Sökning: WFRF:(Bale S D) > Electrostatic Turbu...
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000 | 03464naa a2200445 4500 | |
001 | oai:DiVA.org:kth-271752 | |
003 | SwePub | |
008 | 200408s2020 | |||||||||||000 ||eng| | |
024 | 7 | a https://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-2717522 URI |
024 | 7 | a https://doi.org/10.3847/2041-8213/ab65822 DOI |
040 | a (SwePub)kth | |
041 | a engb eng | |
042 | 9 SwePub | |
072 | 7 | a ref2 swepub-contenttype |
072 | 7 | a art2 swepub-publicationtype |
100 | 1 | a Wang, R.u Univ Calif Berkeley, Space Sci Lab, Berkeley, CA 94720 USA.;Univ Calif Berkeley, Phys Dept, Berkeley, CA 94720 USA.4 aut |
245 | 1 0 | a Electrostatic Turbulence and Debye-scale Structures in Collisionless Shocks |
264 | c 2020-01-20 | |
264 | 1 | b IOP PUBLISHING LTD,c 2020 |
338 | a print2 rdacarrier | |
500 | a QC 20200408 | |
520 | a We present analysis of more than 100 large-amplitude bipolar electrostatic structures in a quasi-perpendicular supercritical Earth's bow shock crossing, measured by the Magnetospheric Multiscale spacecraft. The occurrence of the bipolar structures is shown to be tightly correlated with magnetic field gradients in the shock transition region. The bipolar structures have negative electrostatic potentials and spatial scales of a few Debye lengths. The bipolar structures propagate highly oblique to the shock normal with velocities (in the plasma rest frame) of the order of the ion-acoustic velocity. We argue that the bipolar structures are ion phase space holes produced by the two-stream instability between incoming and reflected ions. This is the first identification of the ion two-stream instability in collisionless shocks. | |
650 | 7 | a NATURVETENSKAPx Fysikx Fusion, plasma och rymdfysik0 (SwePub)103032 hsv//swe |
650 | 7 | a NATURAL SCIENCESx Physical Sciencesx Fusion, Plasma and Space Physics0 (SwePub)103032 hsv//eng |
653 | a Astrophysical processes | |
700 | 1 | a Vasko, I. Y.u Univ Calif Berkeley, Space Sci Lab, Berkeley, CA 94720 USA.4 aut |
700 | 1 | a Mozer, F. S.u Univ Calif Berkeley, Space Sci Lab, Berkeley, CA 94720 USA.4 aut |
700 | 1 | a Bale, S. D.u Univ Calif Berkeley, Space Sci Lab, Berkeley, CA 94720 USA.;Univ Calif Berkeley, Phys Dept, Berkeley, CA 94720 USA.4 aut |
700 | 1 | a Artemyev, A. V.u Russian Acad Sci, Space Res Inst, Moscow, Russia.;Univ Calif Los Angeles, Inst Geophys & Planetary Sci, Los Angeles, CA 90024 USA.4 aut |
700 | 1 | a Bonnell, J. W.u Univ Calif Berkeley, Space Sci Lab, Berkeley, CA 94720 USA.4 aut |
700 | 1 | a Ergun, R.u Univ Colorado, Boulder, CO 80309 USA.4 aut |
700 | 1 | a Giles, B.u NASA, Goddard Space Flight Ctr, Greenbelt, MD USA.4 aut |
700 | 1 | a Lindqvist, Per-Arneu KTH,Rymd- och plasmafysik4 aut0 (Swepub:kth)u1yukyk9 |
700 | 1 | a Russell, C. T.u Univ Calif Los Angeles, Inst Geophys & Planetary Sci, Los Angeles, CA 90024 USA.4 aut |
700 | 1 | a Strangeway, R.u Univ Calif Los Angeles, Inst Geophys & Planetary Sci, Los Angeles, CA 90024 USA.4 aut |
710 | 2 | a Univ Calif Berkeley, Space Sci Lab, Berkeley, CA 94720 USA.;Univ Calif Berkeley, Phys Dept, Berkeley, CA 94720 USA.b Univ Calif Berkeley, Space Sci Lab, Berkeley, CA 94720 USA.4 org |
773 | 0 | t Astrophysical Journal Lettersd : IOP PUBLISHING LTDg 889:1q 889:1x 2041-8205x 2041-8213 |
856 | 4 | u http://arxiv.org/pdf/1912.01770 |
856 | 4 8 | u https://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-271752 |
856 | 4 8 | u https://doi.org/10.3847/2041-8213/ab6582 |
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