Search: onr:"swepub:oai:DiVA.org:uu-3478" >
Substorm Features i...
Substorm Features in the High-Latitude Ionosphere and Magnetosphere : Multi-Instrument Observations
-
- Borälv, Eva (author)
- Uppsala universitet,Institutet för rymdfysik, Uppsalaavdelningen
-
Opgenoorth, Hermann (thesis advisor)
-
- Lester, Mark, Professor (opponent)
- Radio and Space Plasma Physics Group, Dept. Physics and Astronomy, University of Leicester, Leicester
-
(creator_code:org_t)
- ISBN 9155456707
- Uppsala : Acta Universitatis Upsaliensis, 2003
- English 50 s.
-
Series: Comprehensive Summaries of Uppsala Dissertations from the Faculty of Science and Technology, 1104-232X ; 860
- Related links:
-
https://uu.diva-port... (primary) (Raw object)
-
show more...
-
https://urn.kb.se/re...
-
show less...
Abstract
Subject headings
Close
- The space around Earth, confined in the terrestrial magnetosphere, is to some extent shielded from the Sun's solar wind plasma and magnetic field. During certain conditions, however, strong interaction can occur between the solar wind and the magnetosphere, resulting in magnetospheric activity of several forms, among which substorms and storms are the most prominent. A general framework for how these processes work have been outlayed through the history of research, however, there still remain questions to be answered. The most striking example regards the onset of substorms, where both the onset cause and location in the magnetosphere/ionosphere are still debated. These are clearly not easily solved problems, since a substorm is a global process, ideally requiring simultaneous measurements in the magnetotail and ionosphere. Investigated in this work are temporal and spatial scales for substorm and convection processes in the Earth's magnetosphere and ionosphere. This is performed by combining observations from a number of both ground-based and spacecraft-borne instruments. The observations indicate that the magnetotail's cross-section is involved to a larger spatial extent than previously considered in the substorm process. Furthermore, convection changes result in topological changes of the magnetosphere on a fast time scale. The results show that the magnetosphere is, on a global magnetospheric scale, highly dynamic during convection changes and ensuing substorms.
Subject headings
- NATURVETENSKAP -- Fysik -- Fusion, plasma och rymdfysik (hsv//swe)
- NATURAL SCIENCES -- Physical Sciences -- Fusion, Plasma and Space Physics (hsv//eng)
Keyword
- Space and plasma physics
- Substorm
- Convection
- magnetosphere-ionosphere coupling
- Rymd- och plasmafysik
- Space physics
- Rymdfysik
- Space and Plasma Physics
- rymd- och plasmafysik
Publication and Content Type
- vet (subject category)
- dok (subject category)
Find in a library
To the university's database