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On the magnetic characteristics of magnetic holes in the solar wind between Mercury and Venus
Austrian Acad Sci, Space Res Inst, Graz, Austria..ORCID iD: 0000-0002-4455-3403
Tech Univ Carolo Wilhelmina Braunschweig, Inst Geophys & Extraterr Phys, Braunschweig, Germany.;European Space Agcy, Estec, Keplerlaan 1, NL-2201 AZ Noordwijk, Netherlands..
Austrian Acad Sci, Space Res Inst, Graz, Austria..
KTH, School of Electrical Engineering and Computer Science (EECS), Electrical Engineering, Space and Plasma Physics.ORCID iD: 0000-0003-1270-1616
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2020 (English)In: Annales Geophysicae, ISSN 0992-7689, E-ISSN 1432-0576, Vol. 38, no 1, p. 51-60Article in journal (Refereed) Published
Abstract [en]

The occurrence rate of linear and pseudo magnetic holes has been determined during MESSENGER's cruise phase starting from Venus (2007) and arriving at Mercury (2011). It is shown that the occurrence rate of linear magnetic holes, defined as a maximum of 10 degrees rotation of the magnetic field over the hole, slowly decreases from Mercury to Venus. The pseudo magnetic holes, defined as a rotation between 10 and 45 degrees over the hole, have mostly a constant occurrence rate.

Place, publisher, year, edition, pages
COPERNICUS GESELLSCHAFT MBH , 2020. Vol. 38, no 1, p. 51-60
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Physical Sciences
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URN: urn:nbn:se:kth:diva-267157DOI: 10.5194/angeo-38-51-2020ISI: 000507331400001Scopus ID: 2-s2.0-85078300551OAI: oai:DiVA.org:kth-267157DiVA, id: diva2:1393497
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QC 20200217

Available from: 2020-02-17 Created: 2020-02-17 Last updated: 2020-02-17Bibliographically approved

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Karlsson, Tomas

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