Eruptive Solar Flares 爆发的太阳耀斑 第1版

基本信息

Format Paperback | 409 pages

Dimensions 170 x 244 x 21.84mm | 728g

Publication date 20 Nov 2013

Publisher Springer-Verlag Berlin and Heidelberg GmbH & Co. KG

Imprint Springer-Verlag Berlin and Heidelberg GmbH & Co. K

Edition Statement Softcover reprint of the original 1st ed. 1992

ISBN10 3662138743

ISBN13 9783662138748

页面参数仅供参考，具体以实物为准

书籍简介

这是一份对当今太阳研究的详尽调查，包括理论和观测。它涉及到爆发性耀斑、X射线和无线电波中的丝状爆发、能量释放和传输，以及地球对太阳耀斑的反应。还介绍了最近SOLAR-A项目（在会议后不久启动）的细节。

This is an exhaustive survey of present-day solar research including both theory and observations. It deals with eruptive flares, filament eruption in x-rays and radio waves, energy release and transport, and terrestrial response to solar flares. Details of the most recent SOLAR-A project (launched shortly after the conference) are also presented.

目录

作者简介

Zdenek Svestka , Bernard V. Jackson , Marcos E. Machado

兹登克·维斯卡是一名捷克天文学家。几十年来，他是世界上研究太阳耀斑的主要专家。他在布拉格查尔斯大学学习数学和物理，直到1948年毕业。他和科内利斯·德·贾格尔是《太阳物理学》杂志的联合创始人和编辑。38年来，从1967年《华尔街日报》创刊到2005年退休，他负责所有关于太阳耀斑的论文，而德·贾格尔则负责其他一切。小行星17805灶神星是以他的名字命名的。

Zdeněk Švestka (30 September 1925 – 2 March 2013) was a Czech astronomer. For several decades he was the world's leading expert on solar flares. He studied mathematics and physics at Charles University, Prague, until graduating in 1948. Together with Cornelis de Jager, he was the co-founder and editor of the journal Solar Physics. For 38 years, from the establishment of the journal in 1967 until his retirement in 2005, he handled all papers on solar flares, while De Jager took care of everything else. The minor planet 17805 Švestka was named after him.[1]

伯纳德·V·杰克逊

我的研究领域是太阳和日光层物理。特别是，我对日冕、太阳风和日光层内的瞬变现象感兴趣。

我们在加州大学圣地亚哥分校的研究小组已经开发了一个设施，用于处理来自HELIOS航天器黄道带光度计的档案数据。利用这些数据和行星际闪烁（IPS）数据，我们可以在三维空间中重建太阳风结构，并着眼于空间天气预报。

目前，我是太阳质量抛射成像仪（SMEI）的共同研究者，该仪器目前正在建造中。SMEI将在加州大学圣地亚哥分校和英国伯明翰大学为美国空军科里奥利任务开发的一个地球轨道航天器上飞行。我还参与了SOHO LASCO冠状仪的工作。

Bernard V. Jackson

My research area is Solar and Heliospheric Physics. In particular, I am interested in the solar corona, the solar wind, and transient phenomena within the heliosphere.

Our group here at UCSD has developed a facility for processing archival data from the HELIOS spacecraft Zodiacal Light Photometers. Using this and interplanetary scintillation (IPS) data allows us to reconstruct solar wind structures in 3 dimensions, with an eye toward space weather forecasting.

Currently, I am co-investigator on the Solar Mass Ejection Imager, (SMEI), now under construction. SMEI will fly on an Earth-orbiting spacecraft being developed for the U.S.Air Force Coriolis Mission by UC San Diego and the University of Birmingham,in Birmingham,England. I am also involved with the SOHO LASCO coronograph instrumentation.

马科斯·E·马查多于1971年毕业于阿根廷布宜诺斯艾利斯的拉普拉塔国立大学的天文学专业。他在科罗拉多大学博尔德分校继续深造，直到1974年，并在实验室天体物理学联合研究所和萨克拉门托峰天文台担任短期助理研究员的职务。从1977年到1979年，他在哈佛-史密森天体物理学中心担任研究员。他的几篇关于太阳大气的光谱分析和建模的文章属于这个时期，至今仍被引用。

Marcos E. Machado graduated in Astronomy at Universidad Nacional de La Plata, Buenos Aires, Argentina, in 1971. He continued his education at the University of Colorado, Boulder, until 1974, and held short-term positions as assistant researcher at the Joint Institute for Laboratory Astrophysics and Sacramento Peak Observatory. From 1977 until 1979, he was research fellow at the Harvard-Smithsonian Center for Astrophysics. Several of his most and still cited articles on spectral analysis and modelling of the solar atmosphere belong to this period.