1977
DOI: 10.1029/ja082i029p04720
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Pulsating aurora: Local and global morphology

Abstract: Pulsating describes a low‐intensity aurora that undergoes rapid alternating increases and decreases in luminosity. Extensive new data available from ground‐based low‐light‐level television cameras and satellite scanners have allowed a detailed study of the pulsating aurora phenomenon. Intensity variations in pulsating auroras may be repetitive, quasi‐periodic, or occasionally periodic with a time scale ranging from less than 1 s to several tens of seconds. The maximum intensity does not exceed approximately 10… Show more

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Cited by 181 publications
(224 citation statements)
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“…Its wavelength was also 1.6 km, but it drifted eastward at 0.6 km/s. The first black curl system lasted for 8 s, and the second one lasted 5 s. These are the same two black curl systems reported by Royrvik [1976].…”
Section: Black Vortex Streetssupporting
confidence: 83%
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“…Its wavelength was also 1.6 km, but it drifted eastward at 0.6 km/s. The first black curl system lasted for 8 s, and the second one lasted 5 s. These are the same two black curl systems reported by Royrvik [1976].…”
Section: Black Vortex Streetssupporting
confidence: 83%
“…Black aurora has been defined as the lack of auroral emissions in well-defined regions within diffuse aurora [Royrvik, 1976;Davis, 1978] …”
mentioning
confidence: 99%
“…A few cropped frames of the FSMI ASI at around ∼1135, 1140, and 1145 UT are given in Figure 7. For the PsA patch under investigation one can clearly see a quasiperiodic "brightening-dimming" cycle over a period of 12-18 s. The patch size is in general 40-80 km in latitudinal dimension while 100-150 km in longitudinal, typical of the PsA [e.g., Royrvik and Davis, 1977]. The patch exhibits an overall eastward bulk motion.…”
Section: Psa Observations and Their Relationship To The Ulf Waves Andmentioning
confidence: 98%
“…[3] Observationally, PsA is a repetitive modulation of the auroral luminosity with typical frequency range 0.05-1 Hz, while a ∼3 Hz modulation are often found to be superimposed on the pulsation structures [e.g., Royrvik and Davis, 1977;Lepine et al, 1980;Yamamoto, 1988;Sato et al, 2004]. The PsA usually occurs in the postmidnight sector during the late expansion and recovery phase of a substorm, and manifests in forms of geostable or slowly convecting luminous patches with scale sizes 10-200 km [Royrvik and Davis, 1977;Johnstone, 1983].…”
Section: Introductionmentioning
confidence: 99%
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