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IPIM Modeling of the Ionospheric F 2 Layer Depletion at High Latitudes During a High-Speed Stream Event
- Source :
- Journal of Geophysical Research Space Physics, Journal of Geophysical Research Space Physics, American Geophysical Union/Wiley, 2018, 123 (8), pp.7051-7066. ⟨10.1029/2018JA025744⟩, Journal of Geophysical Research Space Physics, 2018, 123 (8), pp.7051-7066. ⟨10.1029/2018JA025744⟩
- Publication Year :
- 2018
- Publisher :
- HAL CCSD, 2018.
-
Abstract
- International audience; Our aim is to understand the effect of high-speed stream events on the high-latitude ionosphere and more specifically the decrease of the f o F 2 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 f o F 2 is associated with a transition from F 2 to F 1 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 F 2 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]/[N 2 ] ratio. This thermospheric change explains long-term extinction of the F 2 layer.
- Subjects :
- FLUX
010504 meteorology & atmospheric sciences
THERMOSPHERIC COMPOSITION
Incoherent scatter
[SDU.ASTR.EP]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Earth and Planetary Astrophysics [astro-ph.EP]
Super Dual Auroral Radar Network
Plasmasphere
01 natural sciences
7. Clean energy
high-speed stream
ATOMIC OXYGEN
Atmosphere
0103 physical sciences
EXCITATION
ionosondes
RATES
010303 astronomy & astrophysics
0105 earth and related environmental sciences
Geomagnetic storm
ELECTRON-ENERGY TRANSFER
WIND
115 Astronomy, Space science
SuperDARN
Computational physics
EISCAT
PATTERN
Geophysics
13. Climate action
Space and Planetary Science
CONVECTION
Physics::Space Physics
Thermosphere
Ionosphere
Joule heating
GEOMAGNETIC STORM
Subjects
Details
- Language :
- English
- ISSN :
- 21699380 and 21699402
- Database :
- OpenAIRE
- Journal :
- Journal of Geophysical Research Space Physics, Journal of Geophysical Research Space Physics, American Geophysical Union/Wiley, 2018, 123 (8), pp.7051-7066. ⟨10.1029/2018JA025744⟩, Journal of Geophysical Research Space Physics, 2018, 123 (8), pp.7051-7066. ⟨10.1029/2018JA025744⟩
- Accession number :
- edsair.doi.dedup.....f90afdf27c912e6f8efca2badb494a54
- Full Text :
- https://doi.org/10.1029/2018JA025744⟩