An effect of the ionospheric Alfvén resonator on multiband Pc1 pulsations

International audience On 2 December 1999, the magnetometer stations in northern Finland registered structured Pc1 activity simultaneously in three distinct frequency bands. Using simultaneous EISCAT radar measurements of the high-latitude ionosphere, we have studied the ionospheric resonator proper...

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Bibliographic Details
Main Authors: Prikner, K., Mursula, K., Kangas, J., Kerttula, R., Feygin, F. Z.
Other Authors: Geophysical Institute, Czech Academy of Sciences Prague (CAS), Department of Physical Sciences Oulu, University of Oulu, Schmidt United Institute of Physics of the Earth Moscow (IPE), Russian Academy of Sciences Moscow (RAS)
Format: Article in Journal/Newspaper
Language:English
Published: HAL CCSD 2004
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Online Access:https://hal.science/hal-00317245
https://hal.science/hal-00317245/document
https://hal.science/hal-00317245/file/angeo-22-643-2004.pdf
Description
Summary:International audience On 2 December 1999, the magnetometer stations in northern Finland registered structured Pc1 activity simultaneously in three distinct frequency bands. Using simultaneous EISCAT radar measurements of the high-latitude ionosphere, we have studied the ionospheric resonator properties during this multiband Pc1 event. The frequencies of the three structured Pc1 bands were found to closely correspond to the second, third and fourth harmonic of the calculated fundamental frequency of the ionospheric Alfvén resonator (IAR). In addition, those frequencies of the three pearl bands that were closest to the exact IAR harmonics were found to have the strongest intensities. The results demonstrate that the resonator can have an important role on ground-based Pc1 activity over a notably large frequency range, favoring transmission of waves with frequencies close to the resonator's eigenfrequencies. Since the frequencies of all three bands correspond to the maximum rather than the minimum of the transmission coefficient, the traditional bouncing wave packet model needs to be revised. Key words. Ionosphere (auroral ionosphere; ionosphere magnetosphere interactions; wave propagation)