Results 51 to 60 of about 14,186 (205)
Solar neutrino oscillation phenomenology [PDF]
Pramana, 2004 This article summarises the status of the solar neutrino oscillation phenomenology at the end of 2002 in the light of the SNO and KamLAND results. We first present the allowed areas obtained from global solar analysis and demonstrate the preference of the solar data towards the Large-Mixing-Angle (LMA) MSW solution. A clear confirmation in favor of the
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A NOTE ON THE TORSIONAL OSCILLATION AT SOLAR MINIMUM [PDF]
The Astrophysical Journal, 2009 We examine the evolution of the zonal flow pattern in the upper solar convection zone during the current extended solar minimum, and compare it with that during the previous minimum. The results suggest that a configuration matching that at the previous minimum was reached during 2008, but that the flow band corresponding to the new cycle has been ...
Howe, Rachel +5 more
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The possible role of vortex shedding in the excitation of kink-mode oscillations in the solar corona [PDF]
, 2009 We propose a model for the excitation of horizontally polarised transverse (kink) magnetoacoustic oscillations of solar coronal loops by upflows associated with coronal mass ejections.
V. M. Nakariakov +5 more
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The Astrophysical Journal Supplement SeriesThe TESS space mission has generated an extensive collection of light curves, providing a valuable opportunity to search for solar-like oscillations.
Yezheng Feng +4 more
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, 2009 The Birmingham Solar-Oscillations Network Group has owned, and destroyed, many Pockels cells over the ...
Miller, Brek A. +2 more
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, 2004 The Birmingham Solar-Oscillations Network Group has owned, and destroyed, many Pockels cells over the ...
Miller, Brek A. +2 more
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A Neptunian mirror for solar oscillations [PDF]
Science, 2017 Asteroseismology![Figure][1] The Kepler satellite PHOTO: NASA AMES/JPL-CALTECH/T PYLE The Sun's brightness varies by a tiny amount because of seismic oscillations. The Kepler satellite has detected the same process on other Sun-like stars, which can be used to determine their mass ...
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Solar-Like Oscillations in a Massive Star [PDF]
Science, 2009 Star Gazing Seismology of stars provides a unique insight into physical mechanisms taking place in their interior. Like the Sun, some stars have low-amplitude pulsations that are excited by turbulent convection in their outer layers. Belkacem et al. (p.
Belkacem, Kevin +17 more
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Evolution and characteristics of global pc5 ULF waves during a high solar wind speed interval [PDF]
, 2005 We present an interval of extremely long-lasting narrow-band Pc5 pulsations during the recovery phase of a large geomagnetic storm. These pulsations occurred continuously for many hours and were observed throughout the magnetosphere and in the dusk ...
Mann, I. R. +11 more
core
The n−n¯ oscillations in neutron fluxes running from Sun to Earth
Vestnik Samarskogo Gosudarstvennogo Tehničeskogo Universiteta. Seriâ: Fiziko-Matematičeskie Nauki, 2011 The process of n−n¯ oscillations in the solar cosmic-rays is considered. It is shown that it has high intensity with respect to the analogic processes on the Earth (Ic−r/IEarth∝108), because magnetic field strongly suppresses n−n¯ oscillations. Energetic
L. S. Molchatsky
doaj +1 more source