This volume represents the state of the art of the science covered by the International Association of Geomagnetism and Aeronomy (IAGA) Division IV: Solar Wind and Interplanetary Field. It contains a collection of contributions by top experts addressing and reviewing a variety of topics included und
The Sun, the Solar Wind, and the Heliosphere || Current Sheets in the Solar Atmosphere
✍ Scribed by Miralles, Mari Paz; Sánchez Almeida, Jorge
- Book ID
- 118153338
- Publisher
- Springer Netherlands
- Year
- 2010
- Tongue
- Dutch
- Weight
- 534 KB
- Edition
- 2011
- Category
- Article
- ISBN
- 9048197872
No coin nor oath required. For personal study only.
✦ Synopsis
This volume represents the state of the art of the science covered by the International Association of Geomagnetism and Aeronomy (IAGA) Division IV: Solar Wind and Interplanetary Field. It contains a collection of contributions by top experts addressing and reviewing a variety of topics included under the umbrella of the division. It covers subjects that extend from the interior of the Sun to the heliopause, and from the study of physical processes in the Sun and the solar wind plasma to space weather forecasts. The book is organized in 6 parts: the solar interior, the solar atmosphere, the heliosphere, heliophysical processes, radio emissions, and coordinated science in the Sun-Earth system. In addition, we highlight some of the results presented during the IAGA Division IV symposia in the 11th Scientific Assembly of IAGA in Sopron, Hungary, on 23-30 August 2009, which was planned simultaneously with this book.
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This volume represents the state of the art of the science covered by the International Association of Geomagnetism and Aeronomy (IAGA) Division IV: Solar Wind and Interplanetary Field. It contains a collection of contributions by top experts addressing and reviewing a variety of topics included und
Neutral current sheets are expected to form in the solar atmosphere when photospheric motions or the emergence of new magnetic flux causes oppositely directed magnetic fields to he pressed together. Magnetic energy may thus be stored slowly in excess of the minimum energy associated with a purely po