A slow mode wave as a possible source of Pi 2 and associated particle precipitation: a case study
Abstract. An intensi®cation of auroral luminosity referred to as an auroral break-up often accompanies the onset of geomagnetic pulsation (Pi 2) at the dip-equator. One such auroral break-up occurred at 2239 UT on 16 June, 1986, being accompanied by weak substorm activity (AE 50 nT) which was record...
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ftciteseerx:oai:CiteSeerX.psu:10.1.1.371.7529 2023-05-15T14:01:15+02:00 A slow mode wave as a possible source of Pi 2 and associated particle precipitation: a case study O. Saka O. Watanabe K. Okada D. N. Baker The Pennsylvania State University CiteSeerX Archives application/pdf http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.371.7529 http://hal.archives-ouvertes.fr/docs/00/31/65/98/PDF/angeo-17-674-1999.pdf en eng http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.371.7529 http://hal.archives-ouvertes.fr/docs/00/31/65/98/PDF/angeo-17-674-1999.pdf Metadata may be used without restrictions as long as the oai identifier remains attached to it. http://hal.archives-ouvertes.fr/docs/00/31/65/98/PDF/angeo-17-674-1999.pdf text ftciteseerx 2016-01-08T01:20:37Z Abstract. An intensi®cation of auroral luminosity referred to as an auroral break-up often accompanies the onset of geomagnetic pulsation (Pi 2) at the dip-equator. One such auroral break-up occurred at 2239 UT on 16 June, 1986, being accompanied by weak substorm activity (AE 50 nT) which was recorded in all-sky image of Syowa Station, Antarctica (66.2°S, 71.8°E in geomagnetic coordinates). The associated Pi 2 magnetic pulsation was detected by a ¯uxgate magnetometer in the afternoon sector at the dip-equator (Huancayo, Peru; 1.44°N, 355.9 ° in geomagnetic coordinates; 12.1°S, 75.2°W in geographic coordinates; L ˆ 1:00). In spite of the large separation of the two stations in longitude and latitude, the auroral break-up and subsequent luminosity modulation were seen to be correlated with the wave form of the ground Pi 2 pulsation. This occurred in such a way that the luminosity maximum was seen to occur at the phase of maximum amplitudes of Pi 2 wave form. We argue that the observed correlation could be interpreted as indicating a Pi 2-modulation of a ®eld-aligned acceleration of the low energy electrons that may occur near the equator of the midnight magnetosphere. Key words. Magnetospheric physics (auroral phenomena; energetic particles, precipitating; MHD waves and instabilities) Text Antarc* Antarctica Unknown Syowa Station |
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English |
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Abstract. An intensi®cation of auroral luminosity referred to as an auroral break-up often accompanies the onset of geomagnetic pulsation (Pi 2) at the dip-equator. One such auroral break-up occurred at 2239 UT on 16 June, 1986, being accompanied by weak substorm activity (AE 50 nT) which was recorded in all-sky image of Syowa Station, Antarctica (66.2°S, 71.8°E in geomagnetic coordinates). The associated Pi 2 magnetic pulsation was detected by a ¯uxgate magnetometer in the afternoon sector at the dip-equator (Huancayo, Peru; 1.44°N, 355.9 ° in geomagnetic coordinates; 12.1°S, 75.2°W in geographic coordinates; L ˆ 1:00). In spite of the large separation of the two stations in longitude and latitude, the auroral break-up and subsequent luminosity modulation were seen to be correlated with the wave form of the ground Pi 2 pulsation. This occurred in such a way that the luminosity maximum was seen to occur at the phase of maximum amplitudes of Pi 2 wave form. We argue that the observed correlation could be interpreted as indicating a Pi 2-modulation of a ®eld-aligned acceleration of the low energy electrons that may occur near the equator of the midnight magnetosphere. Key words. Magnetospheric physics (auroral phenomena; energetic particles, precipitating; MHD waves and instabilities) |
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The Pennsylvania State University CiteSeerX Archives |
format |
Text |
author |
O. Saka O. Watanabe K. Okada D. N. Baker |
spellingShingle |
O. Saka O. Watanabe K. Okada D. N. Baker A slow mode wave as a possible source of Pi 2 and associated particle precipitation: a case study |
author_facet |
O. Saka O. Watanabe K. Okada D. N. Baker |
author_sort |
O. Saka |
title |
A slow mode wave as a possible source of Pi 2 and associated particle precipitation: a case study |
title_short |
A slow mode wave as a possible source of Pi 2 and associated particle precipitation: a case study |
title_full |
A slow mode wave as a possible source of Pi 2 and associated particle precipitation: a case study |
title_fullStr |
A slow mode wave as a possible source of Pi 2 and associated particle precipitation: a case study |
title_full_unstemmed |
A slow mode wave as a possible source of Pi 2 and associated particle precipitation: a case study |
title_sort |
slow mode wave as a possible source of pi 2 and associated particle precipitation: a case study |
url |
http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.371.7529 http://hal.archives-ouvertes.fr/docs/00/31/65/98/PDF/angeo-17-674-1999.pdf |
geographic |
Syowa Station |
geographic_facet |
Syowa Station |
genre |
Antarc* Antarctica |
genre_facet |
Antarc* Antarctica |
op_source |
http://hal.archives-ouvertes.fr/docs/00/31/65/98/PDF/angeo-17-674-1999.pdf |
op_relation |
http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.371.7529 http://hal.archives-ouvertes.fr/docs/00/31/65/98/PDF/angeo-17-674-1999.pdf |
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Metadata may be used without restrictions as long as the oai identifier remains attached to it. |
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1766270843168489472 |