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Volume 23, issue 5
Ann. Geophys., 23, 1771–1783, 2005
https://doi.org/10.5194/angeo-23-1771-2005
© Author(s) 2005. This work is distributed under
the Creative Commons Attribution 3.0 License.
Ann. Geophys., 23, 1771–1783, 2005
https://doi.org/10.5194/angeo-23-1771-2005
© Author(s) 2005. This work is distributed under
the Creative Commons Attribution 3.0 License.

  28 Jul 2005

28 Jul 2005

Effects on SuperDARN HF radar echoes of sudden impulses of solar wind dynamic pressure

I. Coco1,2, E. Amata1, M. F. Marcucci1, M. De Laurentis3, J. P. Villain4, C. Hanuise4, and M. Candidi1 I. Coco et al.
  • 1Istituto di Fisica dello Spazio Interplanetario (IFSI), INAF, Rome, Italy
  • 2Earth Science Dept., University of Siena, Italy
  • 3Vitrociset S.p.a., Rome, Italy
  • 4Laboratoire de Physique et Chimie de l’Environnement (LPCE), CNRS/Université d’Orléans, Orléans, France

Abstract. In this work we perform a statistical analysis of the ionospheric echo response observed by six radars of the SuperDARN network in the Northern Hemisphere, over 236 Sudden Impulses (SI) of solar wind dynamic pressure events (from 1997 through 2000). For that purpose, we make use of MRS, the Mean Rate of Scattering, as a function of time during the SI event. We classify the events in sudden increases (I events, 144 cases) and decreases (D events, 92 cases) of the solar wind dynamic pressure. Moreover, we make use of the AE index to define two distinct conditions of the ionosphere under which each event may take place: Quiet and Disturbed. Regarding Quiet conditions, for both I and D events, we find that MRS displays an increase related to the SI time. On the contrary, for Disturbed conditions, D events display an increase in MRS, while I events show a clear dip. The similarity of response for I and D events under Quiet conditions is briefly discussed, but the smaller number of D events does not allow one to further analyse them.

As for the I events, a latitudinal analysis shows that the MRS increase for Quiet conditions is seen both at low latitudes (60°–70° Λ) and at high latitudes (70°–80° Λ); for Disturbed Is the MRS decrease is stronger at high latitudes. We suggest that the MRS increase for Quiet Is can be due to two different mechanisms: 1) a soft electron precipitation induced by Field Line Resonances (FLR) or loss cone instability at lower latitudes; 2) an enlargement of the cusp at higher latitudes, which in turn may induce enhanced particle precipitation.

For what concerns Disturbed Is, the MRS decrease can be produced by a higher energy electron precipitation (>1 keV), that enhances the electron density in the E and D regions. This provokes a strong absorbtion of the radio waves in the D region and a higher refraction in the E region, leading to a decrease in MRS, especially at higher latitudes.

For I events a further classification has been made on the basis of IMF orientation: this suggests that the effects summarized above are due to the SI itself.

Keywords. Ionosphere (Ionospheric irregularities) – Magnetospheric physics (Magnetosphere-ionosphere interactions; Solar wind-magnetosphere interactions)

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