Observations of the April 2002 geomagnetic storm by the global network of incoherent scatter radars

L. P. Goncharenko, J. E. Salah, A. Van Eyken, V. Howells, J. P. Thayer, V. I. Taran, B. Shpynev, Q. Zhou, J. Chau

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Abstract

This paper describes the ionospheric response to a geomagnetic storm beginning on 17 April 2002. We present the measurements of ionospheric parameters in the F-region obtained by the network of eight incoherent scatter radars. The main effects of this storm include a deep decrease in the electron density observed at high and middle latitudes in the pre-noon sector, and a minor enhancement in the density observed in the daytime sector at middle latitudes. Extreme plasma heating (> 1000-3000 K) is observed at high latitudes, subsiding to 200-300 K at subauroral latitudes. The western hemisphere radar chain observed the prompt penetration of the electric field from auroral to equatorial latitudes, as well as the daytime enhancement of plasma drift parallel to the magnetic field line, which is related to the enhancement in the equatorward winds. We suggest that in the first several hours after the storm onset, a negative phase above Millstone Hill (pre-noon sector) results from counter-acting processes - penetration electric field, meridional wind, and electrodynamic heating, with electrodynamic heating being the dominant mechanism. At the lower latitude in the pre-noon sector (Arecibo and Jicamarca), the penetration electric field becomes more important, leading to a negative storm phase over Arecibo. In contrast, in the afternoon sector at mid-latitudes (Kharkov, Irkutsk), effects of penetration electric field and meridional wind do not counteract, but add up, leading to a small (∼15%), positive storm phase over these locations. As the storm develops, Millstone Hill and Irkutsk mid-latitude radars observe further depletion of electron density due to the changes in the neutral composition.

Original languageEnglish
Pages (from-to)163-181
Number of pages19
JournalAnnales Geophysicae
Volume23
Issue number1
DOIs
Publication statusPublished - Jan 1 2005

Fingerprint

geomagnetic storm
magnetic storms
sectors
noon
penetration
electric field
electric fields
daytime
electrodynamics
polar regions
ionospherics
augmentation
heating
Western hemisphere
electron density
plasma drift
plasma heating
F region
tropical regions
plasma

All Science Journal Classification (ASJC) codes

  • Astronomy and Astrophysics
  • Geology
  • Atmospheric Science
  • Earth and Planetary Sciences (miscellaneous)
  • Space and Planetary Science

Cite this

Goncharenko, L. P., Salah, J. E., Van Eyken, A., Howells, V., Thayer, J. P., Taran, V. I., ... Chau, J. (2005). Observations of the April 2002 geomagnetic storm by the global network of incoherent scatter radars. Annales Geophysicae, 23(1), 163-181. https://doi.org/10.5194/angeo-23-163-2005

Observations of the April 2002 geomagnetic storm by the global network of incoherent scatter radars. / Goncharenko, L. P.; Salah, J. E.; Van Eyken, A.; Howells, V.; Thayer, J. P.; Taran, V. I.; Shpynev, B.; Zhou, Q.; Chau, J.

In: Annales Geophysicae, Vol. 23, No. 1, 01.01.2005, p. 163-181.

Research output: Contribution to journalArticle

Goncharenko, LP, Salah, JE, Van Eyken, A, Howells, V, Thayer, JP, Taran, VI, Shpynev, B, Zhou, Q & Chau, J 2005, 'Observations of the April 2002 geomagnetic storm by the global network of incoherent scatter radars', Annales Geophysicae, vol. 23, no. 1, pp. 163-181. https://doi.org/10.5194/angeo-23-163-2005
Goncharenko LP, Salah JE, Van Eyken A, Howells V, Thayer JP, Taran VI et al. Observations of the April 2002 geomagnetic storm by the global network of incoherent scatter radars. Annales Geophysicae. 2005 Jan 1;23(1):163-181. https://doi.org/10.5194/angeo-23-163-2005
Goncharenko, L. P. ; Salah, J. E. ; Van Eyken, A. ; Howells, V. ; Thayer, J. P. ; Taran, V. I. ; Shpynev, B. ; Zhou, Q. ; Chau, J. / Observations of the April 2002 geomagnetic storm by the global network of incoherent scatter radars. In: Annales Geophysicae. 2005 ; Vol. 23, No. 1. pp. 163-181.
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