Auroral precipitation fading before and at substorm onset: ionospheric and geostationary signatures
| Autor: | Tuija Pulkkinen, Hermann Opgenoorth, Daniel N. Baker, Kirsti Kauristie, A. Huuskonen, M. Syrjäsuo, A. Korth, R. J. Pellinen |
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| Přispěvatelé: | EGU, Publication |
| Jazyk: | angličtina |
| Rok vydání: | 2018 |
| Předmět: |
Atmospheric Science
[SDU.OCEAN] Sciences of the Universe [physics]/Ocean Atmosphere lcsh:QC801-809 Magnetosphere Geology Astronomy and Astrophysics Geophysics Breakup lcsh:QC1-999 Solar wind Current sheet lcsh:Geophysics. Cosmic physics Space and Planetary Science Substorm Earth and Planetary Sciences (miscellaneous) [SDU.STU] Sciences of the Universe [physics]/Earth Sciences GEOS Fading lcsh:Q Ionosphere Longitude lcsh:Science lcsh:Physics |
| Zdroj: | Annales Geophysicae Annales Geophysicae, Vol 15, Pp 967-983 (1997) Annales Geophysicae, Vol 15, Iss 8, Pp 967-983 (0000) |
| ISSN: | 1432-0576 |
| Popis: | Rapid fading of auroral activity a few minutes before substorm breakup has earlier been analyzed in case-studies. Here we report on a study in which all-sky camera (ASC) and magnetic data over 3 years were examined to find breakups that were accompanied by a preceding fading. To illustrate typical features of the fading effect we analyze three events in detail and discuss seven other events to find the spatial and temporal behavior of the fading and the global conditions favoring this phenomenon, which is not associated with every breakup. In these ten events the precipitation diminished typically for about 2 min and a local breakup followed after 2–3 min. Usually the arc which broke up had faded earlier. Comparison with geostationary electron flux recordings shows that in many cases the global onset had already taken place when the fading was recorded at a different longitude. Thus fading is not just a growth-phase phenomenon as often thought, but can also appear as a precursor of the approaching auroral bulge. The AE index and solar-wind data reveal that the fading has a tendency to take place during magnetically disturbed conditions caused by continuous energy input from the solar wind. Furthermore, while a widely recognized phenomenon, we have found that the fading prior to breakup is not a very common feature in the spatio-temporal scale of auroral ASC recordings. In many cases the deepness of the fading had a longitudinal dependence, which leads to the suggestion that this phenomenon is related to azimuthal gradients in the tail magnetic field and/or plasma pressure. Possible scenarios causing fading both before and after the onset are discussed based on a few previously presented theoretical auroral-arc models. |
| Databáze: | OpenAIRE |
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