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Interdependence of solar wind models and solar wind observations
AIP Conference Proceedings, 1997A 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
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Highly structured slow solar wind emerging from an equatorial coronal hole
Nature, 2019S. Bale +51 more
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Alfvénic velocity spikes and rotational flows in the near-Sun solar wind
Nature, 2019J. Kasper +42 more
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Turbulent Heating and Anisotropy in the Solar Wind, 2019
Victor Montagud-Camps
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Victor Montagud-Camps
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2000
Variations in the Earth’s magnetic field were first observed in the nineteenth century as a sudden increase (by about 10-3 G) followed by a slow decrease. These geomagnetic storms were sometimes found to occur one or two days after large solar flares, and further evidence for a link between the two phenomena came with the discovery of an 11-yr ...
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Variations in the Earth’s magnetic field were first observed in the nineteenth century as a sudden increase (by about 10-3 G) followed by a slow decrease. These geomagnetic storms were sometimes found to occur one or two days after large solar flares, and further evidence for a link between the two phenomena came with the discovery of an 11-yr ...
openaire +1 more source
Molecular engineering of contact interfaces for high-performance perovskite solar cells
Nature Reviews Materials, 2022Furkan H Isikgor +2 more
exaly
Optimal power point tracking of solar and wind energy in a hybrid wind solar energy system
International Journal of Energy and Environmental Engineering, 2021G. B. A. Kumar, Shivashankar
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