Vladimir Florinski (ed.) | Akateeminen Kirjakauppa

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PHYSICS OF THE OUTER HELIOSPHERE : 3RD INTERNATIONAL IGPP CONFERENCE

Vladimir Florinski (ed.); Nikolai V. Pogorelov (ed.); Gary P. Zank (ed.)
American Institute of Physics (2004)
Kovakantinen kirja

163,40 €

PARTIALLY IONIZED PLASMAS THROUGHOUT THE COSMOS - PROCEEDINGS OF THE 2010 HUNTSVILLE WORKSHOP

Vladimir Florinski (ed.); Jacob Heerikhuisen (ed.); Gary P. Zank (ed.); Dennis L. Gallagher (ed.)
American Institute of Physics (2011)
Pehmeäkantinen kirja

112,30 €

PHYSICS OF THE INNER HELIOSHEATH : VOYAGER OBSERVATIONS, THEORY, AND FUTURE PROSPECTS; 5TH IGPP INTERNATIONAL ASTROPHYSICS CONFE

Jacob Heerikhuisen (ed.); Vladimir Florinski (ed.); Gary P. Zank (ed.); Nikolai V. Pogorelov (ed.)
American Institute of Physics (2006)
Kovakantinen kirja

112,10 €

PICKUP IONS THROUGHOUT THE HELIOSPHERE AND BEYOND : PROCEEDINGS OF THE 9TH INTERNATIONAL ASTROPHYSICS CONFERENCE

Jakobus Roux (ed.); Gary Zank (ed.); Andrew J. Coates (ed.); Vladimir Florinski (ed.)
American Institute of Physics (2010)
Kovakantinen kirja

121,30 €

Physics of the Outer Heliosphere : 3rd International IGPP Conference

Vladimir Florinski (ed.), Nikolai V. Pogorelov (ed.), Gary P. Zank (ed.)

163,40 €

American Institute of Physics
Sivumäärä: 431 sivua
Asu: Kovakantinen kirja
Painos: 2004
Julkaisuvuosi: 2004, 20.10.2004 (lisätietoa)
Kieli: Englanti
Tuotesarja: Astronomy and Astrophysics

This volume consists of articles written by leading scientists in the field of heliospheric physics, analyzing the latest spacecraft measurements and theoretical models related to the solar wind interaction with the Local Interstellar Medium. Particular focus is on the puzzling Voyager cosmic-ray and magnetic field data in the vicinity of the termination shock, and their possible theoretical interpretations. The purposes of future spacecraft missions and modeling issues are also discussed. Topics include: global structure of the outer heliosphere; spacecraft measurements: present and future; galactic and anomalous cosmic rays; shock structure, turbulence and kinetic physics; and remote sensing of the distant heliosphere and Local Interstellar Medium.

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