IDENTIFICATION OF SUPER- AND SUBCRITICAL REGIONS IN SHOCKS DRIVEN BY CORONAL MASS EJECTIONS
- Istituto Nazionale di Astrofisica (INAF), Osservatorio Astronomico di Torino, Strada Osservatorio 20, 10025 Pino Torinese, Torino (Italy)
In this work, we focus on the analysis of a coronal mass ejection (CME) driven shock observed by the Solar and Heliospheric Observatory/Large Angle and Spectrometric Coronagraph Experiment. We show that white-light coronagraphic images can be employed to estimate the compression ratio X = {rho}{sub d}/{rho}{sub u} all along the front of CME-driven shocks. X increases from the shock flanks (where X {approx_equal} 1.2) to the shock center (where X {approx_equal} 3.0 is maximum). From the estimated X values, we infer the Alfven Mach number for the general case of an oblique shock. It turns out that only a small region around the shock center is supercritical at earlier times, while higher up in the corona the whole shock becomes subcritical. This suggests that CME-driven shocks could be efficient particle accelerators at the initiation phases of the event, while at later times they progressively loose energy, also losing their capability to accelerate high-energy particles. This result has important implications on the localization of particle acceleration sites and in the context of predictive space weather studies.
- OSTI ID:
- 21565415
- Journal Information:
- Astrophysical Journal Letters, Vol. 739, Issue 2; Other Information: DOI: 10.1088/2041-8205/739/2/L64; ISSN 2041-8205
- Country of Publication:
- United States
- Language:
- English
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