onr:"swepub:oai:DiVA.org:kth-18097"
Sökning: onr:"swepub:oai:DiVA.org:kth-18097" > Plasma transport al...
- 1 av 1
- Föregående post
- Nästa post
- Till träfflistan
| Fältnamn | Indikatorer | Metadata |
|---|---|---|
| 000 | 04298naa a2200661 4500 | |
| 001 | oai:DiVA.org:kth-18097 | |
| 003 | SwePub | |
| 008 | 100805s2008 | |||||||||||000 ||eng| | |
| 009 | oai:DiVA.org:uu-149290 | |
| 024 | 7 | a https://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-180972 URI |
| 024 | 7 | a https://doi.org/10.5194/angeo-26-3279-20082 DOI |
| 024 | 7 | a https://urn.kb.se/resolve?urn=urn:nbn:se:uu:diva-1492902 URI |
| 040 | a (SwePub)kthd (SwePub)uu | |
| 041 | a engb engb -1 | |
| 042 | 9 SwePub | |
| 072 | 7 | a ref2 swepub-contenttype |
| 072 | 7 | a art2 swepub-publicationtype |
| 100 | 1 | a Kullen, A.u Uppsala universitet,Institutet för rymdfysik, Uppsalaavdelningen4 aut0 (Swepub:uu)ankul516 |
| 245 | 1 0 | a Plasma transport along discrete auroral arcs and its contribution to the ionospheric plasma convection |
| 264 | c 2008-10-21 | |
| 264 | 1 | b Copernicus GmbH,c 2008 |
| 338 | a print2 rdacarrier | |
| 500 | a QC 20100525 | |
| 520 | a The role of intense high-altitude electric field (E-field) peaks for large-scale plasma convection is investigated with the help of Cluster E-field, B-field and density data. The study covers 32 E-field events between 4 and 7 R-E geocentric distance, with E-field magnitudes in the range 500 1000 mV/m when mapped to ionospheric altitude. We focus on E-field structures above the ionosphere that are typically coupled to discrete auroral arcs and their return current region. Connected to such E-field peaks are rapid plasma flows directed along the discrete arcs in opposite directions on each side of the arc. Nearly all the E-field events occur during active times. A strong dependence on different substorm phases is found: a majority of intense E-field events appearing during substorm expansion or maximum phase are located on the night-side oval, while most recovery events occur on the dusk-to-dayside part of the oval. For most expansion and maximum phase cases, the average background plasma flow is in the sunward direction. For a majority of recovery events, the flow is in the anti-sunward direction. The net plasma flux connected to a strong E-field peak is in two thirds of the cases in the same direction as the background plasma flow. However, in only one third of the cases the strong flux caused by an E-field peak makes an important contribution to the plasma transport within the boundary plasma sheet. For a majority of events, the area covered by rapid plasma flows above discrete arcs is too small to have an effect on the global convection. This questions the role of discrete auroral arcs as major driver of plasma convection. | |
| 520 | a | |
| 650 | 7 | a NATURVETENSKAPx Fysik0 (SwePub)1032 hsv//swe |
| 650 | 7 | a NATURAL SCIENCESx Physical Sciences0 (SwePub)1032 hsv//eng |
| 653 | a Ionosphere | |
| 653 | a Auroral ionosphere | |
| 653 | a Electric fields and currents | |
| 653 | a Planetary | |
| 653 | a ionospheres | |
| 653 | a interplanetary magnetic field | |
| 653 | a latitude boundary-layer | |
| 653 | a electric-fields | |
| 653 | a low-altitude | |
| 653 | a particle-acceleration | |
| 653 | a reversal | |
| 653 | a boundaries | |
| 653 | a cluster | |
| 653 | a precipitation | |
| 653 | a magnetosphere | |
| 653 | a sheet | |
| 653 | a Physics | |
| 700 | 1 | a Buchert, Stephanu Uppsala universitet,Institutet för rymdfysik, Uppsalaavdelningen4 aut0 (Swepub:uu)stbuc254 |
| 700 | 1 | a Karlsson, Tomasu KTH,Rymd- och plasmafysik4 aut0 (Swepub:kth)u154ti5p |
| 700 | 1 | a Johansson, T.4 aut |
| 700 | 1 | a Lileo, S.4 aut |
| 700 | 1 | a Eriksson, Andersu Uppsala universitet,KTH,Strukturmekanik,Institutet för rymdfysik, Uppsalaavdelningen4 aut0 (Swepub:uu)andeerik |
| 700 | 1 | a Nilsson, H.4 aut |
| 700 | 1 | a Marchaudon, A.4 aut |
| 700 | 1 | a Fazakerley, A. N.4 aut |
| 710 | 2 | a Uppsala universitetb Institutet för rymdfysik, Uppsalaavdelningen4 org |
| 773 | 0 | t Annales Geophysicaed : Copernicus GmbHg 26:11, s. 3279-3293q 26:11<3279-3293x 0992-7689x 1432-0576 |
| 856 | 4 | u https://www.ann-geophys.net/26/3279/2008/angeo-26-3279-2008.pdf |
| 856 | 4 8 | u https://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-18097 |
| 856 | 4 8 | u https://doi.org/10.5194/angeo-26-3279-2008 |
| 856 | 4 8 | u https://urn.kb.se/resolve?urn=urn:nbn:se:uu:diva-149290 |
- 1 av 1
- Föregående post
- Nästa post
- Till träfflistan
Hitta mer i SwePub
- Av författaren/redakt...
- Kullen, A.
- Buchert, Stephan
- Karlsson, Tomas
- Johansson, T.
- Lileo, S.
- Eriksson, Anders
- visa fler...
- Nilsson, H.
- Marchaudon, A.
- Fazakerley, A. N ...
- visa färre...
- Om ämnet
-
- NATURVETENSKAP
- NATURVETENSKAP
- och Fysik
- Artiklar i publikationen
- Annales Geophysi ...
- Av lärosätet
- Kungliga Tekniska Högskolan
- Uppsala universitet
Sök utanför SwePub
- Sök vidare i:
- Google Book Search
- Google Scholar
Kungliga biblioteket hanterar dina personuppgifter i enlighet med EU:s dataskyddsförordning (2018), GDPR. Läs mer om hur det funkar här.
Så här hanterar KB dina uppgifter vid användning av denna tjänst.
- Copyright © LIBRIS - Nationella bibliotekssystem
- LIBRIS.kb.se
