Published February 20, 2017 | Version v1
Journal article

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/aa5eac

Additional 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