EGU21-6775
https://doi.org/10.5194/egusphere-egu21-6775
EGU General Assembly 2021
© Author(s) 2021. This work is distributed under
the Creative Commons Attribution 4.0 License.

Polar cap patches, GPS TEC variations, and atmospheric gravity waves

Paul Prikryl1,2, Robert G. Gillies3, David R. Themens1,4, Bharat S. R. Kunduri5, Roger Varney6, and James M. Weygand7
Paul Prikryl et al.
  • 1University of New Brunswick, Physics Department, Ottawa, ON, Canada
  • 2Geomagnetic Laboratory, Natural Resources Canada, Ottawa, ON, Canada
  • 3Department of Physics and Astronomy, University of Calgary, AB, Canada
  • 4School of Engineering, University of Birmingham, Birmingham, UK
  • 5Bradley Department of Electrical and Computer Engineering, Virginia Tech, Blacksburg, VA, USA
  • 6Center for Geospace Studies, SRI International, Menlo Park, California, USA
  • 7Earth Planetary and Space Sciences, University of California, Los Angeles, CA, USA

The southward pointing field of view of the Canadian component of the Resolute Bay Incoherent Scatter Radar (RISR-C) is well suited for observing the ionospheric signatures of flux transfer events and subsequent polar patch formation in the cusp.  The fast azimuthally oriented flows and associated density depletions often show an enhanced ion temperature from Joule heating caused by the sudden change in plasma flow direction. The newly formed polar patches are then observed as they propagate through the field-of-views of both RISR-C and RISR-N. In the ionosphere, the electron density gradients imposed in the cusp, and small-scale irregularities resulting from gradient-drift instability, particularly in the trailing edges of patches, cause GPS TEC and phase variations, and sometimes amplitude scintillation. The neutral atmosphere is affected by ionospheric currents resulting in Joule heating. The pulses of ionospheric currents in the cusp launch atmospheric gravity waves (AGWs) causing traveling ionospheric disturbances, as they propagate equatorward and upward. On the other hand, the downward propagating AGW packets can impact the lower atmosphere, including the troposphere. Despite significantly reduced wave amplitudes, but subject to amplification upon over-reflection in the upper troposphere, these AGWs can trigger/release existing moist instabilities, initiating convection and latent heat release, the energy leading to intensification of storms.

How to cite: Prikryl, P., Gillies, R. G., Themens, D. R., Kunduri, B. S. R., Varney, R., and Weygand, J. M.: Polar cap patches, GPS TEC variations, and atmospheric gravity waves, EGU General Assembly 2021, online, 19–30 Apr 2021, EGU21-6775, https://doi.org/10.5194/egusphere-egu21-6775, 2021.

Corresponding displays formerly uploaded have been withdrawn.