Nonlinearity and Instability in Stellar Coronae

Details Nonlinearity and Instability in Stellar Coronae Nonlinearity and Instability in Stellar Coronae

Jan 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983phdt.......138m&link_type=abstract

Ph.D. Thesis, University of Utrecht, The Netherlands

Statistics

Applications

Coronae, Winds, Thermal Stability, Nonlinear Methods

Scientific paper

This thesis consists of three parts. Chapter 2, the first part, reviews applications of nonlinear methods in astronomy, in particular in stellar coronae. Chapters 3, 4, and 5, the second part, deal with various aspects of the acceleration and thermal stability of stellar winds, while chapters 6 through 9 consider the thermal structure and stability of the plasma in closed coronal loops, such as observed on the Sun. All chapters have been published as papers in refereed journals.

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