The Heliosphere at Solar Minimum and beyond
Published on 29. July 1997
Book
Paperback/Softback
160 pages
978-0-08-043107-9 (ISBN)
Description
The Heliosphere is the large volume of space dominated by the expanding solar atmosphere. Even the most distant spacecraft, now at more than sixty Astronomical Units (1 Astronomical Unit = 150 million kilometers) from the sun, have yet to encounter the boundary between the Heliosphere and interstellar space. This publication contains 30 papers, reporting observations made throughout the Heliosphere and presenting theories to explain these observations. The results of the Ulysses spacecraft mission, the first to explore the Heliosphere over the solar poles, are summarised. Modulation of the galactic cosmic radiation and energetic solar particles by heliospheric structures is discussed. New results on the anomalous component of cosmic radiation are given, and predictions are made as to where the boundary of the Heliosphere may be found.
The Heliosphere is the large volume of space dominated by the expanding solar atmosphere. Even the most distant spacecraft, now at more than sixty Astronomical Units (1 Astronomical Unit = 150 million kilometers) from the sun, have yet to encounter the boundary between the Heliosphere and interstellar space. This publication contains 30 papers, reporting observations made throughout the Heliosphere and presenting theories to explain these observations. The results of the Ulysses spacecraft mission, the first to explore the Heliosphere over the solar poles, are summarised. Modulation of the galactic cosmic radiation and energetic solar particles by heliospheric structures is discussed. New results on the anomalous component of cosmic radiation are given, and predictions are made as to where the boundary of the Heliosphere may be found.
The Heliosphere is the large volume of space dominated by the expanding solar atmosphere. Even the most distant spacecraft, now at more than sixty Astronomical Units (1 Astronomical Unit = 150 million kilometers) from the sun, have yet to encounter the boundary between the Heliosphere and interstellar space. This publication contains 30 papers, reporting observations made throughout the Heliosphere and presenting theories to explain these observations. The results of the Ulysses spacecraft mission, the first to explore the Heliosphere over the solar poles, are summarised. Modulation of the galactic cosmic radiation and energetic solar particles by heliospheric structures is discussed. New results on the anomalous component of cosmic radiation are given, and predictions are made as to where the boundary of the Heliosphere may be found.
More details
Series
Language
English
Place of publication
Amsterdam
Netherlands
Publishing group
Elsevier Science & Technology
Target group
College/higher education
Professional and scholarly
ISBN-13
978-0-08-043107-9 (9780080431079)
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Schweitzer Classification
Content
Selected papers: Preface (D.E. Page, R.G. Marsden). Ulysses: A summary of the first high-latitude survey (R.G. Marsden, E.J. Smith). On-line access to heliospheric measurements at high latitudes using the ESA archive for Ulysses data (C. Tranquille et al. ). Ulysses observations of intermittent heliospheric turbulence (T.S. Horbury et al. ). Acceleration and modulation of energetic particles in the 3-D heliosphere by corotating interaction regions (G.M. Simnett, E.C. Roelof). A large magnetic depression observed in the solar wind close to the Earth's bow shock (G. Chisham et al. ). Low frequency plasma waves in the solar wind: from ecliptic plane to the solar polar regions (N. Lin et al. ). Cosmic ray latitudinal effects predicted by a three-dimensional drift model (M. Hattingh et al. ). An alternative approach to the modelling of galactic cosmic ray intensities in the heliosphere (J.P.L. Reinecke et al. ). MeV to GeV electron propagation and modulation: results of the KET telescope on board Ulysses (P. Ferrando). North-South cosmic ray asymmetry and high speed solar wind (A.K. Svirzhevskaya et al. ). The cosmic ray intensity averaged over the longitude in the tilted-current-sheet heliosphere (M.S. Kalinin, M.B. Krainev). Interstellar neutral hydrogen in the heliosphere (Y.C. Whang). Distribution of ACR ions in the heliosheath and the related ENA flux (A. Czechowski, S. Grzedzielski). Pioneer 10 and Voyagers 1 and 2 backscattered UV data and the nature of the interstellar medium (P. Gangopadhyay et al. ). The solar wind termination shock in the presence of cosmic rays and interstellar neutrals (J. Ziemkiewicz, M. Banaszkiewicz). The electric field beyond the termination shock and some possible GCR and ACR effects (M.S. Kalinin, M.B. Krainev).