Marchaudon, A., Blelly, P.‐L., Grandin, M., Aikio, A., Kozlovsky, A., & Virtanen, I. (2018). IPIM modeling of the ionospheric F2 layer depletion at high latitudes during a high‐speed stream event. Space Physics Space Physics, 123, 7051–7066. https://doi.org/10.1029/2018JA025744
IPIM modeling of the ionospheric F₂ layer depletion at high latitudes during a high‐speed stream event
|Author:||Marchaudon, A.1; Blelly, P.-L.1; Grandin, M.2;|
1Institut de Recherche en Astrophysique et Planétologie, Université de Toulouse, CNRS, CNES, Toulouse, France
2Department of Physics, University of Helsinki, Helsinki, Finland
3Ionospheric Physics Research Unit, University of Oulu, Oulu, Finland
4Sodankylä Geophysical Observatory, University of Oulu, Sodankylä, Finland
|Online Access:||PDF Full Text (PDF, 2.7 MB)|
|Persistent link:|| http://urn.fi/urn:nbn:fi-fe201903128671
American Geophysical Union,
|Publish Date:|| 2019-02-28
Our aim is to understand the effect of high‐speed stream events on the high‐latitude ionosphere and more specifically the decrease of the foF2 frequency during the entire day following the impact. First, we have selected one summertime event, for which a large data set was available: Super Dual Auroral Radar Network (SuperDARN) and European Incoherent SCATter (EISCAT) radars, Tromsø and Sodankylä ionosondes, and the CHAllenging Minisatellite Payload (CHAMP) satellite. We modeled with the IPIM model (IRAP Plasmasphere Ionosphere Model) the dynamics of the ionosphere at Tromsø and Sodankylä using inputs derived from the data. The simulations nicely match the measurements made by the EISCAT radar and the ionosondes, and we showed that the decrease of foF2 is associated with a transition from F2 to F1 layer resulting from a decrease of neutral atomic oxygen concentration. Modeling showed that electrodynamics can explain short‐term behavior on the scale of a few hours, but long‐term behavior on the scale of a few days results from the perturbation induced in the atmosphere. Enhancement of convection is responsible for a sharp increase of the ion temperature by Joule heating, leading through chemistry to an immediate reduction of the F2 layer. Then, ion drag on neutrals is responsible for a rapid heating and expansion of the thermosphere. This expansion affects atomic oxygen through nonthermal upward flow, which results in a decrease of its concentration and amplifies the decrease of [O]/[N2] ratio. This thermospheric change explains long‐term extinction of the F2 layer.
Journal of geophysical research. Space physics
|Pages:||7051 - 7066|
|Type of Publication:||
A1 Journal article – refereed
|Field of Science:||
115 Astronomy and space science
114 Physical sciences
This work is supported by the Programme National Soleil Terre (PNST) from Institut des Sciences de l'Univers of Centre National de la Recherche Scientifique (INSU/CNRS) cofunded by CNES and by the Academy of Finland project 285474. M. G. is supported by the Academy of Finland (grant 312351). This work was granted access to the HPC resources of CALMIP supercomputing center under the allocation 2017‐P1520.
|Academy of Finland Grant Number:||
285474 (Academy of Finland Funding decision)
© 2018. American Geophysical Union. All Rights Reserved.