2025-02-21T08:18:53-05:00 DEBUG: VuFindSearch\Backend\Solr\Connector: Query fl=%2A&wt=json&json.nl=arrarr&q=id%3A%22ujp2-article-2022420%22&qt=morelikethis&rows=5
2025-02-21T08:18:53-05:00 DEBUG: VuFindSearch\Backend\Solr\Connector: => GET http://localhost:8983/solr/biblio/select?fl=%2A&wt=json&json.nl=arrarr&q=id%3A%22ujp2-article-2022420%22&qt=morelikethis&rows=5
2025-02-21T08:18:53-05:00 DEBUG: VuFindSearch\Backend\Solr\Connector: <= 200 OK
2025-02-21T08:18:53-05:00 DEBUG: Deserialized SOLR response
Модель кінематичного динамо для сонячного магнітного циклу

Модель кінематичного динамо для сонячного магнітного циклу

The paper deals with the problem of explaining the origin and nature of the space-time variations in the magnetic activity of the Sun. It presents a new hydrodynamic model of the solar magnetic cycle, which uses helioseismological data on the differential rotation of the solar convective zone. The m...

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Bibliographic Details
Main Authors: Loginov, O.O., Cheremnykh, O.K., Krivodubskij, V.N., Selivanov, Y.O.
Format: Article
Language:English
Published: Publishing house "Academperiodika" 2023
Subjects:
plasma
plasma confinement
magnetohydrodynamics
solar magnetic cycle
solar dynamo
плазма
утримання плазми
магнiтогiдродинамiка
сонячний магнiтний цикл
сонячне динамо
Online Access:https://ujp.bitp.kiev.ua/index.php/ujp/article/view/2022420
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2025-02-21T08:18:53-05:00 DEBUG: VuFindSearch\Backend\Solr\Connector: Query fl=%2A&rows=40&rows=5&wt=json&json.nl=arrarr&q=id%3A%22ujp2-article-2022420%22&qt=morelikethis
2025-02-21T08:18:53-05:00 DEBUG: VuFindSearch\Backend\Solr\Connector: => GET http://localhost:8983/solr/biblio/select?fl=%2A&rows=40&rows=5&wt=json&json.nl=arrarr&q=id%3A%22ujp2-article-2022420%22&qt=morelikethis
2025-02-21T08:18:53-05:00 DEBUG: VuFindSearch\Backend\Solr\Connector: <= 200 OK
2025-02-21T08:18:53-05:00 DEBUG: Deserialized SOLR response

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