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How to improve our understanding of solar wind-magnetosphere interactions on the basis of the statistical evaluation of the energy budget in the magnetosheath?
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- Vörös, Zoltán (författare)
- Space Research Institute, Austrian Academy of Sciences, Graz, Austria; Institute of Earth Physics and Space Science, Sopron, Hungary,Austrian Acad Sci, Space Res Inst, Graz, Austria.;Inst Earth Phys & Space Sci, Sopron, Hungary.
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- Roberts, Owen W. (författare)
- Space Research Institute, Austrian Academy of Sciences, Graz, Austria,Austrian Acad Sci, Space Res Inst, Graz, Austria.
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- Yordanova, Emiliya (författare)
- Uppsala universitet,Institutet för rymdfysik, Uppsalaavdelningen
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- Sorriso Valvo, Luca (författare)
- Uppsala universitet,KTH,Rymd- och plasmafysik,Swedish Institute of Space Physics, Uppsala, Sweden; CNR/ISTP—Istituto per la Scienza e la Tecnologia dei Plasmi, Bari, Italy,Institutet för rymdfysik, Uppsalaavdelningen,CNR, ISTP Ist Sci & Tecnol Plasmi, Bari, Italy.;KTH Royal Inst Technol, Sch Elect Engn & Comp Sci, Space & Plasma Phys, Stockholm, Sweden.
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- Nakamura, Rumi (författare)
- Space Research Institute, Austrian Academy of Sciences, Graz, Austria,Austrian Acad Sci, Space Res Inst, Graz, Austria.
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- Narita, Yasuhito (författare)
- Space Research Institute, Austrian Academy of Sciences, Graz, Austria,Austrian Acad Sci, Space Res Inst, Graz, Austria.
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- Schmid, Daniel (författare)
- Space Research Institute, Austrian Academy of Sciences, Graz, Austria,Austrian Acad Sci, Space Res Inst, Graz, Austria.
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- Plaschke, Ferdinand (författare)
- Institut für Geophysik und Extraterrestrische Physik, TUBraunschweig, Germany,TUBraunschweig, Inst Geophys & Extraterr Phys, Braunschweig, Germany.
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- Kis, Árpád (författare)
- Institute of Earth Physics and Space Science, Sopron, Hungary,Inst Earth Phys & Space Sci, Sopron, Hungary.
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Space Research Institute, Austrian Academy of Sciences, Graz, Austria; Institute of Earth Physics and Space Science, Sopron, Hungary Austrian Acad Sci, Space Res Inst, Graz, Austria;Inst Earth Phys & Space Sci, Sopron, Hungary. (creator_code:org_t)
- Frontiers Media SA, 2023
- 2023
- Engelska.
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Ingår i: Frontiers in Astronomy and Space Sciences. - : Frontiers Media SA. - 2296-987X. ; 10
- Relaterad länk:
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https://doi.org/10.3...
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https://uu.diva-port... (primary) (Raw object)
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https://urn.kb.se/re...
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https://doi.org/10.3...
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https://urn.kb.se/re...
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Abstract
Ämnesord
Stäng
- Solar wind (SW) quantities, referred to as coupling parameters (CPs), are often used in statistical studies devoted to the analysis of SW–magnetosphere–ionosphere couplings. Here, the CPs and their limitations in describing the magnetospheric response are reviewed. We argue that a better understanding of SW magnetospheric interactions could be achieved through estimations of the energy budget in the magnetosheath (MS), which is the interface region between the SW and magnetosphere. The energy budget involves the energy transfer between scales, energy transport between locations, and energy conversions between electromagnetic, kinetic, and thermal energy channels. To achieve consistency with the known multi-scale complexity in the MS, the energy terms have to be complemented with kinetic measures describing some aspects of ion–electron scale physics.
Ämnesord
- NATURVETENSKAP -- Fysik -- Astronomi, astrofysik och kosmologi (hsv//swe)
- NATURAL SCIENCES -- Physical Sciences -- Astronomy, Astrophysics and Cosmology (hsv//eng)
- TEKNIK OCH TEKNOLOGIER -- Naturresursteknik -- Energisystem (hsv//swe)
- ENGINEERING AND TECHNOLOGY -- Environmental Engineering -- Energy Systems (hsv//eng)
Nyckelord
- coupling parameters
- energy budget
- magnetosphere
- solar wind
- turbulence
Publikations- och innehållstyp
- ref (ämneskategori)
- art (ämneskategori)
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