Search: WFRF:(Louarn P.) > Alfven :
Fältnamn | Indikatorer | Metadata |
---|---|---|
000 | 05971naa a2201213 4500 | |
001 | oai:DiVA.org:umu-56167 | |
003 | SwePub | |
008 | 120612s2012 | |||||||||||000 ||eng| | |
009 | oai:DiVA.org:kth-96448 | |
009 | oai:DiVA.org:uu-175213 | |
024 | 7 | a https://urn.kb.se/resolve?urn=urn:nbn:se:umu:diva-561672 URI |
024 | 7 | a https://doi.org/10.1007/s10686-011-9273-y2 DOI |
024 | 7 | a https://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-964482 URI |
024 | 7 | a 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 | 7 | a ref2 swepub-contenttype |
072 | 7 | a art2 swepub-publicationtype |
100 | 1 | a Berthomier, M.4 aut |
245 | 1 0 | a Alfven :b magnetosphere-ionosphere connection explorers |
264 | c 2011-12-27 | |
264 | 1 | a 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 | 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 |
650 | 7 | a NATURVETENSKAPx Fysik0 (SwePub)1032 hsv//swe |
650 | 7 | a NATURAL SCIENCESx Physical Sciences0 (SwePub)1032 hsv//eng |
653 | a Alfven | |
653 | a Cosmic vision | |
653 | a Auroral acceleration region | |
653 | a Space plasmas | |
700 | 1 | a Fazakerley, A. N.4 aut |
700 | 1 | a Forsyth, C.4 aut |
700 | 1 | a Pottelette, R.4 aut |
700 | 1 | a Alexandrova, O.4 aut |
700 | 1 | a Anastasiadis, A.4 aut |
700 | 1 | a Aruliah, A.4 aut |
700 | 1 | a Blelly, P. -L4 aut |
700 | 1 | a Briand, C.4 aut |
700 | 1 | a Bruno, R.4 aut |
700 | 1 | a Canu, P.4 aut |
700 | 1 | a Cecconi, B.4 aut |
700 | 1 | a Chust, T.4 aut |
700 | 1 | a Daglis, I.4 aut |
700 | 1 | a Davies, J.4 aut |
700 | 1 | a Dunlop, M.4 aut |
700 | 1 | a Fontaine, D.4 aut |
700 | 1 | a Genot, V.4 aut |
700 | 1 | a Gustavsson, B.4 aut |
700 | 1 | a Haerendel, G.4 aut |
700 | 1 | a Hamrin, Mariau Umeå universitet,Institutionen för fysik4 aut0 (Swepub:umu)maha0006 |
700 | 1 | a Hapgood, M.4 aut |
700 | 1 | a Hess, S.4 aut |
700 | 1 | a Kataria, D.4 aut |
700 | 1 | a Kauristie, K.4 aut |
700 | 1 | a Kemble, S.4 aut |
700 | 1 | a Khotyaintsev, Yuriu Uppsala universitet,Institutet för rymdfysik, Uppsalaavdelningen4 aut0 (Swepub:uu)ykh28990 |
700 | 1 | a Koskinen, H.4 aut |
700 | 1 | a Lamy, L.4 aut |
700 | 1 | a Lanchester, B.4 aut |
700 | 1 | a Louarn, P.4 aut |
700 | 1 | a Lucek, E.4 aut |
700 | 1 | a Lundin, R.4 aut |
700 | 1 | a Maksimovic, M.4 aut |
700 | 1 | a Manninen, J.4 aut |
700 | 1 | a Marchaudon, A.4 aut |
700 | 1 | a Marghitu, O.4 aut |
700 | 1 | a Marklund, Göran T.u KTH,Alfvénlaboratoriet,Rymd- och plasmafysik4 aut0 (Swepub:kth)u1yq52h6 |
700 | 1 | a Milan, S.4 aut |
700 | 1 | a Moen, J.4 aut |
700 | 1 | a Mottez, F.4 aut |
700 | 1 | a Nilsson, H.4 aut |
700 | 1 | a Ostgaard, N.4 aut |
700 | 1 | a Owen, C. J.4 aut |
700 | 1 | a Parrot, M.4 aut |
700 | 1 | a Pedersen, A.4 aut |
700 | 1 | a Perry, C.4 aut |
700 | 1 | a Pincon, J. -L4 aut |
700 | 1 | a Pitout, F.4 aut |
700 | 1 | a Pulkkinen, T.4 aut |
700 | 1 | a Rae, I. J.4 aut |
700 | 1 | a Rezeau, L.4 aut |
700 | 1 | a Roux, A.4 aut |
700 | 1 | a Sandahl, I.4 aut |
700 | 1 | a Sandberg, I.4 aut |
700 | 1 | a Turunen, E.4 aut |
700 | 1 | a Vogt, J.4 aut |
700 | 1 | a Walsh, A.4 aut |
700 | 1 | a Watt, C. E. J.4 aut |
700 | 1 | a Wild, J. A.4 aut |
700 | 1 | a Yamauchi, M.4 aut |
700 | 1 | a Zarka, P.4 aut |
700 | 1 | a Zouganelis, I.4 aut |
710 | 2 | a Umeå universitetb Institutionen för fysik4 org |
773 | 0 | t Experimental astronomyd Dordrecht : Springerg 33:2-3, s. 445-489q 33:2-3<445-489x 0922-6435x 1572-9508 |
856 | 4 | u https://eprints.lancs.ac.uk/id/eprint/54376/1/Alfven_ExpAst_resubmission_forprint.pdf |
856 | 4 8 | u https://urn.kb.se/resolve?urn=urn:nbn:se:umu:diva-56167 |
856 | 4 8 | u https://doi.org/10.1007/s10686-011-9273-y |
856 | 4 8 | u https://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-96448 |
856 | 4 8 | u https://urn.kb.se/resolve?urn=urn:nbn:se:uu:diva-175213 |
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