Post-noon two-minute period pulsating aurora and their relationship to the dayside convection pattern

Poleward-moving auroral forms, as observed by meridian-scanning photometers, in the vicinity of the cusp region are generally assumed to be the optical signature of flux transfer events. Another class of quasi-continuous, short period (1-2 min) wave-like auroral emission has been identified, closely...
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Gespeichert in:

Autor*in:	S. E. Milan [verfasserIn] T. K. Yeoman [verfasserIn] M. Lester [verfasserIn] J. Moen [verfasserIn] P. E. Sandholt [verfasserIn]

Format:	E-Artikel
Sprache:	Englisch

Erschienen:	1999

Übergeordnetes Werk:	In: Annales Geophysicae - Copernicus Publications, 2002, 17(1999), Seite 877-891
Übergeordnetes Werk:	volume:17 ; year:1999 ; pages:877-891

Links:	Link aufrufen Link aufrufen Link aufrufen Journal toc Journal toc

DOI / URN:	10.1007/s00585-999-0877-8

Katalog-ID:	DOAJ054639654

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520			\|a Poleward-moving auroral forms, as observed by meridian-scanning photometers, in the vicinity of the cusp region are generally assumed to be the optical signature of flux transfer events. Another class of quasi-continuous, short period (1-2 min) wave-like auroral emission has been identified, closely co-located with the convection reversal boundary in the post-noon sector, which is similar in appearance to such cusp aurora. It is suggested that these short period wave-like auroral emissions, the optical signature of boundary plasma sheet precipitation in the region 1 field-aligned current system, are associated with ULF magnetohydrodynamic wave activity, which is observed simultaneously by ground magnetometer stations. This association with ULF wave activity is strengthened by the observation of several harmonic frequencies in the pulsation spectrum, each an overtone of the fundamental standing wave resonance frequency.<br<<br<<b<Key words.</b< Magnetospheric physics (auroral phenomena; magnetopause · cusp · and boundary layers; MHD waves and instabilities)
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callnumber-first	Q - Science
author	S. E. Milan
spellingShingle	S. E. Milan misc QC1-999 misc QC801-809 misc Science misc Q misc Physics misc Geophysics. Cosmic physics Post-noon two-minute period pulsating aurora and their relationship to the dayside convection pattern
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topic_title	QC1-999 QC801-809 Post-noon two-minute period pulsating aurora and their relationship to the dayside convection pattern
topic	misc QC1-999 misc QC801-809 misc Science misc Q misc Physics misc Geophysics. Cosmic physics
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title	Post-noon two-minute period pulsating aurora and their relationship to the dayside convection pattern
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title_full	Post-noon two-minute period pulsating aurora and their relationship to the dayside convection pattern
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title_sort	post-noon two-minute period pulsating aurora and their relationship to the dayside convection pattern
callnumber	QC1-999
title_auth	Post-noon two-minute period pulsating aurora and their relationship to the dayside convection pattern
abstract	Poleward-moving auroral forms, as observed by meridian-scanning photometers, in the vicinity of the cusp region are generally assumed to be the optical signature of flux transfer events. Another class of quasi-continuous, short period (1-2 min) wave-like auroral emission has been identified, closely co-located with the convection reversal boundary in the post-noon sector, which is similar in appearance to such cusp aurora. It is suggested that these short period wave-like auroral emissions, the optical signature of boundary plasma sheet precipitation in the region 1 field-aligned current system, are associated with ULF magnetohydrodynamic wave activity, which is observed simultaneously by ground magnetometer stations. This association with ULF wave activity is strengthened by the observation of several harmonic frequencies in the pulsation spectrum, each an overtone of the fundamental standing wave resonance frequency.<br<<br<<b<Key words.</b< Magnetospheric physics (auroral phenomena; magnetopause · cusp · and boundary layers; MHD waves and instabilities)
abstractGer	Poleward-moving auroral forms, as observed by meridian-scanning photometers, in the vicinity of the cusp region are generally assumed to be the optical signature of flux transfer events. Another class of quasi-continuous, short period (1-2 min) wave-like auroral emission has been identified, closely co-located with the convection reversal boundary in the post-noon sector, which is similar in appearance to such cusp aurora. It is suggested that these short period wave-like auroral emissions, the optical signature of boundary plasma sheet precipitation in the region 1 field-aligned current system, are associated with ULF magnetohydrodynamic wave activity, which is observed simultaneously by ground magnetometer stations. This association with ULF wave activity is strengthened by the observation of several harmonic frequencies in the pulsation spectrum, each an overtone of the fundamental standing wave resonance frequency.<br<<br<<b<Key words.</b< Magnetospheric physics (auroral phenomena; magnetopause · cusp · and boundary layers; MHD waves and instabilities)
abstract_unstemmed	Poleward-moving auroral forms, as observed by meridian-scanning photometers, in the vicinity of the cusp region are generally assumed to be the optical signature of flux transfer events. Another class of quasi-continuous, short period (1-2 min) wave-like auroral emission has been identified, closely co-located with the convection reversal boundary in the post-noon sector, which is similar in appearance to such cusp aurora. It is suggested that these short period wave-like auroral emissions, the optical signature of boundary plasma sheet precipitation in the region 1 field-aligned current system, are associated with ULF magnetohydrodynamic wave activity, which is observed simultaneously by ground magnetometer stations. This association with ULF wave activity is strengthened by the observation of several harmonic frequencies in the pulsation spectrum, each an overtone of the fundamental standing wave resonance frequency.<br<<br<<b<Key words.</b< Magnetospheric physics (auroral phenomena; magnetopause · cusp · and boundary layers; MHD waves and instabilities)
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title_short	Post-noon two-minute period pulsating aurora and their relationship to the dayside convection pattern
url	https://doi.org/10.1007/s00585-999-0877-8 https://doaj.org/article/bac53a163d55463b888c75733e054b6d https://www.ann-geophys.net/17/877/1999/angeo-17-877-1999.pdf https://doaj.org/toc/0992-7689 https://doaj.org/toc/1432-0576
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Post-noon two-minute period pulsating aurora and their relationship to the dayside convection pattern

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