Ionospheric travelling convection vortices observed by the Greenland magnetometer chain

The Greenland magnetometer array continuously provides geomagnetic variometer data since the early eighties. With the polar cusp passing over it almost every day, the array is suitable to detect ionospheric traveling convection vortices (TCVs), which were rst detected by Friis-Christensen et al. [19...

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Bibliographic Details
Main Authors: Kotsiaros, Stavros, Stolle, Claudia, Friis-Christensen, Eigil, Matzka, Jürgen
Other Authors: Corona, J. Jesus Silva, Böhnel, Harald
Format: Conference Object
Language:English
Published: IAGA 2013
Subjects:
Online Access:https://orbit.dtu.dk/en/publications/0dfd0cb5-8082-464a-a42e-1214b9d08787
https://backend.orbit.dtu.dk/ws/files/59173096/ABSTRACTvolume_IAGA2013.pdf
https://backend.orbit.dtu.dk/ws/files/59173095/IAGA_2013.pdf
http://www.iaga2013.org.mx/public/1/ABSTRACTvolume-IAGA2013.pdf
Description
Summary:The Greenland magnetometer array continuously provides geomagnetic variometer data since the early eighties. With the polar cusp passing over it almost every day, the array is suitable to detect ionospheric traveling convection vortices (TCVs), which were rst detected by Friis-Christensen et al. [1988]. A climatological assessment of their occurrence properties using Greenland data in 1996 has been presented by Clauer and Petrov [2002]. In our ongoing study, a detection algorithm for TCVs in Greenland magnetic data is being developed and the rst results of their climatological assessment are discussed. Specifically, three years of magnetometer data, from 1986 to 1988, collected at seven stations at the West coast of Greenland are analysed and TCV events are identied and isolated. The events are classied with respect to their intensity, duration and time of occurrence and they are correlated with values of the interplanetary magnetic eld (IMF), solar wind velocity and Kp index. The results indicate that TCVs occur usually around magnetic local noon with a typical duration of approximately 15 minutes. TCV detection is clearly facilitated during times of low geomagnetic background activity.