SwePub
Sök i LIBRIS databas

  Extended search

onr:"swepub:oai:DiVA.org:uu-279651"
 

Search: onr:"swepub:oai:DiVA.org:uu-279651" > Estimation of cold ...

  • 1 of 1
  • Previous record
  • Next record
  •    To hitlist
  • Haaland, S.Univ Bergen, Birkeland Ctr Space Sci, Bergen, Norway.;Max Planck Inst Solar Syst Res, Gottingen, Germany. (author)

Estimation of cold plasma outflow during geomagnetic storms

  • Article/chapterEnglish2015

Publisher, publication year, extent ...

  • 2015
  • electronicrdacarrier

Numbers

  • LIBRIS-ID:oai:DiVA.org:uu-279651
  • https://urn.kb.se/resolve?urn=urn:nbn:se:uu:diva-279651URI
  • https://doi.org/10.1002/2015JA021810DOI

Supplementary language notes

  • Language:English
  • Summary in:English

Part of subdatabase

Classification

  • Subject category:ref swepub-contenttype
  • Subject category:art swepub-publicationtype

Notes

  • Low-energy ions of ionospheric origin constitute a significant contributor to the magnetospheric plasma population. Measuring cold ions is difficult though. Observations have to be done at sufficiently high altitudes and typically in regions of space where spacecraft attain a positive charge due to solar illumination. Cold ions are therefore shielded from the satellite particle detectors. Furthermore, spacecraft can only cover key regions of ion outflow during segments of their orbit, so additional complications arise if continuous longtime observations, such as during a geomagnetic storm, are needed. In this paper we suggest a new approach, based on a combination of synoptic observations and a novel technique to estimate the flux and total outflow during the various phases of geomagnetic storms. Our results indicate large variations in both outflow rates and transport throughout the storm. Prior to the storm main phase, outflow rates are moderate, and the cold ions are mainly emanating from moderately sized polar cap regions. Throughout the main phase of the storm, outflow rates increase and the polar cap source regions expand. Furthermore, faster transport, resulting from enhanced convection, leads to a much larger supply of cold ions to the near-Earth region during geomagnetic storms.

Subject headings and genre

Added entries (persons, corporate bodies, meetings, titles ...)

  • Eriksson, AndersUppsala universitet,Institutet för rymdfysik, Uppsalaavdelningen(Swepub:uu)andeerik (author)
  • André, MatsUppsala universitet,Institutet för rymdfysik, Uppsalaavdelningen(Swepub:uu)maand125 (author)
  • Maes, L.Belgian Inst Aeron, Brussels, Belgium. (author)
  • Baddeley, L.Univ Ctr Svalbard, Dept Arctic Geophys, Longyearbyen, Norway. (author)
  • Barakat, A.Utah State Univ, Ctr Atmospher & Space Sci, Logan, UT 84322 USA. (author)
  • Chappell, R.Vanderbilt Univ, Sci & Res Commun, Nashville, TN 37235 USA. (author)
  • Eccles, V.Utah State Univ, Ctr Atmospher & Space Sci, Logan, UT 84322 USA. (author)
  • Johnsen, C.Univ Oslo, Dept Geophys, Oslo, Norway. (author)
  • Lybekk, B.Univ Oslo, Dept Phys, Oslo, Norway. (author)
  • Li, K.Max Planck Inst Solar Syst Res, Gottingen, Germany. (author)
  • Pedersen, A.Univ Oslo, Dept Phys, Oslo, Norway. (author)
  • Schunk, R.Utah State Univ, Ctr Atmospher & Space Sci, Logan, UT 84322 USA. (author)
  • Welling, D.Univ Bergen, Birkeland Ctr Space Sci, Bergen, Norway.;Univ Michigan, Dept Atmospher Ocean & Space Sci, Ann Arbor, MI 48109 USA. (author)
  • Univ Bergen, Birkeland Ctr Space Sci, Bergen, Norway.;Max Planck Inst Solar Syst Res, Gottingen, Germany.Institutet för rymdfysik, Uppsalaavdelningen (creator_code:org_t)

Related titles

  • In:Journal of Geophysical Research - Space Physics120:12, s. 10622-106392169-93802169-9402

Internet link

Find in a library

To the university's database

  • 1 of 1
  • Previous record
  • Next record
  •    To hitlist

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.

 
pil uppåt Close

Copy and save the link in order to return to this view