Literature DB >> 16484488

Plasma acceleration above martian magnetic anomalies.

R Lundin1, D Winningham, S Barabash, R Frahm, M Holmström, J-A Sauvaud, A Fedorov, K Asamura, A J Coates, Y Soobiah, K C Hsieh, M Grande, H Koskinen, E Kallio, J Kozyra, J Woch, M Fraenz, D Brain, J Luhmann, S McKenna-Lawler, R S Orsini, P Brandt, P Wurz.   

Abstract

Auroras are caused by accelerated charged particles precipitating along magnetic field lines into a planetary atmosphere, the auroral brightness being roughly proportional to the precipitating particle energy flux. The Analyzer of Space Plasma and Energetic Atoms experiment on the Mars Express spacecraft has made a detailed study of acceleration processes on the nightside of Mars. We observed accelerated electrons and ions in the deep nightside high-altitude region of Mars that map geographically to interface/cleft regions associated with martian crustal magnetization regions. By integrating electron and ion acceleration energy down to the upper atmosphere, we saw energy fluxes in the range of 1 to 50 milliwatts per square meter per second. These conditions are similar to those producing bright discrete auroras above Earth. Discrete auroras at Mars are therefore expected to be associated with plasma acceleration in diverging magnetic flux tubes above crustal magnetization regions, the auroras being distributed geographically in a complex pattern by the many multipole magnetic field lines extending into space.

Entities:  

Year:  2006        PMID: 16484488     DOI: 10.1126/science.1122071

Source DB:  PubMed          Journal:  Science        ISSN: 0036-8075            Impact factor:   47.728


  1 in total

1.  Machine-learning ready data on the thermal power consumption of the Mars Express Spacecraft.

Authors:  Matej Petković; Luke Lucas; Jurica Levatić; Martin Breskvar; Tomaž Stepišnik; Ana Kostovska; Panče Panov; Aljaž Osojnik; Redouane Boumghar; José A Martínez-Heras; James Godfrey; Alessandro Donati; Sašo Džeroski; Nikola Simidjievski; Bernard Ženko; Dragi Kocev
Journal:  Sci Data       Date:  2022-05-24       Impact factor: 8.501

  1 in total

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