André Balogh (ed.); Andrei Bykov (ed.); Robert P. Lin (ed.); John Raymond (ed.); Manfred Scholer (ed.) Springer (2013) Saatavuus: Tilaustuote Kovakantinen kirja
André Balogh (ed.); Andrei Bykov (ed.); Peter Cargill (ed.); Richard Dendy (ed.); Thierry Dudok de Wit (ed.); John Raymond Springer (2014) Saatavuus: Tilaustuote Kovakantinen kirja
André Balogh (ed.); Andrei Bykov (ed.); Peter Cargill (ed.); Richard Dendy (ed.); Thierry Dudok de Wit (ed.); John Raymond Springer (2016) Saatavuus: Tilaustuote Pehmeäkantinen kirja
André Balogh (ed.); Andrei Bykov (ed.); Robert P. Lin (ed.); John Raymond (ed.); Manfred Scholer (ed.) Springer (2015) Saatavuus: Tilaustuote Pehmeäkantinen kirja
Andrew F. Nagy (ed.); A. Balogh (ed.); Thomas E. Cravens (ed.); Michael Mendillo (ed.); Ingo Müller-Wodarg (ed.) Springer (2010) Saatavuus: Tilaustuote Pehmeäkantinen kirja
Rainer Beck (ed.); Andre Balogh (ed.); D. V. Bykov (ed.); Rudolf A. Treumann (ed.); Lawrence Widrow (ed.) Springer (2014) Saatavuus: Tilaustuote Pehmeäkantinen kirja
Daniel Baker (ed.); André Balogh (ed.); Tamas Gombosi (ed.); Hannu E. J. Koskinen (ed.); Astrid Veronig (ed.); von Steiger Springer (2018) Saatavuus: Tilaustuote Kovakantinen kirja
Daniel Baker (ed.); André Balogh (ed.); Tamas Gombosi (ed.); Hannu E. J. Koskinen (ed.); Astrid Veronig (ed.); von Steiger Springer (2019) Saatavuus: Tilaustuote Pehmeäkantinen kirja
Springer Sivumäärä: 640 sivua Asu: Kovakantinen kirja Painos: 2013 Julkaisuvuosi: 2013, 11.01.2013 (lisätietoa) Kieli: Englanti
The review articles collected in this volume present a critical assessment of particle acceleration mechanisms and observations from suprathermal particles in the magnetosphere and heliosphere to high-energy cosmic rays, thus covering a range of energies over seventeen orders of magnitude, from 103 eV to 1020 eV. The main themes are observations of accelerated populations from the magnetosphere to extragalactic scales and assessments of the physical processes underlying particle acceleration in different environments (magnetospheres, the solar atmosphere, the heliosphere, supernova remnants, pulsar wind nebulae and relativistic outflows). Several contributions review the status of shock acceleration in different environments and also the role of turbulence in particle acceleration. Observational results are compared with modelling in different parameter regimes. The book concludes with contributions on the status of particle acceleration research and its future perspectives.
This volume is aimed at graduate students and researchers active in astrophysics and space science.
Previously published in Space Science Reviews journal, Vol. 173 Nos. 1-4, 2012.
