The Library
Scaling laws of quasi-periodic pulsations in solar flares
Tools
Pugh, Chloe E., Broomhall, Anne-Marie and Nakariakov, V. M. (Valery M.) (2019) Scaling laws of quasi-periodic pulsations in solar flares. Astronomy and Astrophysics, 624 . A65. doi:10.1051/0004-6361/201834455 ISSN 0004-6361.
|
PDF
WRAP-scaling-laws-quasi-periodic-pulsations-solar-flares-Pugh-2019.pdf - Accepted Version - Requires a PDF viewer. Download (9Mb) | Preview |
Official URL: https://doi.org/10.1051/0004-6361/201834455
Abstract
Context
Quasi-periodic pulsations (QPPs) are a common feature of solar flares, but previously there has been a lack of observational evidence to support any of the theoretical models that might explain the origin of these QPPs. Aims. We aimed to determine if there are any relationships between the QPP period and other properties of the flaring region, using the sample of flares with QPPs from Pugh et al. (2017b). If any relationships exist then these can be compared with scaling laws for the theoretical QPP mechanisms.
Methods
To obtain the flaring region properties we made use of the Atmospheric Imaging Assembly (AIA) 1600 Å and Helioseismic and Magnetic Imager (HMI) data. The AIA 1600 Å images allow the flare ribbons to be seen while the HMI magnetograms allow the positive and negative magnetic polarity ribbons to be distinguished and the magnetic properties determined. The ribbon properties calculated in this study were the ribbon separation distance, area, total unsigned magnetic flux, and average magnetic field strength. Only the flares that occurred within 60◦ of the solar disk centre were included, which meant a sample of 20 flares with 22 QPP signals.
Results
Positive correlations were found between the QPP period and the ribbon properties. The strongest correlations were with the separation distance and magnetic flux. Because these ribbon properties also correlate with the flare duration, and the relationship between the QPP period and flare duration may be influenced by observational bias, we also made use of simulated data to check if artificial correlations could be introduced. These simulations show that although QPPs cannot be detected for certain combinations of QPP period and flare duration, this does not introduce an apparent correlation. Conclusions. There is evidence of relationships between the QPP period and flare ribbon properties, and in the future the derived scaling laws between these properties can be compared to equivalent scaling laws for theoretical QPP mechanisms.
Item Type: | Journal Article | ||||||||||||
---|---|---|---|---|---|---|---|---|---|---|---|---|---|
Subjects: | Q Science > QB Astronomy | ||||||||||||
Divisions: | Faculty of Science, Engineering and Medicine > Science > Physics | ||||||||||||
Library of Congress Subject Headings (LCSH): | Solar activity, Solar flares, Solar oscillations | ||||||||||||
Journal or Publication Title: | Astronomy and Astrophysics | ||||||||||||
Publisher: | EDP Sciences | ||||||||||||
ISSN: | 0004-6361 | ||||||||||||
Official Date: | 11 April 2019 | ||||||||||||
Dates: |
|
||||||||||||
Volume: | 624 | ||||||||||||
Article Number: | A65 | ||||||||||||
DOI: | 10.1051/0004-6361/201834455 | ||||||||||||
Status: | Peer Reviewed | ||||||||||||
Publication Status: | Published | ||||||||||||
Re-use Statement: | Reproduced with permission from Astronomy & Astrophysics, © ESO | ||||||||||||
Access rights to Published version: | Restricted or Subscription Access | ||||||||||||
Date of first compliant deposit: | 1 March 2019 | ||||||||||||
Date of first compliant Open Access: | 4 March 2019 | ||||||||||||
RIOXX Funder/Project Grant: |
|
Request changes or add full text files to a record
Repository staff actions (login required)
View Item |
Downloads
Downloads per month over past year