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The Deflection of the Cartwheel CME: ForeCAT Results
- Source :
- The Astrophysical Journal. 839:37
- Publication Year :
- 2017
- Publisher :
- American Astronomical Society, 2017.
-
Abstract
- We analyze the Cartwheel coronal mass ejection's (CME; 2008 April 9) trajectory in the low corona with the ForeCAT model. This complex event presented a significant rotation in the low corona and a reversal in its original latitude direction. We successfully reproduce the observed CME's trajectory (latitude and longitude deflection) and speed. Through a test, we are able to constrain the CME's mass to (2.3ā3.0) × 1014 g and the CME's initial shape. We are able to constrain the expansion of the CME as well: the angular width linearly increases until 2.1 , and is constant afterward. In order to match the observed latitude, we include a non-radial initial speed of ā42 km sā1. Despite allowing the CME to rotate in the model, the magnetic forces of the solar background are not able to reproduce the observed rotation. We suggest that the complex reversal in latitude and the significant rotation of the Cartwheel CME can be justified with an asymmetrical reconnection event that ejected the CME non-radially and also initiated its rotation.
- Subjects :
- Physics
010504 meteorology & atmospheric sciences
Astronomy
Astronomy and Astrophysics
Rotation
01 natural sciences
Latitude
Space and Planetary Science
Deflection (engineering)
Physics::Space Physics
0103 physical sciences
Coronal mass ejection
Astrophysics::Solar and Stellar Astrophysics
Astrophysics::Earth and Planetary Astrophysics
010303 astronomy & astrophysics
0105 earth and related environmental sciences
Subjects
Details
- ISSN :
- 15384357
- Volume :
- 839
- Database :
- OpenAIRE
- Journal :
- The Astrophysical Journal
- Accession number :
- edsair.doi...........472ee30c8fdfe0eee2caa02b6d7c3e7b