dc.contributor.author |
Jha, Bibhuti Kumar |
|
dc.date.accessioned |
2022-11-16T11:29:37Z |
|
dc.date.available |
2022-11-16T11:29:37Z |
|
dc.date.issued |
2022-09 |
|
dc.identifier.uri |
http://localhost:8080/xmlui/handle/123456789/1339 |
|
dc.description |
The thesis is submitted to Pondicherry University, Pondicherry under the supervision of Prof. Dipankar Banerjee. |
en_US |
dc.description.abstract |
The Sun shows a wide range of temporal variations, from a few seconds to decades and
even centuries, broadly classi ed into two classes short{term and long{term. The solar
dynamo mechanism is believed to be responsible for these global changes happening
in the Sun. Hence, many dynamo models have been proposed to explain the observed
behaviour of the Sun. This thesis is primarily focused on studying the long{term
variation of the Sun and provides various inputs to the solar dynamo models. |
en_US |
dc.language.iso |
en_US |
en_US |
dc.publisher |
ARIES |
en_US |
dc.subject |
Sun; Solar atmosphere; Sunspot; Solar Dynamo Models |
en_US |
dc.title |
Long-term study of the Sun and its implications to Solar Dynamo Models |
en_US |
dc.type |
Thesis |
en_US |