Astrophysical evidence for the direct electron- neutrino weak interaction.
Plasma neutrino process of Adams, Ruderman and Woo dependent on direct electron-neutrino interaction and connected with stellar evolution
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Plasma neutrino process of Adams, Ruderman and Woo dependent on direct electron-neutrino interaction and connected with stellar evolution
Turbulence and longitudinal heat transfer for accelerating and decelerating flow using Navier- Stokes, continuity and energy equations
Shear and normal strain effects on turbulence and turbulent heat transfer analyzed in model of turbulent boundary layer in accelerating flows
Method of processing data from a spacecraft, where the carrier has a low signal-to-noise ratio and wide unpredictable frequency shifts, consists of analogue recording of the noisy signal along with a high-frequency tone that is used as a clock to trigger a digitizer.
Calibration of water absorption bands in near infrared region
Vlasov equation for solving initial value problem for unstable electron plasma
Quasi-linear theory of turbulent plasmas with fluctuation fields and coherent waves
Magnetosphere model for plasma pressure by solar wind, discussing plasma drift from neutral sheet into geomagnetic tail
Spectroscopic observations of Venus atmosphere rotational temperature based on carbon dioxide band at 7883 A
Nonlinear finite-amplitude instability of two dimensional compressible laminar wake flows, using Fourier expansion and Landau equation
Solution of Cauchy problem for quasilinear equation of first order
Venus upper atmosphere average rotational temperature determined from high dispersion spectroscopic observations of 7883 A carbon dioxide band
Unstable electron plasma initial value problem solved by numerically integrating Vlasov equation in one dimension
Covering properties of topological space as function of set density
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Rotating inviscid incompressible fluids in tubes, investigating axisymmetric nonlinear waves motion in relation to vortex breakdown
Substorm related magnetic field variations in near geomagnetic tail from OGO 5 inbound pass
Sonic boom and explosion shock wave propagation over long distances through turbulence modeled by sound speed fluctuation, including acoustic scattering effect