Toward Understanding the Early Stags of an Impulsively Accelerated Coronal Mass Ejection

Abstract

The expanding magnetic flux in coronal mass ejections (CMEs) often forms a cavity. Studies of CME cavities have so far been limited to the pre-event configuration or to evolved CMEs at large heights, and to two-dimensional imaging data. AIMS. Quantitative analysis of three-dimensional cavity evolution at CME onset can reveal information that is relevant to the genesis of the eruption. METHODS. A spherical model is simultaneously fit to Solar Terrestrial Relations Observatory (STEREO) Extreme Ultraviolet Imager (EUVI) and Inner Coronagraph (COR1) data of an impulsively accelerated CME on 25 March 2008, which displays a well-defined extreme ultraviolet (EUV) and white-light cavity of nearly circular shape already at low heights h approximately = 0.2R. The center height h(t)and radial expansion r(t) of the cavity are obtained in the whole height range of the main acceleration. We interpret them as the axis height and as a quantity proportional to the minor radius of a flux rope, respectively. RESULTS. The three-dimensional expansion of the CME exhibits two phases in the course of its main upward acceleration. From the first h and r data points, taken shortly after the onset of the main acceleration, the erupting flux shows an overexpansion compared to its rise, as expressed by the decrease of the aspect ratio from k = h/r approximately = 3 to k approximately = 3 to k approximately = (1.5-2). This phase is approximately coincident with the impulsive rise of the acceleration and is followed by a phase of very gradual change of the aspect ratio (a nearly self-similar expansion) toward k tilda 2.5 at h tilde 10R. The initial overexpansion of the CME cavity can be caused by flux conservation around a rising flux rope of decreasing axial current and by the addition of flux to a growing, or even newly forming, flux rope by magnetic reconnection. Further analysis will be required to decide

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Document Details

Document Type
Technical Report
Publication Date
Aug 09, 2010
Accession Number
ADA526478

Entities

People

  • Angelos Vourlidas
  • B. Kliem
  • S. Patsourakos

Organizations

  • University of Ioannina

Tags

Communities of Interest

  • Ground and Sea Platforms
  • Space

DTIC Thesaurus Topics

  • Aspect Ratio
  • Astrophysics
  • Coronal Mass Ejections
  • Ejection
  • Geometry
  • Magnetic Flux
  • Observatories
  • Personal Information Managers
  • Shape
  • Soft X Rays
  • Solar System
  • Space Sciences
  • Sun
  • Three Dimensional
  • Two Dimensional
  • White Light
  • X Rays

Fields of Study

  • Physics

Readers

  • Fluid Dynamics.
  • Solar Physics