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Preliminary Results of Tomography Analysis of Westward Traveling Surge

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Preliminary Results of Tomography Analysis of Westward Traveling Surge

Yoshimasa Tanaka1,2,3, Yasunobu Ogawa2,3,Akira Kadokura1,2,3, Takanori Nishiyama2,3, Björn Gustavsson4, Kirsti Kauristie5, Carl-fredrik Enell6, Urban Brändström7, Tima Sergienko7, Alexander Kozlovsky8, Tero Raita8,

Vanhamäki Heikki9, and Akimasa Yoshikawa10

1 Polar Environment Data Science Center, Joint Support-Center for Data Science Research, Research Organization of Information and Systems

2 National Institute of Polar Research

3 The Graduate University for Advanced Studies (SOKENDAI)

4 University of Tromsø - The Arctic University of Norway

5 Finnish Meteorological Institute

6 EISCAT Scientific Association

7 Swedish Institute of Space Physics

8 Sodankylä Geophysical Observatory, Finland

9 University of Oulu, Finland

10 Kyushu University

We present the preliminary results of tomography analysis of a westward traveling surge observed on February 16, 2018.

The campaign of ground-based network observation using multiple monochromatic imagers and the EISCAT-UHF radar was carried out in the northern Europe during February 14-17, 2018, in order to derive three dimensional (3D) current system of various mesoscale auroral vortex structures (e.g., spirals, westward traveling surges, eastward expanding auroral vortices, and omega bands) and quantitatively estimate the ionospheric effect on the formation of them. The auroral activity was high during this period, so we could observe various types of auroras, such as auroral breakups, poleward expansions, westward traveling surges, and omega bands, simultaneously at many stations. In particular, we focus on the westward traveling surge observed around 22:45 UT on February 16. The flow of this research is summarized as follows. (1) We reconstruct 3D structure of the auroral emission by using the auroral computed tomography (ACT) method and derive the height-integrated ionospheric conductivity from the 3D aurora. (2) We derive the ionospheric equivalent current from the ground-based magnetometer network data. (3) We combine the conductivity with the ionospheric equivalent current to estimate the 3D current system (i.e., horizontal ionospheric current and field-aligned current) and horizontal distribution of the electric field. (4) We estimate the Cowling effect on the WTS.

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