Geomagn. Aeron.
 2015
DOI: 10.1134/s0016793215080198
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The longitudinal inhomogeneity of the solar toroidal magnetic field generation

V. L. Merzlyakov
1
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L. I. Starkova
2
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Cited by 4 publications
(1 citation statement)
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“…Магнитное поле в период низкой солнечной активности формируется регулярной системой подфотосферных источников [4], которые создают ячеистую структуру поля в экваториальной зоне и средних широтах. В таком случае определяющей компонентой коронального магнитного поля будет B  >> B  , B  >> B r в сферической системе координат, связанной с Солнцем.…”
Section: методикаunclassified

Energy Sorces in the Solar Corona

Merzlyakov1,
Starkova2
2022
Proceedings of the 26th All-Russia Conference on Solar and Solar-Terrestrial Physics
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“…Магнитное поле в период низкой солнечной активности формируется регулярной системой подфотосферных источников [4], которые создают ячеистую структуру поля в экваториальной зоне и средних широтах. В таком случае определяющей компонентой коронального магнитного поля будет B  >> B  , B  >> B r в сферической системе координат, связанной с Солнцем.…”
Section: методикаunclassified

Energy Sorces in the Solar Corona

Merzlyakov1,
Starkova2
2022
Proceedings of the 26th All-Russia Conference on Solar and Solar-Terrestrial Physics
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Peculiarities of the magnetic flux emerging in the equatorial solar zone

Merzlyakov
1
,
Starkova
2
2016
Geomagn. Aeron.
2
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Evolutionary Changes in the Configuration of the Magnetic Field of the Solar Corona in the Epoch of the Minimum

Merzlyakov
1
,
Starkova
2
2019
Geomagn. Aeron.
1
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