WFRF:(Alm J.)
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| Fältnamn | Indikatorer | Metadata |
|---|---|---|
| 000 | 06222naa a2200709 4500 | |
| 001 | oai:DiVA.org:kth-219466 | |
| 003 | SwePub | |
| 008 | 171206s2017 | |||||||||||000 ||eng| | |
| 009 | oai:DiVA.org:uu-342095 | |
| 024 | 7 | a https://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-2194662 URI |
| 024 | 7 | a https://doi.org/10.1002/2017JA0245632 DOI |
| 024 | 7 | a https://urn.kb.se/resolve?urn=urn:nbn:se:uu:diva-3420952 URI |
| 040 | a (SwePub)kthd (SwePub)uu | |
| 041 | a engb eng | |
| 042 | 9 SwePub | |
| 072 | 7 | a ref2 swepub-contenttype |
| 072 | 7 | a art2 swepub-publicationtype |
| 100 | 1 | a Farrugia, C. J.u Univ New Hampshire, Ctr Space Sci, Durham, NH 03824 USA.4 aut |
| 245 | 1 0 | a MMS Observations of Reconnection at Dayside Magnetopause Crossings During Transitions of the Solar Wind to Sub-Alfvénic Flow |
| 264 | 1 | b Blackwell Publishing Ltd,c 2017 |
| 338 | a print2 rdacarrier | |
| 500 | a QC 20190918 | |
| 520 | a We present MMS observations during two dayside magnetopause crossings under hitherto unexamined conditions: (i) when the bow shock is weakening and the solar wind transitioning to sub-Alfvénic flow and (ii) when it is reforming. Interplanetary conditions consist of a magnetic cloud with (i) a strong B (∼20 nT) pointing south and (ii) a density profile with episodic decreases to values of ∼0.3 cm−3 followed by moderate recovery. During the crossings the magnetosheath magnetic field is stronger than the magnetosphere field by a factor of ∼2.2. As a result, during the outbound crossing through the ion diffusion region, MMS observed an inversion of the relative positions of the X and stagnation (S) lines from that typically the case: the S line was closer to the magnetosheath side. The S line appears in the form of a slow expansion fan near which most of the energy dissipation is taking place. While in the magnetosphere between the crossings, MMS observed strong field and flow perturbations, which we argue to be due to kinetic Alfvén waves. During the reconnection interval, whistler mode waves generated by an electron temperature anisotropy (Te⊥>Te∥) were observed. Another aim of the paper is to distinguish bow shock-induced field and flow perturbations from reconnection-related signatures. The high-resolution MMS data together with 2-D hybrid simulations of bow shock dynamics helped us to distinguish between the two sources. We show examples of bow shock-related effects (such as heating) and reconnection effects such as accelerated flows satisfying the Walén relation. | |
| 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 |
| 650 | 7 | a NATURVETENSKAPx Geovetenskap och miljövetenskapx Geofysik0 (SwePub)105052 hsv//swe |
| 650 | 7 | a NATURAL SCIENCESx Earth and Related Environmental Sciencesx Geophysics0 (SwePub)105052 hsv//eng |
| 650 | 7 | a NATURVETENSKAPx Fysikx Astronomi, astrofysik och kosmologi0 (SwePub)103052 hsv//swe |
| 650 | 7 | a NATURAL SCIENCESx Physical Sciencesx Astronomy, Astrophysics and Cosmology0 (SwePub)103052 hsv//eng |
