Improvement of the MSIS 86 and DTM thermospheric models by investigating the geomagnetic effect

I. Almár, E. Illés-Almár, A. Horváth, Z. Kolláth, D. V. Bisikalo, T. V. Kasimenko

Research output: Contribution to journalArticle

9 Citations (Scopus)

Abstract

Based on measurements of the CACTUS accelerometer it has been found that during the recovery phase of geomagnetic disturbances the models are unable to describe properly the total density changes in the equatorial thermosphere. Introducing the geomagnetic activity index Dst instead of Kp as a model input parameter gives a much better description of the measurements. The residuals show a diurnal dependence, hinting partly at model errors in the diurnal effect (though MSIS 86 is much better than DTM in this respect), partly at a diurnal term in the geomagnetic effect.

Original languageEnglish
Pages (from-to)313-316
Number of pages4
JournalAdvances in Space Research
Volume12
Issue number6
DOIs
Publication statusPublished - 1992

    Fingerprint

ASJC Scopus subject areas

  • Aerospace Engineering
  • Astronomy and Astrophysics
  • Geophysics
  • Atmospheric Science
  • Space and Planetary Science
  • Earth and Planetary Sciences(all)

Cite this