Observations of quasi-periodic phenomena associated with a large blowout solar jet

Morton, Richard, Srivastava, Abhishek and Erdélyi, Robert (2012) Observations of quasi-periodic phenomena associated with a large blowout solar jet. Astronomy & Astrophysics, 542 (A70). ISSN 0004-6361

[img] PDF (arXiv preprint of article published in A&A, 542, A70 (2012))
1204.5033v1.pdf - Submitted Version
Restricted to Repository staff only

Download (595kB) | Request a copy
PDF (Article)
aa17218-11.pdf - Published Version

Download (693kB) | Preview
Official URL: http://dx.doi.org/10.1051/0004-6361/201117218


Aims: A variety of periodic phenomena have been observed in conjunction with large solar jets. We aim to find further evidence for (quasi-)periodic behaviour in solar jets and determine what the periodic behaviour can tell us about the excitation mechanism and formation process of the large solar jet.

Methods: Using the 304 Å (He-II), 171 Å (Fe IX), 193 Å (Fe XII/XXIV) and 131 Å (Fe VIII/XXI) filters onboard the Solar Dynamic Observatory (SDO) Atmospheric Imaging Assembly (AIA), we investigate the intensity oscillations associated with a solar jet.

Results: Evidence is provided for multiple magnetic reconnection events occurring between a pre-twisted, closed field and open field lines. Components of the jet are seen in multiple SDO/AIA filters covering a wide range of temperatures, suggesting the jet can be classified as a blowout jet. Two bright, elongated features are observed to be co-spatial with the large jet, appearing at the jet's footpoints. Investigation of these features reveal they are defined by multiple plasma ejections. The ejecta display (quasi-)periodic behaviour on timescales of 50 s and have rise velocities of 40-150 km/s along the open field lines. Due to the suggestion that the large jet is reconnection-driven and the observed properties of the ejecta, we further propose that these ejecta events are similar to type-II spicules. The bright features also display (quasi)-periodic intensity perturbations on the timescale of 300 s. Possible explanations for the existence of the (quasi-)periodic perturbations in terms of jet dynamics and the response of the transition region are discussed.

Item Type: Article
Subjects: F300 Physics
F500 Astronomy
G100 Mathematics
Department: Faculties > Engineering and Environment > Mathematics, Physics and Electrical Engineering
Related URLs:
Depositing User: Dr Richard Morton
Date Deposited: 05 Oct 2012 08:47
Last Modified: 17 Dec 2023 13:01
URI: https://nrl.northumbria.ac.uk/id/eprint/9436

Actions (login required)

View Item View Item


Downloads per month over past year

View more statistics