TY - JOUR
T1 - Electrodynamic structure of the morning high-latitude trough region
AU - Vanhamäki, H.
AU - Aikio, A.
AU - Voiculescu, M.
AU - Juusola, L.
AU - Nygrén, T.
AU - Kuula, R.
N1 - Funding Information:
We thank P. Ritter for providing the CHAMP data. The CHAMP mission is sponsored by the Space Agency of the German Aerospace Center (DLR) through funds of the Federal Ministry of Economics and Technology, following a decision of the German Federal Parliament (grant code 50EE0944). The data retrieval and operation of the CHAMP satellite by the German Space Operations Center (GSOC) of DLR is acknowledged. We thank EISCAT for providing us with the data. EISCAT is an international association supported by China (CRIRP), Finland (SA), Japan (STEL and NIPR), Germany (DFG), Norway (NFR), Sweden (VR), and United Kingdom (NERC). We thank the institutes who maintain the IMAGE Magnetometer Array. The solar wind data were obtained from the OMNIWeb service maintained by GSFC/SPDF. We thank Aki Ieda for useful discussions about collision frequencies. This work was supported by the grant 285474 from Academy of Finland. The work of M.V. was partially supported by project PN-II-IDPCE-2011-3-0709, SOLACE (IDEI 283) of the Romanian National Authority for Scientific Research, CNCS, UEFISCDI.
Publisher Copyright:
© 2016. American Geophysical Union. All Rights Reserved.
PY - 2016/3/1
Y1 - 2016/3/1
N2 - We describe the electrodynamics of a postmidnight, high-latitude ionospheric trough, observed with the European Incoherent Scatter radar in northern Scandinavia on 24-25 June 2003 around 22:00-02:30 UT during quiet conditions. The UHF radar made meridian scans with a 30 min cadence resulting in nine cross sections of ionospheric parameters. The F region electric field was also determined with the tristatic system. Ionospheric equivalent currents, calculated from ground magnetometer data, mostly show an electrojet-like current that is reasonably uniform in the longitudinal direction. Combined analysis of the conductances and equivalent current with a local Kamide-Richmond-Matsushita (KRM) method yields the ionospheric electric field and field-aligned current (FAC) in a 2-D (latitude-longitude) area around the radar. We conclude that the most likely scenario is one where the trough is initially created poleward of the auroral oval by downward FAC that evacuates the F region, but as the trough moves to lower latitudes during the early morning hours, it becomes colocated with the westward electrojet. There the electron density further decreases due to increased recombination caused by enhanced ion temperature, which in turn is brought about by a larger convection speed. Later in the morning the convection speed decreases and the trough is filled by increasing photoionization.
AB - We describe the electrodynamics of a postmidnight, high-latitude ionospheric trough, observed with the European Incoherent Scatter radar in northern Scandinavia on 24-25 June 2003 around 22:00-02:30 UT during quiet conditions. The UHF radar made meridian scans with a 30 min cadence resulting in nine cross sections of ionospheric parameters. The F region electric field was also determined with the tristatic system. Ionospheric equivalent currents, calculated from ground magnetometer data, mostly show an electrojet-like current that is reasonably uniform in the longitudinal direction. Combined analysis of the conductances and equivalent current with a local Kamide-Richmond-Matsushita (KRM) method yields the ionospheric electric field and field-aligned current (FAC) in a 2-D (latitude-longitude) area around the radar. We conclude that the most likely scenario is one where the trough is initially created poleward of the auroral oval by downward FAC that evacuates the F region, but as the trough moves to lower latitudes during the early morning hours, it becomes colocated with the westward electrojet. There the electron density further decreases due to increased recombination caused by enhanced ion temperature, which in turn is brought about by a larger convection speed. Later in the morning the convection speed decreases and the trough is filled by increasing photoionization.
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U2 - 10.1002/2015JA022021
DO - 10.1002/2015JA022021
M3 - Article
AN - SCOPUS:84961262718
SN - 2169-9380
VL - 121
SP - 2669
EP - 2682
JO - Journal of Geophysical Research: Space Physics
JF - Journal of Geophysical Research: Space Physics
IS - 3
ER -