Surface Magnetism
Observations of the solar magnetic field are largely confined to the radiation emitted from the photosphere, the thin layer of the solar atmosphere which we call "the solar surface". It is from solar surface observations that we must infer the internal structure and the internal magnetohydrodynamic processes that lead to the multitude of fascinat ing phenomena of solar magnetic activity, and from solar surface observations we must also infer the interplay of convection and magnetism that regulates field dispersal, drives the heating of the outer-atmospheric plasma, and generates the solar wind. There is much to be learned from solar surface magnetism in physics and astrophysics; currently, t...
