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Reiner Gamma albedo...
Reiner Gamma albedo features reproduced by modeling solar wind standoff
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- Deca, Jan (författare)
- Univ Colorado Boulder, Lab Atmospher & Space Phys, Boulder, CO USA; NASA SSERVI, Inst Modeling Plasma Atmospheres & Cosm Dust, Moffett Field, CA USA; Univ Versailles St Quentin, Lab Atmospheres Milieux Observat Spatiales, Guyancourt, France
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- Divin, Andrey (författare)
- Uppsala universitet,Institutet för rymdfysik, Uppsalaavdelningen,St Petersburg State Univ, Phys Dept, St Petersburg, Russia; Swedish Inst Space Phys, Uppsala, Sweden
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- Lue, Charles (författare)
- Univ Iowa, Dept Phys & Astron, Iowa City, IA USA; Swedish Inst Space Phys, Kiruna, Sweden
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- Ahmadi, Tara (författare)
- St Petersburg State Univ, Phys Dept, St Petersburg, Russia
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- Horanyi, Mihaly (författare)
- Univ Colorado Boulder, Lab Atmospher & Space Phys, Boulder, CO USA; NASA SSERVI, Inst Modeling Plasma Atmospheres & Cosm Dust, Moffett Field, CA USA
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(creator_code:org_t)
- 2018-04-19
- 2018
- Engelska.
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Ingår i: Communications Physics. - : Springer Science and Business Media LLC. - 2399-3650. ; 1
- Relaterad länk:
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https://doi.org/10.1...
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https://uu.diva-port... (primary) (Raw object)
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https://www.nature.c...
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https://urn.kb.se/re...
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https://doi.org/10.1...
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Abstract
Ämnesord
Stäng
- All lunar swirls are known to be co-located with crustal magnetic anomalies (LMAs). Not all LMAs can be associated with albedo markings, making swirls, and their possible connection with the former, an intriguing puzzle yet to be solved. By coupling fully kinetic simulations with a Surface Vector Mapping model, we show that solar wind standoff, an ion–electron kinetic interaction mechanism that locally prevents weathering by solar wind ions, reproduces the shape of the Reiner Gamma albedo pattern. Our method reveals why not every magnetic anomaly forms a distinct albedo marking. A qualitative match between optical remote observations and in situ particle measurements of the back-scattered ions is simultaneously achieved, demonstrating the importance of a kinetic approach to describe the solar wind interaction with LMAs. The anti-correlation between the predicted amount of surface weathering and the surface reflectance is strongest when evaluating the proton energy flux.
Ämnesord
- NATURVETENSKAP -- Fysik -- Astronomi, astrofysik och kosmologi (hsv//swe)
- NATURAL SCIENCES -- Physical Sciences -- Astronomy, Astrophysics and Cosmology (hsv//eng)
Publikations- och innehållstyp
- ref (ämneskategori)
- art (ämneskategori)
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