Journal cover Journal topic
Annales Geophysicae An interactive open-access journal of the European Geosciences Union
Journal topic

Journal metrics

Journal metrics

  • IF value: 1.585 IF 1.585
  • IF 5-year value: 1.698 IF 5-year
    1.698
  • CiteScore value: 1.62 CiteScore
    1.62
  • SNIP value: 0.820 SNIP 0.820
  • IPP value: 1.52 IPP 1.52
  • SJR value: 0.781 SJR 0.781
  • Scimago H <br class='hide-on-tablet hide-on-mobile'>index value: 83 Scimago H
    index 83
  • h5-index value: 24 h5-index 24
Volume 17, issue 5
Ann. Geophys., 17, 623–630, 1999
https://doi.org/10.1007/s00585-999-0623-2
© European Geosciences Union 1999

Special issue: Solar System Plasmas

Ann. Geophys., 17, 623–630, 1999
https://doi.org/10.1007/s00585-999-0623-2
© European Geosciences Union 1999

  31 May 1999

31 May 1999

Stability of stationary and time-varying nongyrotropic particle distributions

A. L. Brinca A. L. Brinca
  • Centro de F. de Plasmas, Instituto Superior Técnico, P-1096 Lisboa Codex, Portugal
  • Correspondence to: ebrinca@beta.ist.utl.pt

Abstract. The ubiquity of nongyrotropic particle populations in space plasmas warrants the study of their characteristics, in particular their stability. The unperturbed nongyrotropic distribution functions in homogeneous media without sources and sinks (closed phase space) must be rotating and time-varying (TNG), whereas consideration of open phase spaces allows for the occurrence of homogeneous and stationary distributions (SNG). The free energy brought about by the introduction of gyrophase organization in a particle population can destabilize otherwise thoroughly stable magnetoplasmas (or, a fortiori, enhance pre-existing gyrotropic instabilities) and feed intense wave growth both in TNG and SNG environments: The nongyrotropic (electron or ion) species can originate unstable coupling among the gyrotropic characteristic waves. The stability properties of these two types of homogeneous nongyrotropy shall be contrasted for parallel (with respect to the ambient magnetic field) and perpendicular propagation, and their potential role as wave activity sources shall be illustrated resorting to solutions of the appropriate dispersion equations and numerical simulations.

Key words. Space plasma physics (waves and instabilities) · Magnetospheric physics (plasma waves and instabilities) · Interplanetary physics (plasma waves and turbulence)

Publications Copernicus
Special issue
Download
Citation