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  • 1
    Electronic Resource
    Electronic Resource
    Cosmic-Ray Propagation in the Galaxy: Collective Effects (1974)
    Palo Alto, Calif. : Annual Reviews
    Annual Review of Astronomy and Astrophysics 12 (1974), S. 71-96 
    Details
    ISSN: 0066-4146
    Source: Annual Reviews Electronic Back Volume Collection 1932-2001ff
    Topics: Physics
    Type of Medium: Electronic Resource
    URL: http://dx.doi.org/10.1146/annurev.aa.12.090174.000443
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    Paper (German National Licenses)
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  • 2
    Electronic Resource
    Electronic Resource
    Magnetic Fields and Spiral Structure (1963)
    Palo Alto, Calif. : Annual Reviews
    Annual Review of Astronomy and Astrophysics 1 (1963), S. 195-218 
    Details
    ISSN: 0066-4146
    Source: Annual Reviews Electronic Back Volume Collection 1932-2001ff
    Topics: Physics
    Type of Medium: Electronic Resource
    URL: http://dx.doi.org/10.1146/annurev.aa.01.090163.001211
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    Paper (German National Licenses)
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  • 3
    Electronic Resource
    Electronic Resource
    Report on the solar physics-plasma physics workshop (1976)
    Springer
    Solar physics 46 (1976), S. 411-431 
    Details
    ISSN: 1573-093X
    Source: Springer Online Journal Archives 1860-2000
    Topics: Physics
    Notes: Abstract This report summarizes the proceedings of a meeting held on 17–20 September 1974, at Stanford University. The purpose was to explore plasma physics problems which arise in the study of solar physics. Sessions were concerned with specific questions including the following: Is the solar plasma thermal or non-thermal? What spectroscopic data are required? What types of magnetic field structures exist? Do MHD instabilities occur? Do resistive or non-MHD instabilities occur? What mechanisms of particle acceleration have been proposed? What information do we have concerning shock waves? Very few questions were answered categorically but, for each question, there was discussion concerning the observational evidence, theoretical analyses, and existing or potential laboratory and numerical experiments.
    Type of Medium: Electronic Resource
    URL: http://dx.doi.org/10.1007/BF00149863
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    Paper (German National Licenses)
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  • 4
    Electronic Resource
    Electronic Resource
    Do changes in coronal emission structure imply magnetic reconnection? (1977)
    Springer
    Solar physics 55 (1977), S. 401-412 
    Details
    ISSN: 1573-093X
    Source: Springer Online Journal Archives 1860-2000
    Topics: Physics
    Notes: Abstract We examine three major possible interpretations of observed reconfigurations of coronal X-ray and XUV emitting structures on a scale comparable to the size of the structures themselves. One possibility is that little change in the large-scale magnetic field configuration is associated with the change in emission. The other two possibilities are processes by which the magnetic field structure can change. We demonstrate that large changes in visibility in X-rays or XUV lines can be associated with relatively minor changes in the coronal magnetic field by showing the behavior of magnetic interconnections between individual active regions in a complex of activity observed by the S-054 X-ray spectrographic telescope on Skylab. While the large-scale interconnections are continuously present for at least several days, individual loops in these structures are visible for only relatively short times (≲1 day). The two theoretical possibilities which we discuss are ‘frozen-in’ motion of the fields, and field line reconnection. We emphasize that reconnection occurs in regions much smaller than telescopic resolution. Because there are no measurements of the magnetic field in the corona in projection against the disk, existing observations are generally not sufficient to show in detail howmuch reconnection has occurred.
    Type of Medium: Electronic Resource
    URL: http://dx.doi.org/10.1007/BF00152583
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    Paper (German National Licenses)
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