Results 11 to 20 of about 614 (179)
Influences on the radius of the auroral oval [PDF]
We examine the variation in the radius of the auroral oval, as measured from auroral images gathered by the Imager for Magnetopause-to-Aurora Global Exploration (IMAGE) spacecraft, in response to solar wind inputs measured by the Advanced Composition ...
S. E. Milan +4 more
doaj +4 more sources
A radio oval above Earth's auroral oval. [PDF]
Auroral kilometric radiation (AKR), Earth’s strongest radio emission, has long been associated with discrete auroras and electrons near a few kilo–electron volt (keV) range. However, auroras also occur in diffuse forms with broader electron energies, raising the question of why AKR has not been observed above diffuse auroras or linked to electrons ...
Wu S +14 more
europepmc +3 more sources
Problems with mapping the auroral oval and magnetospheric substorms. [PDF]
Accurate mapping of the auroral oval into the equatorial plane is critical for the analysis of aurora and substorm dynamics. Comparison of ion pressure values measured at low altitudes by Defense Meteorological Satellite Program (DMSP) satellites during their crossings of the auroral oval, with plasma pressure values obtained at the equatorial plane ...
Antonova EE +4 more
europepmc +4 more sources
Wandering of the auroral oval 41,000 years ago. [PDF]
In the recent geological past, Earth’s magnetic field reduced to ~10% of the modern values and the magnetic poles shifted away from the geographic poles, causing the Laschamps geomagnetic excursion, about 41 millennia ago. The excursion lasted ~2000 years, with dipole strength reduction and tilting spanning 300 years.
Mukhopadhyay A +8 more
europepmc +5 more sources
The auroral electrojet is enhanced in the polar ionosphere associated with charged particle precipitation and field-aligned currents during substorms. In this paper the geometry of the elctrojet is determined by using the ionospheric equivalent current systems for every 5 minutes during March 18 and 19, 1978.
Chen, Geng-Xiong +4 more
openaire +1 more source
SuperDARN E-region backscatter boundary in the dusk-midnight sector – tracer of equatorward boundary of the auroral oval [PDF]
We compare the locations of the equatorward boundaries of SuperDARN E-region backscatter and Hb emissions, focusing on the dusk-midnight sector of the auroral oval where the proton aurora is statistically located equatorward of the discrete ...
P. T. Jayachandran +6 more
doaj +1 more source
Discontinuity in Jupiter's main auroral oval [PDF]
On the basis of a series of FUV Hubble Space Telescope images obtained between 1997 and 2007 it is shown that there is a segment of the main auroral oval where the emission drops significantly from a few hundreds to a few tens of kiloRayleigh, forming a discontinuity in the oval.
Radioti, Aikaterini +5 more
openaire +2 more sources
Correspondence between the ULF wave power spatial distribution and auroral oval boundaries
The world-wide spatial distribution of the wave power in the Pc5 band during magnetic storms has been compared with auroral oval boundaries. The poleward and equatorward auroral oval boundaries are estimated using either the British Antarctic Survey ...
Kozyreva O.V. +4 more
doaj +1 more source
Thermospheric vertical winds in the auroral oval/polar cap region [PDF]
Thermospheric mean vertical winds from high-resolution Fabry-Perot Spectrometer observations of the l630 nm emission (from ~ 240 km altitude), over a four year interval 1997–2000, from Mawson (67.6° S, 62.9° E, Inv 70.5° S) and Davis (68.6° S, 78.
P. A. Greet +5 more
doaj +1 more source
Article highlights Professional satellite positioning services in the vicinity of the auroral oval region are frequently degraded during night-time.
Knut Stanley Jacobsen +3 more
doaj +1 more source

