Results 71 to 80 of about 614 (179)

The auroral oval, the auroral substorm, and their relations with the internal structure of the magnetosphere [PDF]

open access: yesPlanetary and Space Science, 1966
Auroral oval, auroral substorm and relations with internal magnetospheric structure during growth and decay of ring current and neutral sheet ...
openaire   +1 more source

Auroral oval as a beautiful but outdated paradigm [PDF]

open access: yesSolnechno-Zemnaya Fizika, 2015
Being an important region of the polar ionosphere, the auroral oval is considered in many studies on the disturbed magnetosphere. The oval seems to be thoroughly known to all researchers, but there is evidence of misunderstanding in some papers, so it is time to review this matter.
openaire   +1 more source

A Superposed Epoch Analysis of Auroral Oval Coverage During Substorms Using Deep Learning‐Based Segmentation Models

open access: yesSpace Weather
As an effect of solar‐terrestrial activity, the aurora has always been a focus of substorm research. The expansion of the aurora is one of the important characteristics during substorms, which could be directly reflected by the change of auroral oval ...
Jia‐Nan Jiang   +6 more
doaj   +1 more source

Possible role of auroral oval-related currents in two intense magnetic storms recorded by old mid-latitude observatories Clementinum and Greenwich

open access: yesJournal of Space Weather and Space Climate, 2019
Some recent studies point out that currents related to the auroral oval, electrojets and field aligned currents (FACs), are serious candidates for the mechanism of the intense mid-latitude magnetic storms.
Valach Fridrich   +3 more
doaj   +1 more source

Localized aurora beyond the auroral oval [PDF]

open access: yesReviews of Geophysics, 2007
Aurora is the result of the interaction between precipitating energetic electrons and protons with the upper atmosphere. Viewed from space, it generally occurs in continuous and diffuse ovals of light around the geomagnetic poles. Additionally, there are localized regions of aurora that are unrelated to the ovals and exhibit different morphological ...
openaire   +1 more source

A quarter of a century with the auroral oval

open access: yesEos, Transactions American Geophysical Union, 1986
A quarter of a century has elapsed since the concept of auroral oval was introduced into geophysics, and there has been a recent revival of interest among scientists in the evolution throughout the last 3 centuries of our knowledge of the global distribution of auroras. The auroral oval is considered to be a high‐latitude region of the upper atmosphere
openaire   +1 more source

Spatial distribution of auroral precipitation and failures in railway automatics at the north of European Russia

open access: yesSolar-Terrestrial Physics
We study the relationship between space weather disturbances and spatial distribution of failures in railway automatics at segments of Northern and October railways in 2001–2006.
Sakharov Y. A.   +4 more
doaj   +1 more source

Regular observations of the geomagnetic field at the Ógyalla observatory (present-day Hurbanovo) near the turn of the 20th century, including magnetic storms accompanied by auroras in March 1894, September 1898, and October 1903

open access: yesContributions to Geophysics and Geodesy
From 1893 to 1905, the values of the geomagnetic field recorded three times a day are available from the Ógyalla magnetic observatory. We introduce these unique records, and at the same time, we provide an analysis of three noteworthy magnetic storms ...
Fridrich VALACH   +3 more
doaj   +1 more source

Which latitudes of the Russian Federation may be affected by extreme magnetic storms?

open access: yesSolar-Terrestrial Physics
If we consider the auroral oval as an indicator of the electrojet position, the information about the position of its equatorial boundary allows us to predict the latitudes at which the most intense geomagnetic variations can be observed.
Savelieva Natalia   +2 more
doaj   +1 more source

A statistical study of poleward boundary intensifications (PBIs) associated with the arrival of polar cap patches

open access: yesFrontiers in Astronomy and Space Sciences
Poleward Boundary Intensifications (PBIs) are transient auroral brightenings at the poleward edge of the auroral oval that serve as optical tracers of nightside plasma transport and energy deposition.
Yu-Lin Fang   +14 more
doaj   +1 more source

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