Cristin-resultat-ID: 156726
Sist endret: 20. januar 2015, 14:03
Resultat
Vitenskapelig foredrag
2002

Anomalous ion line spectra associated with enhanced plasma lines observed during auroral precipitation

Bidragsytere:
  • Brett Cameron Isham
  • Cesar La Hoz
  • Michael T Rietveld
  • Tom Grydeland og
  • Francois Forme

Presentasjon

Navn på arrangementet: National Radio Science Meeting
Sted: Boulder, Colorado
Dato fra: 9. januar 2002
Dato til: 12. januar 2002

Arrangør:

Arrangørnavn: University of Colorado at Boulder

Om resultatet

Vitenskapelig foredrag
Publiseringsår: 2002

Beskrivelse Beskrivelse

Tittel

Anomalous ion line spectra associated with enhanced plasma lines observed during auroral precipitation

Sammendrag

Anomalous incoherent scatter echoes are radar echoes from the F or upper E regions whose ion line spectral shape departs from that corresponding to thermal equilibrium. The scattered power is enhanced and the spectra can be symmetric or asymmetric with one or the other shoulder more enhanced. Several theories have been proposed which can be divided into two classes: (1) direct electron or ion beam instabilities that distort and enhance the ion line and (2) a beam-enhanced Langmuir wave which becomes the pump for a parametric decay into enhanced daughter Langmuir and ion acoustic waves; the beam-enhanced pump and the enhanced daughter waves may be observed as non-thermally enhanced incoherent scatter ion and plasma lines. Direct beam instabilities fail to explain one or another characteristic of the observations, for example they may require large currents or enhance only one ion line shoulder, contrary to observations showing enhancements of either or both shoulders, or both with a central peak. On the other hand, parametric instability mechanisms appear better positioned to explain most if not all of the observations. Since they also produce enhancements of the plasma lines, a decisive test is whether the anomalous ion line echoes are accompanied by enhanced plasma lines. Parametric instabilities, or Langmuir turbulence, can also explain the enhanced central ion line peak. Here we present recent measurements made with the EISCAT VHF (224 MHz) radar in northern Scandinavia of anomalous ion line spectra accompanied by strong plasma line enhancements. These measurements provide important evidence in support of the parametric decay instability, or, more generally, of natural Langmuir turbulence in the aurora.

Bidragsytere

Brett Cameron Isham

  • Tilknyttet:
    Forfatter
    ved EISCAT ved UiT Norges arktiske universitet

Cesar Augusto Vergara La Hoz

Bidragsyterens navn vises på dette resultatet som Cesar La Hoz
  • Tilknyttet:
    Forfatter
    ved Institutt for fysikk og teknologi ved UiT Norges arktiske universitet

Michael T. Rietveld

Bidragsyterens navn vises på dette resultatet som Michael T Rietveld
  • Tilknyttet:
    Forfatter
    ved EISCAT ved UiT Norges arktiske universitet

Tom Grydeland

  • Tilknyttet:
    Forfatter
    ved Institutt for fysikk og teknologi ved UiT Norges arktiske universitet

Francois Forme

  • Tilknyttet:
    Forfatter
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