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Interdependence of solar wind models and solar wind observations

AIP Conference Proceedings, 1997
A brief overview of the observations in the inner corona is presented together with three different solar wind models. It is shown that the very high flow speeds derived from the observations in the inner corona can be modeled if either the proton temperature is extremely high, or if there exists a mechanism that adds momentum to the flow much closer ...
Ruth Esser, Nancy S. Brickhouse
openaire   +1 more source

SOLAR/WIND POWER PLANTS

Solar & Wind Technology, 1986
Abstract This paper discusses the background, theory, design, construction, costs and economics of solar/wind power plants and provides a brief description of the 50 kW plant which has been built in Spain to demonstrate the feasibility of the concept and to verify the theoretical work.
openaire   +1 more source

Solar Wind Correlations: Using a Solar Wind Monitor Successfully

1999
Solar wind plasma correlations between data from three spacecraft — IMP 8, INTERBALL-1, and WIND — are analyzed for periods near the most recent solar minimum. There are two primary foci of this study: 1) to understand the physics underlying good and poor correlation periods, and 2) to investigate and quantify the degree to which distant solar wind ...
K. I. Paularena   +3 more
openaire   +1 more source

Solar-Wind Disturbances and the Solar Wind-Magnetosphere Energy Coupling Function

Space Science Reviews, 1983
Recent studies of the solar wind-magnetosphere interaction are reviewed in terms of the input-output relationship. We show that the magnetosphere is primarily a directly driven system and that the interaction constitutes a dynamo. As another important problem of the interaction, we examine the chain of processes by which the dynamo-generated power is ...
openaire   +1 more source

Impact of siting ordinances on land availability for wind and solar development

Nature Energy, 2023
Anthony Lopez   +2 more
exaly  

Solar Orbiter Neutral Solar Wind Detector

2006
Neutral hydrogen atoms, which give rise to the prominent so lar Ly-alpha corona, are closely coup led to the emerging solar-wind plasma. The density ratio of neutral hydrogen to protons is minute, ~10-6; therefore, the neutral atoms are tracers in the solar wind.
M Hilchenbach   +36 more
openaire   +4 more sources

The evolution of the solar wind

Living Reviews in Solar Physics, 2021
Aline A Vidotto
exaly  

THE SOLAR WIND

2018
Axford, W., McKenzie, J.
openaire   +2 more sources

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