Results 11 to 20 of about 1,246,535 (274)
, 2009 The Birmingham Solar-Oscillations Network Group has owned, and destroyed, manyPockels cells over the years.
Miller, Brek A. +2 more
core +21 more sources
Bow shock oscillations of Mars under weakly disturbed solar wind conditions [PDF]
Nature CommunicationsBow shock, where the solar wind first encounters the Martian environment, reflects the complex interplay between the solar wind and Martian upper atmosphere and crustal fields.
Long Cheng +15 more
doaj +2 more sources
, 2004 The Birmingham Solar-Oscillations Network Group has owned, and destroyed, many Pockels cells over the ...
Miller, Brek A. +2 more
core +11 more sources
, 2008 The Birmingham Solar-Oscillations Network Group has owned, and destroyed, many Pockels cells over the ...
Miller, Brek A. +3 more
core +11 more sources
3D numerical simulations of oscillations in solar prominences [PDF]
, 2020 [eng] Context. Oscillations in solar prominences are a frequent phenomenon, and they have been the subject of many studies. A full understanding of the mechanisms that drive them and their attenuation has not been reached yet, however. Aims.
Jaume Terradas Calafell +1 more
core +2 more sources
p-Mode Oscillations in Highly Gravitationally Stratified Magnetic Solar Atmospheres
Physics, 2023 The aim of the study reported in this paper is to gain understanding of solar global oscillations and the propagation characteristics of p-mode oscillations in the highly gravitationally stratified magnetic solar atmosphere.
Michael Griffiths +4 more
doaj +1 more source
SITCoM: SiRGraF Integrated Tool for Coronal dynaMics
Frontiers in Astronomy and Space Sciences, 2023 SiRGraF Integrated Tool for Coronal dynaMics (SITCoM) is based on the Simple Radial Gradient Filter used to filter the radial gradient in the white-light coronagraph images and bring out dynamic structures.
Purvi Udhwani +5 more
doaj +1 more source
On the Origin of Solar Oscillations [PDF]
The Astrophysical Journal, 1998 We have made high resolution observations of the Sun in which we identify individual sunquakes and see power from these seismic events being pumped into the resonant modes of vibration of the Sun. A typical event lasts about five minutes. We report the physical properties of the events and relate them to theories of the excitation of solar oscillations.
Goode, P. L. +3 more
openaire +2 more sources
Remote Sensing, 2022 This research studies the medium timescale (6–30 days) ionospheric response over the Wuhan area to solar radiative, recurrent geomagnetic, and lower atmospheric forcing.
Zhenlin Yang +5 more
doaj +1 more source
The solar oscillations spectrum and the solar cycle [PDF]
Symposium - International Astronomical Union, 1988 During the summer seasons of the years 1977 to 1985 daily velocity measurements of solar global oscillations have been obtained using a resonant scattering spectrometer. After calculating the power spectra of the daily residuals, the mean for each season is found.
A. Jiménez +7 more
openaire +1 more source