Observations of polar patches generated by solar wind Alfvén wave coupling to the dayside magnetosphere

• Main Authors: Prikryl, P., Macdougall, J. W., Grant, I. F., Steele, D. P., Sofko, G. J., Greenwald, R. A.
• Other Authors: Communications Research Centre Canada (CRC), Department of Physics and Astronomy London, ON, University of Western Ontario (UWO), Institute of Space and Atmospheric Studies Saskatoon (ISAS), Department of Physics and Engineering Physics Saskatoon, University of Saskatchewan Saskatoon (U of S)-University of Saskatchewan Saskatoon (U of S), Johns Hopkins University Applied Physics Laboratory Laurel, MD (APL)
• Format: Article in Journal/Newspaper
• Language: English
• Published: HAL CCSD 1999
• Subjects: [SDU.OCEAN]Sciences of the Universe [physics]/Ocean; Atmosphere; [SDU.STU]Sciences of the Universe [physics]/Earth Sciences; North Magnetic Pole
• Online Access: https://hal.science/hal-00316568; https://hal.science/hal-00316568/document; https://hal.science/hal-00316568/file/angeo-17-463-1999.pdf

International audience A long series of polar patches was observed by ionosondes and an all-sky imager during a disturbed period ( K p = 7- and IMF B z < 0). The ionosondes measured electron densities of up to 9 × 10 11 m -3 in the patch center, an increase above the density minimum between patches by a factor of \sim4.5. Bands of F-region irregularities generated at the equatorward edge of the patches were tracked by HF radars. The backscatter bands were swept northward and eastward across the polar cap in a fan-like formation as the afternoon convection cell expanded due to the IMF B y > 0. Near the north magnetic pole, an all-sky imager observed the 630-nm emission patches of a distinctly band-like shape drifting northeastward to eastward. The 630-nm emission patches were associated with the density patches and backscatter bands. The patches originated in, or near, the cusp footprint where they were formed by convection bursts (flow channel events, FCEs) structuring the solar EUV-produced photoionization and the particle-produced auroral/cusp ionization by segmenting it into elongated patches. Just equatorward of the cusp footprint Pc5 field line resonances (FLRs) were observed by magnetometers, riometers and VHF/HF radars. The AC electric field associated with the FLRs resulted in a poleward-progressing zonal flow pattern and backscatter bands. The VHF radar Doppler spectra indicated the presence of steep electron density gradients which, through the gradient drift instability, can lead to the generation of the ionospheric irregularities found in patches. The FLRs and FCEs were associated with poleward-progressing DPY currents (Hall currents modulated by the IMF B y ) and riometer absorption enhancements. The temporal and spatial characteristics of the VHF backscatter and associated riometer absorptions closely resembled those of poleward moving auroral forms (PMAFs). In the solar wind, IMP 8 observed large amplitude Alfvén waves that were correlated with Pc5 pulsations observed by the ground ...