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titleA PIC Simulation for Break-up of the Closed magnetic field of the Pulsar Magnetosphere
Author(jpn)海崎, 光宏; 柴田, 晋平; 結城, 伸哉
Author(eng)Umizaki, Mitsuhiro; Shibata, Shinpei; Yuki, Shinya
Author Affiliation(jpn)山形大学大学院理工学研究科; 山形大学理学部; 山形大学大学院理工学研究科
Author Affiliation(eng)School of Science and Engineering, Yamagata University; Department of Physics, Yamagata University; School of Science and Engineering, Yamagata University
Issue Date2010-02-26
Publisher宇宙航空研究開発機構
Japan Aerospace Exploration Agency (JAXA)
Publication title宇宙航空研究開発機構特別資料:
JAXA Special Publication: The Energetic Cosmos; from Suzaku to ASTRO-H
VolumeJAXA-SP-09-008E
Start page230
End page231
Publication date2010-02-26
Languageeng
AbstractWe investigate the magnetic dissipation in the pulsar magnetosphere, in particular, around the Y-point, which is the boundary region between the closed magnetic flux of the dead zone and the open flux in the wind zone, via axisymmetric particle-in-cell (PIC) method in the cylindrical coordinates. We find that magnetic reconnections occur around the Y-point and magnetic islands are repeatedly formed and ejected outward, which suggests that the magnetic energy converts to the kinetic and thermal energy. It is possible that high-energy emission is radiated from this region. It is also possible that the plasma pressure accelerates the pulsar wind. A polar cap radiation may be emitted by falling particles into the neutron star.
DescriptionMeeting Information: The 3rd Suzaku international Conference "Energetic Cosmos : from Suzaku to ASTRO-H" (June 29-July 2, 2009. Grand Park Otaru Hotel), Otaru, Hokkaido Japan
Meeting sponsors: The University of Tokyo, The Institute of Physical and Chemical Research, The Japan Society for the Promotion of Science
Keywordsmagnetic fields - MHD - pulsars: general - stars: neutron
Document TypeConference Paper
JAXA Category特別資料
ISSN1349-113X
NCIDAA11984031
SHI-NOAA0064574087
Report NoJAXA-SP-09-008E
URIhttps://repository.exst.jaxa.jp/dspace/handle/a-is/19008


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