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Solar activity and the solar wind

Reviews of Geophysics, 1979
The availability of in situ solar wind observations from the complete sunspot cycle 20 (1964–1976) suggests an examination of the changes in the character of the solar wind related to the solar cycle and comparison of these observed changes with those expected from earlier studies of solar‐terrestrial physics.
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The Sun and the Solar Wind

1990
Some 4.56 billion years ago, out of the gravitational collapse of a cloud in the interstellar medium with angular momentum L, a rotating star — the Sun — was formed, and began to burn hydrogen into helium and heavier nuclei. A gaseous disc in the plane orthogonal to L developed; its chemical composition, initially the same as in the solar photosphere ...
Bruno Bertotti   +2 more
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The Solar Wind

2021
Alexis P., Rouillard   +64 more
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Diagnostics of the Solar Wind Plasma

2009
The solar wind is a fully ionized plasma, coming from the outer atmosphere of the Sun, the so-called solar corona, which expands as a supersonic flow into the interplanetary medium [55]. The first observations indicating that the Sun might be emitting a wind were made by Biermann in 1946 of comet tails [1], which are observed to point away from the Sun.
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The solar wind in the Universe

2007
‘To an astronomer, man is nothing more than an insignificant dot in an infinite universe,’ someone once said to Einstein. To which Einstein replied: ‘But I realise that the insignificant dot who is man is also the astronomer.’ What is the solar wind to an astronomer?
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Molecular engineering of contact interfaces for high-performance perovskite solar cells

Nature Reviews Materials, 2022
Furkan H Isikgor   +2 more
exaly  

The Origin of the Solar Wind

American Scientist, 2002
Shadia Rifai Habbal, Richard Woo
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Stability challenges for the commercialization of perovskite–silicon tandem solar cells

Nature Reviews Materials, 2023
Leiping Duan, Kylie R Catchpole
exaly  

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