SOLAR WIND TEN: Proceedings of the Tenth International Solar Wind Conference Marco Velli, Università di Firenze, Dipartimento di Astronomia e Scienza dello Spazio, Firenze, ITALY ; Francesco Malara, Università della Calabria, Dipartimento di Fisica, Arcavacata di Rende, ITALY ; Roberto Bruno, IFSI, Roma, ITALY AIP Conference Proceedings 679 The papers were peer reviewed. The Tenth Solar Wind conference describes the latest results in the physics of the outer solar atmosphere, the solar wind, and the interplanetary medium which together comprise the heliosphere. The conference brought together researchers studying the sun and its influence on the earth’s space environment both from an experimental and theoretical point of view. The effect of the solar magnetic field in shaping and accelerating the solar wind throughout the solar cycle, via coronal heating and coronal mass ejections was described in unprecedented clarity and breadth, thanks to both satellite experiments and numerical modelling. The conference proceedings is of interest to researchers in space science and the geomagnetic effects of solar activity, plasma physicists and astrophysicists as well as other scientists interested in the life of our mother star. The structure of the heliosphere in 3 dimensions was both theoretically and experimentally described here for the first time at both solar minimum and maximum.
SOLAR WIND TEN, PROCEEDINGS OF THE TENTH INTERNATIONAL SOLAR WIND CONFERENCE / M. VELLI; R. BRUNO; F. MALARA. - STAMPA. - (2003).
SOLAR WIND TEN, PROCEEDINGS OF THE TENTH INTERNATIONAL SOLAR WIND CONFERENCE.
VELLI, MARCO;
2003
Abstract
SOLAR WIND TEN: Proceedings of the Tenth International Solar Wind Conference Marco Velli, Università di Firenze, Dipartimento di Astronomia e Scienza dello Spazio, Firenze, ITALY ; Francesco Malara, Università della Calabria, Dipartimento di Fisica, Arcavacata di Rende, ITALY ; Roberto Bruno, IFSI, Roma, ITALY AIP Conference Proceedings 679 The papers were peer reviewed. The Tenth Solar Wind conference describes the latest results in the physics of the outer solar atmosphere, the solar wind, and the interplanetary medium which together comprise the heliosphere. The conference brought together researchers studying the sun and its influence on the earth’s space environment both from an experimental and theoretical point of view. The effect of the solar magnetic field in shaping and accelerating the solar wind throughout the solar cycle, via coronal heating and coronal mass ejections was described in unprecedented clarity and breadth, thanks to both satellite experiments and numerical modelling. The conference proceedings is of interest to researchers in space science and the geomagnetic effects of solar activity, plasma physicists and astrophysicists as well as other scientists interested in the life of our mother star. The structure of the heliosphere in 3 dimensions was both theoretically and experimentally described here for the first time at both solar minimum and maximum.I documenti in FLORE sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.