Material Outflows from Coronal Intensity “Dimming Regions” during Coronal Mass Ejection Onset

By L. Harra, A. Sterling. 2001

148 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics

View Paper: https://www.semanticscholar.org/paper/d44abe24a70ff97e4bedd2d8953a7b450a77d3cf

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In Astronomy and Astrophysics

1. T. Magara
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Citations in the corpus

• NUMERICAL SIMULATION OF AN EUV CORONAL WAVE BASED ON THE 2009 FEBRUARY 13 CME EVENT OBSERVED BY STEREO (2009, background): “These are regions where the plasma density has dramatically decreased due to plasma evacuation along the “opened” magnetic field, usually occurring during an eruption (e.g. Hudson et al. 1996; Harra & Sterling 2001; Harra et al. 2007).”
• Solar Flares: Magnetohydrodynamic Processes (2011, background): “Although usual dimmings associated with CMEs are attributed to stretching /opening of field lines by eruption (e.g., Sterling and Hudson, 1997; Harra and Sterling, 2001), there is a possibility that some of them are caused by the evacuation via the inflow into reconnection region like above (e.”
• On the nature of EIT waves, EUV dimmings and their link to CMEs (2004, methodology): “Harra & Sterling (2001) used the SOHO Coronal Diagnostic Spectrometer (CDS) data in the O V line (629 Å) to analyze an eruption on July 19, 1999.”