The solar corona : proceedings of symposium E1 of the COSPAR Twenty-ninth Plenary Meeting held in Washington, DC, U.S.A., 28 August-5 September, 1992
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書誌事項
The solar corona : proceedings of symposium E1 of the COSPAR Twenty-ninth Plenary Meeting held in Washington, DC, U.S.A., 28 August-5 September, 1992
（Advances in space research, v. 14,
Pergamon, 1993
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内容説明・目次
内容説明
Present knowledge of the structure, physical properties and evolution of the quiet corona is limited and dispersed. It consists of coronagraph and eclipse data in the visible, a few XUV observations, broad-band X-ray images and radio observations. The papers presented in this volume emphasize the aspects of the corona which are always present - the so-called quiet corona - although work relating to activity and transient phenomena is also covered. New observations showing the corona to be very complex and dynamic over a wide range of time scales are examined. Regarding new ways of looking at old problems, these proceedings also include the three-dimensional structure of coronal streamers, the variation of element abundance between different solar structures, micro-flares as a mechanism for coronal heating and the possible existence of hot coronae in low-collision rate atmospheres without the need for a heating mechanism. The 30 papers contained in this volume encapsulate the current knowledge of solar corona and indicate the many avenues now open for future research.
目次
- Coronal observations from the soft X-ray telescope on Yohkoh, K.T. Strong and Yohkoh Team
- a statistical study of the coronal mass ejection phenomenon, R.A. Harrison
- coronal physics from eclipse observations, S. Koutchmy
- the solar cycle variation of coronal temperature and density during cycle 21-22, M. Guhathakurta et al
- redshifted transition region lines explained, V. Hansteen and P. Maltby
- three dimensional coronal structures using Clark Lake observations, E.J. Schmahl et al
- longitudinal structure of quasi-steady equatorial coronal holes near solar minima and their phase reversal, Gong-Liang Zhang and Yu-Fen Gao
- meter wavelength observations of the quiet sun and the slowly varying component during declining phase of the solar cycle, P. Lantos and C.E. Alissandrakis
- theoretical models for the solar wind, E. Marsch
- Alfven waves in the solar corona and solar wind, M. Velli
- the physics of coronal closed-field structures, Spiro K. Antiochos
- abundance determination in solar active region, B.C. Monsignori Fossi et al
- study of the quiet corona with the SOHO/SUMER spectrometer, P. Lemaire and K. Wilhelm
- coronal element abundances derived from solar energetic particles, D.V. Reames
- observations of the solar corona with Ulysses - expectations above the polar regions, K.-P. Wenzel and R.G. Marsden.
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