Modelling the sun's small scale global photospheric magnetic field
- Submitting institution
-
Abertay University
- Unit of assessment
- 12 - Engineering
- Output identifier
- 17661604
- Type
- D - Journal article
- DOI
-
10.3847/0004-637X/830/2/160
- Title of journal
- Astrophysical Journal
- Article number
- 160
- First page
- -
- Volume
- 830
- Issue
- 2
- ISSN
- 0004-637X
- Open access status
- Compliant
- Month of publication
- October
- Year of publication
- 2016
- 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
- No
- Number of additional authors
-
1
- Research group(s)
-
D - Modelling & Simulation
- Proposed double-weighted
- No
- Reserve for an output with double weighting
- No
- Additional information
- This paper considers one possibility for how the Sun’s surface magnetic field distribution would look during a grand minimum of activity, such as was observed from 1645 – 1715. This is significant as it considers the potential impact of such a weak field on the near-Earth environment (Space weather). This work formed the basis for a successful Carnegie Trust Research Incentive Grant (RIG70554). We were pleased to have the opportunity to present our paper as a contributed talk at the AAS Solar Physics Division meeting 2014
- Author contribution statement
- -
- Non-English
- No
- English abstract
- -