| 653 | a magnetic reconnection under extreme conditions | |
| 700 | 1 | a Lugaz, N.u Univ New Hampshire, Ctr Space Sci, Durham, NH 03824 USA.4 aut |
| 700 | 1 | a Alm, L.u Uppsala universitet,Institutet för rymdfysik, Uppsalaavdelningen4 aut |
| 700 | 1 | a Vasquez, B.u Univ New Hampshire, Ctr Space Sci, Durham, NH 03824 USA.4 aut |
| 700 | 1 | a Argall, M. R.u Univ New Hampshire, Ctr Space Sci, Durham, NH 03824 USA.4 aut |
| 700 | 1 | a Kucharek, H.u Univ New Hampshire, Ctr Space Sci, Durham, NH 03824 USA.4 aut |
| 700 | 1 | a Matsui, H.u Univ New Hampshire, Ctr Space Sci, Durham, NH 03824 USA.4 aut |
| 700 | 1 | a Torbert, R. B.u Univ New Hampshire, Ctr Space Sci, Durham, NH 03824 USA.4 aut |
| 700 | 1 | a Lavraud, B.u Univ Toulouse, Inst Rech Astrophys, Toulouse, France.,Southwest Res Inst, San Antonio, TX USA.,NASA, Goddard Space Flight Ctr, Greenbelt, MD USA.4 aut |
| 700 | 1 | a Le Contel, O.u UPMC Univ Paris 06, Univ Paris Sud, Lab Phys Plasmas, UMR7648,CNRS,Ecole Polytech,Observ Paris, Paris, France.4 aut |
| 700 | 1 | a Cohen, I. J.u Johns Hopkins Univ, Appl Phys Lab, Laurel, MD USA.4 aut |
| 700 | 1 | a Burch, J. L.4 aut |
| 700 | 1 | a Russell, C. T.u Univ Calif Los Angeles, Los Angeles, CA USA.4 aut |
| 700 | 1 | a Strangeway, R. J.u Univ Calif Los Angeles, Los Angeles, CA USA.4 aut |
| 700 | 1 | a Shuster, J.u NASA, Goddard Space Flight Ctr, Greenbelt, MD USA.4 aut |
| 700 | 1 | a Dorelli, J. C.u NASA, Goddard Space Flight Ctr, Greenbelt, MD USA.4 aut |
| 700 | 1 | a Eastwood, J. P.u Imperial Coll London, Blackett Lab, London, England.4 aut |
| 700 | 1 | a Ergun, R. E.u Univ Colorado Boulder, Lab Atmospher & Space Phys, Boulder, CO USA.4 aut |
| 700 | 1 | a Fuselier, S. A.u Southwest Res Inst, San Antonio, TX USA.;Univ Texas San Antonio, Dept Phys, San Antonio, TX USA.4 aut |
| 700 | 1 | a Gershman, D. J.u NASA, Goddard Space Flight Ctr, Greenbelt, MD USA.4 aut |
| 700 | 1 | a Giles, B. L.4 aut |
| 700 | 1 | a Khotyaintsev, Yuri V.u Uppsala universitet,Institutet för rymdfysik, Uppsalaavdelningen4 aut0 (Swepub:uu)ykh28990 |
| 700 | 1 | a Lindqvist, Per-Arne4 aut |
| 700 | 1 | a Marklund, Göranu Uppsala universitet,Institutet för rymdfysik, Uppsalaavdelningen4 aut0 (Swepub:kth)u1yq52h6 |
| 700 | 1 | a Paulson, K. W.u Univ New Hampshire, Ctr Space Sci, Durham, NH 03824 USA.4 aut |
| 700 | 1 | a Petrinec, S. M.u Lockheed Martin Adv Technol Ctr, Palo Alto, CA USA.4 aut |
| 700 | 1 | a Phan, T. D.u Space Sci Lab, Berkeley, CA USA.4 aut |
| 700 | 1 | a Pollock, C. J.u NASA, Goddard Space Flight Ctr, Greenbelt, MD USA.4 aut |
| 710 | 2 | a Univ New Hampshire, Ctr Space Sci, Durham, NH 03824 USA.b Institutet för rymdfysik, Uppsalaavdelningen4 org |
| 773 | 0 | t Journal of Geophysical Research - Space Physicsd : Blackwell Publishing Ltdg 122:10, s. 9934-9951q 122:10<9934-9951x 2169-9380x 2169-9402 |
| 856 | 4 8 | u https://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-219466 |
| 856 | 4 8 | u https://doi.org/10.1002/2017JA024563 |
| 856 | 4 8 | u https://urn.kb.se/resolve?urn=urn:nbn:se:uu:diva-342095 |
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