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Observational Plasma Astrophysics: Five Years of Yohkoh and Beyond (Hardcover, 1998 ed.): Tetsuya Watanabe, Takeo Kosugi,... Observational Plasma Astrophysics: Five Years of Yohkoh and Beyond (Hardcover, 1998 ed.)
Tetsuya Watanabe, Takeo Kosugi, Alphonse C. Sterling
R4,349 Discovery Miles 43 490 Ships in 12 - 17 working days

Since its launch in 1991, the Yohkoh satellite has been returning unprecedented observations of solar flares and the dynamic solar corona. This book is a collection of papers presented at a meeting held in: Yoyogi, Tokyo, on the occasion of Yohkoh's fifth anniversary of operation. The papers constitute a summary of observations and results over the five years, including contributions based on data from Yohkoh's hard and soft X-ray telescopes and its spectrometer experiments. The five years of data, covering approximately one-half of a solar cycle, reveal a fresh perspective on solar science, with a new picture of solar flares and the active Sun emerging. Also, for the first time there are extensive results from Yohkoh observations of the Sun during the solar minimum period. This wide-ranging volume will be of interest to workers in solar physics and X-ray astronomy. It also contains material appropriate for supplemental reading for graduate students in solar physics.

Observational Plasma Astrophysics: Five Years of Yohkoh and Beyond (Paperback, Softcover reprint of the original 1st ed. 1998):... Observational Plasma Astrophysics: Five Years of Yohkoh and Beyond (Paperback, Softcover reprint of the original 1st ed. 1998)
Tetsuya Watanabe, Takeo Kosugi, Alphonse C. Sterling
R4,269 Discovery Miles 42 690 Ships in 10 - 15 working days

Since its launch in 1991, the Yohkoh satellite has been returning unprecedented observations of solar flares and the dynamic solar corona. This book is a collection of papers presented at a meeting held in: Yoyogi, Tokyo, on the occasion of Yohkoh's fifth anniversary of operation. The papers constitute a summary of observations and results over the five years, including contributions based on data from Yohkoh's hard and soft X-ray telescopes and its spectrometer experiments. The five years of data, covering approximately one-half of a solar cycle, reveal a fresh perspective on solar science, with a new picture of solar flares and the active Sun emerging. Also, for the first time there are extensive results from Yohkoh observations of the Sun during the solar minimum period. This wide-ranging volume will be of interest to workers in solar physics and X-ray astronomy. It also contains material appropriate for supplemental reading for graduate students in solar physics.

Magnetodynamic Phenomena in the Solar Atmosphere - Prototypes of Stellar Magnetic Activity (Paperback, Softcover reprint of the... Magnetodynamic Phenomena in the Solar Atmosphere - Prototypes of Stellar Magnetic Activity (Paperback, Softcover reprint of the original 1st ed. 1996)
Yutaka Uchida, Takeo Kosugi, Hugh S. Hudson
R1,584 Discovery Miles 15 840 Ships in 10 - 15 working days

These are the Proceedings of Colloquium No. 153 of the International Astro nomical Union, held at Makuhari near Tokyo on May 22 - 26, 1995, and hosted by the National Astronomical Observatory. This meeting was intended to be an interdisciplinary meeting between re searchers of solar and stellar activity, in order for them to exchange the newest information in each field. While each of these areas has seen remarkable advances in recent years, and while the researchers in each field have felt that information from the other's domain would be extremely useful in their own work, there have not been very many opportunities for intensive exchanges of information between these closely related fields. We therefore expected much from this meeting in pro viding stellar researchers with new results of research on the counterparts of their targets of research, spatially and temporarily resolved, as observed on the Sun. Likewise we hoped to provide solar researchers with new results on gigantic ver sions of their targets of research under the very different physical circumstances on other active stars. It was our greatest pleasure that we had wide attendance of experts and active researchers of both research fields from all over the world. This led to extremely interesting talks and very lively discussions, thereby stimulating the exchange of ideas across the fields.

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