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LIBRIS Formathandbok  (Information om MARC21)
FältnamnIndikatorerMetadata
00005971naa a2201213 4500
001oai:DiVA.org:umu-56167
003SwePub
008120612s2012 | |||||||||||000 ||eng|
009oai:DiVA.org:kth-96448
009oai:DiVA.org:uu-175213
024a https://urn.kb.se/resolve?urn=urn:nbn:se:umu:diva-561672 URI
024a https://doi.org/10.1007/s10686-011-9273-y2 DOI
024a https://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-964482 URI
024a https://urn.kb.se/resolve?urn=urn:nbn:se:uu:diva-1752132 URI
040 a (SwePub)umud (SwePub)kthd (SwePub)uu
041 a engb eng
042 9 SwePub
072 7a ref2 swepub-contenttype
072 7a art2 swepub-publicationtype
100a Berthomier, M.4 aut
2451 0a Alfven :b magnetosphere-ionosphere connection explorers
264 c 2011-12-27
264 1a Dordrecht :b Springer,c 2012
338 a print2 rdacarrier
500 a Special Issue: SI
500 a QC 20120604
520 a The aurorae are dynamic, luminous displays that grace the night skies of Earth's high latitude regions. The solar wind emanating from the Sun is their ultimate energy source, but the chain of plasma physical processes leading to auroral displays is complex. The special conditions at the interface between the solar wind-driven magnetosphere and the ionospheric environment at the top of Earth's atmosphere play a central role. In this Auroral Acceleration Region (AAR) persistent electric fields directed along the magnetic field accelerate magnetospheric electrons to the high energies needed to excite luminosity when they hit the atmosphere. The "ideal magnetohydrodynamics" description of space plasmas which is useful in much of the magnetosphere cannot be used to understand the AAR. The AAR has been studied by a small number of single spacecraft missions which revealed an environment rich in wave-particle interactions, plasma turbulence, and nonlinear acceleration processes, acting on a variety of spatio-temporal scales. The pioneering 4-spacecraft Cluster magnetospheric research mission is now fortuitously visiting the AAR, but its particle instruments are too slow to allow resolve many of the key plasma physics phenomena. The Alfv,n concept is designed specifically to take the next step in studying the aurora, by making the crucial high-time resolution, multi-scale measurements in the AAR, needed to address the key science questions of auroral plasma physics. The new knowledge that the mission will produce will find application in studies of the Sun, the processes that accelerate the solar wind and that produce aurora on other planets.
650 7a NATURVETENSKAPx Fysikx Astronomi, astrofysik och kosmologi0 (SwePub)103052 hsv//swe
650 7a NATURAL SCIENCESx Physical Sciencesx Astronomy, Astrophysics and Cosmology0 (SwePub)103052 hsv//eng
650 7a NATURVETENSKAPx Fysik0 (SwePub)1032 hsv//swe
650 7a NATURAL SCIENCESx Physical Sciences0 (SwePub)1032 hsv//eng
653 a Alfven
653 a Cosmic vision
653 a Auroral acceleration region
653 a Space plasmas
700a Fazakerley, A. N.4 aut
700a Forsyth, C.4 aut
700a Pottelette, R.4 aut
700a Alexandrova, O.4 aut
700a Anastasiadis, A.4 aut
700a Aruliah, A.4 aut
700a Blelly, P. -L4 aut
700a Briand, C.4 aut
700a Bruno, R.4 aut
700a Canu, P.4 aut
700a Cecconi, B.4 aut
700a Chust, T.4 aut
700a Daglis, I.4 aut
700a Davies, J.4 aut
700a Dunlop, M.4 aut
700a Fontaine, D.4 aut
700a Genot, V.4 aut
700a Gustavsson, B.4 aut
700a Haerendel, G.4 aut
700a Hamrin, Mariau Umeå universitet,Institutionen för fysik4 aut0 (Swepub:umu)maha0006
700a Hapgood, M.4 aut
700a Hess, S.4 aut
700a Kataria, D.4 aut
700a Kauristie, K.4 aut
700a Kemble, S.4 aut
700a Khotyaintsev, Yuriu Uppsala universitet,Institutet för rymdfysik, Uppsalaavdelningen4 aut0 (Swepub:uu)ykh28990
700a Koskinen, H.4 aut
700a Lamy, L.4 aut
700a Lanchester, B.4 aut
700a Louarn, P.4 aut
700a Lucek, E.4 aut
700a Lundin, R.4 aut
700a Maksimovic, M.4 aut
700a Manninen, J.4 aut
700a Marchaudon, A.4 aut
700a Marghitu, O.4 aut
700a Marklund, Göran T.u KTH,Alfvénlaboratoriet,Rymd- och plasmafysik4 aut0 (Swepub:kth)u1yq52h6
700a Milan, S.4 aut
700a Moen, J.4 aut
700a Mottez, F.4 aut
700a Nilsson, H.4 aut
700a Ostgaard, N.4 aut
700a Owen, C. J.4 aut
700a Parrot, M.4 aut
700a Pedersen, A.4 aut
700a Perry, C.4 aut
700a Pincon, J. -L4 aut
700a Pitout, F.4 aut
700a Pulkkinen, T.4 aut
700a Rae, I. J.4 aut
700a Rezeau, L.4 aut
700a Roux, A.4 aut
700a Sandahl, I.4 aut
700a Sandberg, I.4 aut
700a Turunen, E.4 aut
700a Vogt, J.4 aut
700a Walsh, A.4 aut
700a Watt, C. E. J.4 aut
700a Wild, J. A.4 aut
700a Yamauchi, M.4 aut
700a Zarka, P.4 aut
700a Zouganelis, I.4 aut
710a Umeå universitetb Institutionen för fysik4 org
773t Experimental astronomyd Dordrecht : Springerg 33:2-3, s. 445-489q 33:2-3<445-489x 0922-6435x 1572-9508
856u https://eprints.lancs.ac.uk/id/eprint/54376/1/Alfven_ExpAst_resubmission_forprint.pdf
8564 8u https://urn.kb.se/resolve?urn=urn:nbn:se:umu:diva-56167
8564 8u https://doi.org/10.1007/s10686-011-9273-y
8564 8u https://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-96448
8564 8u https://urn.kb.se/resolve?urn=urn:nbn:se:uu:diva-175213

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