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AGU: Journal of Geophysical Research, Space Physics

 

Keywords

  • electron density
  • thermospheric composition
  • thermospheric wind

Index Terms

  • Atmospheric Composition and Structure: Thermosphere: composition and chemistry
  • Ionosphere: Ionospheric disturbances
  • Magnetospheric Physics: Magnetosphere/ionosphere interactions
  • Magnetospheric Physics: Magnetic storms and substorms
  • Atmospheric Processes: Thermospheric dynamics
Abstract
Cited By (2)
 

Abstract

Large variations in the thermosphere and ionosphere during minor geomagnetic disturbances in April 2002 and their association with IMF By

L. Goncharenko

Haystack Observatory, Massachusetts Institute of Technology, Westford, Massachusetts, USA

J. Salah

Haystack Observatory, Massachusetts Institute of Technology, Westford, Massachusetts, USA

G. Crowley

Southwest Research Institute, San Antonio, Texas, USA

L. J. Paxton

John Hopkins University Applied Physics Laboratory, Laurel, Maryland, USA

Y. Zhang

John Hopkins University Applied Physics Laboratory, Laurel, Maryland, USA

A. Coster

Haystack Observatory, Massachusetts Institute of Technology, Westford, Massachusetts, USA

W. Rideout

Haystack Observatory, Massachusetts Institute of Technology, Westford, Massachusetts, USA

C. Huang

Haystack Observatory, Massachusetts Institute of Technology, Westford, Massachusetts, USA

S. Zhang

Haystack Observatory, Massachusetts Institute of Technology, Westford, Massachusetts, USA

B. Reinisch

Center for Atmospheric Research, University of Massachusetts Lowell, Lowell, Massachusetts, USA

V. Taran

Institute for Ionosphere, Kharkiv, Ukraine

We investigate the variations in the thermosphere and ionosphere using multi-instrument observations during the April 2002 period, with a particular focus on periods during small geomagnetic disturbances. Large and long-lasting reductions in the daytime electron density were observed at midlatitudes by incoherent scatter radars, ionosondes, and GPS receivers. These reductions reached 30–50% and were observed over an extended longitudinal area. They propagated to middle latitudes (35–40°N) in the case of a weak geomagnetic disturbance (K p = 3−) and to low latitudes (0–10°N) in the case of a stronger disturbance (K p = 5−). Data from the GUVI instrument aboard the TIMED satellite reveal a reduction in the daytime O/N2 ratio in the coincident area. Similar decreases are also predicted by the TIMEGCM/ASPEN model in both O/N2 ratio and electron density, though the magnitude of the decrease from the model is smaller than observed. We suggest that these ionospheric and thermospheric disturbances result from high-latitude energy input and efficient transport of regions with reduced O/N2 to lower latitudes. We discuss the possible role of a strong positive B y component of the interplanetary magnetic field in the transport of regions with reduced O/N2.

Received 14 July 2004; accepted 9 December 2005; published 15 March 2006.

Citation: Goncharenko, L., et al. (2006), Large variations in the thermosphere and ionosphere during minor geomagnetic disturbances in April 2002 and their association with IMF By, J. Geophys. Res., 111, A03303, doi:10.1029/2004JA010683.

Cited By

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