Results 41 to 50 of about 14,186 (205)
Solar Oscillations and Convection. II. Excitation of Radial Oscillations [PDF]
The Astrophysical Journal, 2001 Solar p-mode oscillations are excited by the work of stochastic, non-adiabatic, pressure fluctuations on the compressive modes. We evaluate the expression for the radial mode excitation rate derived by Nordlund and Stein (Paper I) using numerical simulations of near surface solar convection.
Stein, R.F., Nordlund, Åke
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Evidence of 5 minute Oscillations from Parker Solar Probe
The Astrophysical Journal LettersThe Sun’s surface vibrates in characteristic 5 minute oscillations, known as p -modes, generated by sound waves trapped within the convection zone. Although these oscillations have long been hypothesized to reach into the solar wind, direct in situ ...
Zesen Huang +21 more
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SOLAR NEUTRINO OSCILLATION – AN OVERVIEW [PDF]
PASCOS 2004, 2005 After a brief summary of the neutrino oscillation formalism and the solar neutrino sources and experiments I discuss the matter effect on solar neutrino oscillation. Then I discuss how the resulting alternative solutions are experimentally resolved in favour of the LMA solution, with particular exphasis on the SK, SNO and KL data.
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Solar Oscillations and Convection. I. Formalism for Radial Oscillations [PDF]
The Astrophysical Journal, 2001 13 pages, 3 ...
Nordlund, Åke, Stein, R.F.
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High-latitude observations of impulse-driven ULF pulsations in the ionosphere and on the ground [PDF]
, 2003 International audienceWe report the simultaneous observation of 1.6?1.7 mHz pulsations in the ionospheric F-region with the CUTLASS bistatic HF radar and an HF Doppler sounder, on the ground with the IMAGE and SAMNET magnetometer arrays, and in the ...
Menk, F. W. +14 more
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The influence of opacity on inferred MHD wave signatures in the lower solar atmosphere
Frontiers in Astronomy and Space SciencesMagnetohydrodynamic wave activity in small-scale magnetic structures, such as solar pores, provides key insights into energy transport in the lower solar atmosphere.
Samuel J. Skirvin +15 more
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Physics of solar-like oscillations [PDF]
Solar Physics, 2004 AbstractThe physics of solar and stellar oscillations determine their observable characteristics. I provide a brief overview of the properties of solar-like oscillations, excited by stochastic processes, in other stars. In addition, I consider the current state of investigations of such oscillations, as well as the prospects for an improved ...
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The 11-year solar cycle, the 27-day Sun's rotation and the area of the stratospheric Aleutian high
Meteorologische Zeitschrift, 2001 The effect of the 11-year solar cycle on the 30-hPa geopotential height and temperature fields in the area of the Aleutian high caused by solar activity oscillations resulting from the Sun's rotation (27.2 d) is investigated, applying methods of ...
Boris Soukharev, Karin Labitzke
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Solar Mass-Varying Neutrino Oscillations [PDF]
Physical Review Letters, 2005 We propose that the solar neutrino deficit may be due to oscillations of mass-varying neutrinos (MaVaNs). This scenario elucidates solar neutrino data beautifully while remaining comfortably compatible with atmospheric neutrino and K2K data and with reactor antineutrino data at short and long baselines (from CHOOZ and KamLAND).
Marfatia, Danny +2 more
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Solar-forced diurnal regulation of cave drip rates via phreatophyte evapotranspiration [PDF]
Hydrology and Earth System Sciences, 2016 We present results of a detailed study of drip rate variations at 12 drip discharge sites in Glory Hole Cave, New South Wales, Australia. Our novel time series analysis, using the wavelet synchrosqueezed transform, reveals pronounced oscillations at ...
K. Coleborn +7 more
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