Excitation of P-modes in the sun and stars
(2005) In Symposium - International Astronomical Union 13. p.411-414- Abstract
- P-mode oscillations in the Sun and stars are excited stochasticly by Reynolds stress and entropy fluctuations produced by convection in their outer envelopes. The excitation increases with increasing effective temperature (until envelope convection ceases in the F stars) and also increases with decreasing gravity.
Please use this url to cite or link to this publication:
https://lup.lub.lu.se/record/392728
- author
- Stein, Robert ; Georgobiani, Dali ; Trampedach, Regner ; Ludwig, Hans-Günter LU and Nordlund, Ake
- organization
- publishing date
- 2005
- type
- Contribution to journal
- publication status
- published
- subject
- in
- Symposium - International Astronomical Union
- volume
- 13
- pages
- 411 - 414
- publisher
- Astronomical Society of the Pacific (ASP)
- external identifiers
-
- wos:000240768700113
- ISSN
- 0074-1809
- language
- English
- LU publication?
- yes
- id
- 3a925948-3eb5-4ec1-a037-b22bcc033650 (old id 392728)
- date added to LUP
- 2016-04-01 15:44:27
- date last changed
- 2018-11-21 20:36:04
@article{3a925948-3eb5-4ec1-a037-b22bcc033650, abstract = {{P-mode oscillations in the Sun and stars are excited stochasticly by Reynolds stress and entropy fluctuations produced by convection in their outer envelopes. The excitation increases with increasing effective temperature (until envelope convection ceases in the F stars) and also increases with decreasing gravity.}}, author = {{Stein, Robert and Georgobiani, Dali and Trampedach, Regner and Ludwig, Hans-Günter and Nordlund, Ake}}, issn = {{0074-1809}}, language = {{eng}}, pages = {{411--414}}, publisher = {{Astronomical Society of the Pacific (ASP)}}, series = {{Symposium - International Astronomical Union}}, title = {{Excitation of P-modes in the sun and stars}}, volume = {{13}}, year = {{2005}}, }