EGU22-1143, updated on 27 Mar 2022
https://doi.org/10.5194/egusphere-egu22-1143
EGU General Assembly 2022
© Author(s) 2022. This work is distributed under
the Creative Commons Attribution 4.0 License.

Interhemispheric Conjugacy of Concurrent Onset and Poleward Traveling Geomagnetic Responses for Throat Aurora Observed Under Quiet Solar Wind Conditions

Hui-Ting Feng1, De‐Sheng Han1, Xiang‐Cai Chen2, Jian‐Jun Liu2, and Zhong‐Hua Xu3
Hui-Ting Feng et al.
  • 1Tongji, School of Ocean and Earth Science, State Key Laboratory of Marine Geology, China (1072868752@qq.com)
  • 2MNR Key Laboratory for Polar Science, Polar Research Institute of China, Shanghai, China,
  • 3Bradley Department of Electrical and Computer Engineering, Virginia Polytechnic Institute and State University, Blacksburg, VA, USA

Throat auroras frequently observed near local noon have been confirmed to correspond to magnetopause indentations, but the generation mechanisms for these indentations and the detailed properties of throat aurora are both not fully understood. Using all‐sky camera and magnetometer observations, we reported some new observational features of throat aurora as follows. (1) Throat auroras can occur under stable solar wind conditions and cause clear geomagnetic responses. (2) These geomagnetic responses can be simultaneously observed at conjugate geomagnetic meridian chains in the Northern and Southern Hemispheres. (3) The initial geomagnetic responses of throat aurora show concurrent onsets that were observed at all stations along the meridians. (4) Immediately after the concurrent onsets, poleward moving signatures and micropositive bays were observed in the X components at higher‐ and lower‐latitude stations, respectively. We argue that these observations provide evidence for throat aurora being generated by low‐latitude magnetopause reconnection. We suggest that the concurrent onsets reflect the instantaneous responses of the reconnection signal arriving at the ionosphere, the followed poleward moving signatures reflect the antisunward dragging of the footprint of newly opened field lines, and the micropositive bays may result from a pair of field‐aligned currents generated during the reconnection. This study may shed new light on the geomagnetic transients observed at cusp latitude near magnetic local noon.

How to cite: Feng, H.-T., Han, D., Chen, X., Liu, J., and Xu, Z.: Interhemispheric Conjugacy of Concurrent Onset and Poleward Traveling Geomagnetic Responses for Throat Aurora Observed Under Quiet Solar Wind Conditions, EGU General Assembly 2022, Vienna, Austria, 23–27 May 2022, EGU22-1143, https://doi.org/10.5194/egusphere-egu22-1143, 2022.