Rotating Magnetic Structures Associated with a Quasi-circular Ribbon Flare
- 1. Yunnan Observatories, Chinese Academy of Sciences, 396 Yangfangwang, Guandu District, Kunming, 650216 (China)
Description
We present the detection of a small eruption and the associated quasi-circular ribbon flare during the emergence of a bipole occurring on 2015 February 3. Under a fan dome, a sigmoid was rooted in a single magnetic bipole, which was encircled by negative polarity. The nonlinear force-free field extrapolation shows the presence of twisted field lines, which can represent a sigmoid structure. The rotation of the magnetic bipole may cause the twisting of magnetic field lines. An initial brightening appeared at one of the footpoints of the sigmoid, where the positive polarity slides toward a nearby negative polarity field region. The sigmoid displayed an ascending motion and then interacted intensively with the spine-like field. This type of null point reconnection in corona led to a violent blowout jet, and a quasi-circular flare ribbon was also produced. The magnetic emergence and rotational motion are the main contributors to the energy buildup for the flare, while the cancellation and collision might act as a trigger.
Availability note (English)
Available from http://dx.doi.org/10.3847/1538-4357/aa5eacAdditional details
Identifiers
Publishing Information
- Journal Title
- Astrophysical Journal
- Journal Volume
- 836
- Journal Issue
- 2
- Journal Page Range
- [10 p.]
- ISSN
- 0004-637X
- CODEN
- ASJOAB
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 49009231
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- BLOWOUTS; COLLISIONS; DETECTION; EXTRAPOLATION; MAGNETIC FIELDS; NONLINEAR PROBLEMS; ROTATION; STELLAR FLARES; SUN
- Descriptors DEC
- ACCIDENTS; MAIN SEQUENCE STARS; MATHEMATICAL SOLUTIONS; MOTION; NUMERICAL SOLUTION; STARS; STELLAR ACTIVITY