The influence of geomagnetic activity on polar cap absorption
Cosmic noise absorption data on polar cap analyzed for geomagnetic activity
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Cosmic noise absorption data on polar cap analyzed for geomagnetic activity
Flare plasma cloud model with magnetic field asymmetry for solar-terrestrial system with reference to polar cap absorption and Forbush decrease
Solar phenomena analysis associated with polar cap absorption events from solar flare protons for prediction space radiation conditions
Polar cap absorption analysis - time relation of major flares and radio frequency emissions at centimeter wavelengths
Polar cap absorption riometer data compared for Thule, Greenland and College, Alaska for determining geomagnetic activity influence
Polar cap absorption effect on polar VLF EMISSIONS used for analysis of solar proton events
Onset patterns of polar cap atmosphere due to enhanced ionization caused by penetrating solar cosmic ray particles
Time history analysis for polar cap absorption of solar flare in July, 1966
Three stages of solar cosmic rays entry into polar cap atmosphere due to differential arrival of solar electrons, protons and alpha particles
Polar cap absorption on July 1966, discussing solar flare, radio outburst, proton intensity, geomagnetic latitude, etc
Electron flux and energy spectrum measurements near polar cap investigated for diurnal intensity variations
In this paper we investigated the possibility of using a shape-from-shading technique, applied to a Landsat MSS image, to create a high spatial resolution DEM of Austfonna, an ice cap in Svalbard.
Recent Polar plasma wave observations indicate that intense wideband waves are always present in the polar cap boundary layer (PCBL) region.
In this paper, we evaluate our method on uncalibrated THEMIS data and find 1) agreement with manual cap edge identifications to within 28.2 km, and 2) high accuracy even with a reduced context window, yielding large reductions in memory requirements.
The northern polar residual cap (NPRC) of Mars is a water ice deposit with a rough surface made up of pits, knobs, and linear depressions on scales of tens of meters. This roughness manifests as a series of bright mounds and dark hollows in visible images; these bright and dark patches have a characteristic wavelength and orientation. Spectral data indicate that the surface of the NPRC is composed of large-grained (and therefore old) water ice. Due to the presence of this old ice, it is thought that the NPRC is in a current state of net loss of material a result potentially at odds with impact crater statistics, which suggest ongoing deposition over the past 10-20 Kyr.
We present the first comprehensive discussion of the south seasonal polar cap spectra obtained by the Mariner7 Infrared Spectrometer in the short wavelength region (2-4 µm).
We report four different types of plasma waves detected in the near the dayside polar cap boundary layer (PCBL) region at high altitudes (>6 R***sub E***).
Magnetopause reconnection is known to impact the dayside ionosphere by driving fast ionospheric flows, auroral transients, and high density plasma structures named polar cap patches. However, most of the observed reconnection impact is limited to one hemisphere, and a question arises as to how symmetric the impact is between hemispheres.