Pulsating Auroral Forms and Their Association with Geomagnetic Giant Pulsations

On the night of 29/30 October 1987 a giant pulsation (Pg) was recorded on the EISCAT magnetometer cross and the U.K. Sub-Auroral Magnetometer Network (SAMNET), accompanied by a variation in auroral luminosity with an identical periodicity of 77 s. Coincident all-sky image data showed that the aurora...

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Bibliographic Details
Published in:Planetary and Space Science
Main Authors: Taylor, Michael J., Chisham, G., Orr, D.
Other Authors: Elsevier
Format: Text
Language:unknown
Published: Hosted by Utah State University Libraries 1989
Subjects:
Online Access:https://digitalcommons.usu.edu/physics_facpub/1275
https://doi.org/10.1016/0032-0633(89)90117-7
Description
Summary:On the night of 29/30 October 1987 a giant pulsation (Pg) was recorded on the EISCAT magnetometer cross and the U.K. Sub-Auroral Magnetometer Network (SAMNET), accompanied by a variation in auroral luminosity with an identical periodicity of 77 s. Coincident all-sky image data showed that the auroral emissions arose from a series of pulsating patches (which exhibited lifetimes of the order 5–15 s) whose occurrence was modulated with a 77 s periodicity. At several times during this event, a new type of pulsating auroral patch was observed. These data provide a unique example of the auroral precipitation signature during a Pg event.