Results 11 to 20 of about 926,286 (251)

Polar cap patch prediction in the expanding contracting polar cap paradigm [PDF]

open access: yesSpace Weather, 2019
Space weather can cause serious disturbances of global navigation satellite systems (GNSS) used for positioning and navigation purposes. This paper describes a new method to forecast space weather disturbances on GNSS at high latitudes, in which we ...
Jin, Yaqi   +9 more
core   +3 more sources

On the Creation, Depletion, and End of Life of Polar Cap Patches [PDF]

open access: yesJournal of Geophysical Research: Space Physics, 2023
Ionospheric convection patterns from the Super Dual Auroral Radar Network are used to determine the trajectories, transit times, and decay rates of three polar cap patches from their creation in the dayside polar cap ionosphere to their end of life on ...
Lorentzen, Dag Arne   +13 more
core   +8 more sources

Do the Throat Auroras Create Polar Cap Patches?

open access: yesGeophysical Research Letters, 2023
Throat auroras and polar cap patches are common phenomena in the polar ionosphere resulting from magnetosphere‐ionosphere coupling. A campaign was organized, with all‐sky imagers at Yellow River Station, the European Incoherent Scatter Svalbard Radar ...
Duan Zhang   +12 more
doaj   +4 more sources

Observations and modeling of scintillation in the vicinity of a polar cap patch

open access: yesJournal of Space Weather and Space Climate, 2022
Small-scale ionospheric plasma structures can cause scintillation in radio signals passing through the ionosphere. The relationship between the scintillated signal and how plasma structuring develops is complex.
Lamarche Leslie J.   +2 more
doaj   +2 more sources

Relationship of Theoretical Patch Climatology to Polar Cap Patch Observations [PDF]

open access: yesRadio Science, 1996
During a southward orientation of the interplanetary magnetic field (IMF), patches are often observed moving antisunward across the polar cap.
Sojka, Jan Josef   +5 more
core   +4 more sources

Positive storm effects in the dayside polar ionospheric F-region observed by EISCAT and ESR during the magnetic storm of 15 May 1997 [PDF]

open access: yesAnnales Geophysicae, 2002
EISCAT/ESR radar data and in situ FAST and POLAR satellite observations are coordinately analyzed to investigate positive ionospheric storm effects in the dayside upper F-region in both the polar cap and the auroral oval during the magnetic storm ...
S. Y. Ma   +5 more
doaj   +3 more sources

Seasonal influence on polar cap patches in the high-latitude nightside ionosphere [PDF]

open access: yesJournal of Geophysical Research: Space Physics, 2010
The influence of the season on the patch-to-background density ratio of polar cap patches in the nightside ionosphere was observed above northern Scandinavia around solar maximum (1999–2001).
Wood, Alan   +4 more
core   +2 more sources

Review of ionospheric effects of solar wind magnetosphere coupling in the context of the expanding contracting polar cap boundary model [PDF]

open access: yes, 2006
This paper reviews the coupling between the solar wind, magnetosphere and ionosphere. The coupling between the solar wind and Earth’s magnetosphere is controlled by the orientation of the Interplanetary Magnetic Field (IMF).
Milan, S. E.   +3 more
core   +4 more sources

Morphology of polar cap patch activity [PDF]

open access: yesRadio Science, 1999
For the period July 1, 1989, to June 30, 1990, for high solar activity, ƒ0F2 data were recorded by the Digital Ionospheric Sounding Systems from two Qaanaaq and Sondrestromfjord; ionospheric UHF scintillation data were recorded from Thule; and airglow images were recorded from Qaanaaq.
B. S. Dandekar, T. W. Bullett
openaire   +2 more sources

Periodicities of polar cap patches [PDF]

open access: yesJournal of Geophysical Research: Space Physics, 2013
A highly sensitive all‐sky electron multiplier charge‐coupled device airglow imager has been operative in Longyearbyen, Norway since October 2011. The imager captures 630.0 nm all‐sky images with an exposure time of 4 s, which is about 10 times shorter than that achieved by conventional cooled CCD imagers.
K. Hosokawa   +3 more
openaire   +1 more source

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