Energy loss of solar p modes due to the excitation of magnetic sausage tube waves: importance of coupling the upper atmosphere
- Submitting institution
-
University of Wolverhampton
- Unit of assessment
- 11 - Computer Science and Informatics
- Output identifier
- 1232
- Type
- D - Journal article
- DOI
-
10.1088/0004-637X/789/2/109
- Title of journal
- The Astrophysical Journal
- Article number
- ARTN 109
- First page
- 109
- Volume
- 789
- Issue
- 2
- ISSN
- 0004-637X
- Open access status
- Out of scope for open access requirements
- Month of publication
- June
- Year of publication
- 2014
- URL
-
-
- Supplementary information
-
-
- Request cross-referral to
- -
- Output has been delayed by COVID-19
- No
- COVID-19 affected output statement
- -
- Forensic science
- No
- Criminology
- No
- Interdisciplinary
- Yes
- Number of additional authors
-
2
- Research group(s)
-
-
- Citation count
- 6
- Proposed double-weighted
- No
- Reserve for an output with double weighting
- No
- Additional information
- A fundamental problem in solar physics is understanding the mechanisms behind how the corona is heated to millions of degrees. This paper is significant because for the first time, a stratified, embedded flux tube model is constructed which explicitly couples wave propagation (acoustic and magnetic) within the interior of the Sun to the overlying atmosphere and hence provides a mechanism by which energy can be transferred from the interior to the atmosphere. This work was produced in collaboration with the SP2RC and JILA research groups and is supported by STFC (UK) and NASA grants NNX09AB04G, NNX14AC05G, and NNX14AG05G.
- Author contribution statement
- -
- Non-English
- No
- English abstract
- -
