Coronal dimmings and energetic CMEs in April‐May 1998

By Barbara J. Thompson, E. Cliver, N. Nitta, C. Delannée, J. Delaboudiniere. 2000

166 citations recorded by the source corpus.

View Paper: https://www.semanticscholar.org/paper/82e50148bf9019e48923563aff41f96427577520

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In Astronomy and Astrophysics

Citations in the corpus

Sixty-five years of solar radioastronomy: flares, coronal mass ejections and Sun–Earth connection (2008, background): “…field over a large region, which has been observed in EUV as a large scale dimming or in soft X-rays in the form of dimmings or disappearing transequatorial loops (e.g. Sterling and Hudson 1997; Zarro et al. 1999; Thompson et al. 1998a, 2000; Khan and Hudson 2000; Pohjolainen et al. 2001, 2005).”
The Role of Magnetic Reconnection in the Observable Features of Solar Eruptions (2004, background): “For a brief review of observations of the dimming phenomenon, see Harrison & Lyons (2000), and for individual studies see Sterling & Hudson (1997), Harrison (1997), Zarro et al. (1999), Thompson et al. (2000), Harrison et al. (2003), and references therein.”
NUMERICAL SIMULATION OF AN EUV CORONAL WAVE BASED ON THE 2009 FEBRUARY 13 CME EVENT OBSERVED BY STEREO (2009, unknown): “Secondary dimmings were originally reported by Thompson et al. (2000).”
STEREO IMPACT Investigation Goals, Measurements, and Data Products Overview (2008, unknown): “The model can be applied to take advantage both of distributed in situ measurements for assessing conditions near Earth, and for relating a coronagraph image and EUV maps of coronal holes to the multipoint in situ solar wind and interplanetary magnetic field time series.”
Coronal “Wave”: Magnetic Footprint of a Coronal Mass Ejection? (2007, unknown): “Coronal dimming has also been associated with front-side CMEs (Thompson et al. 2000a).”
Interplanetary flux rope ejected from an X-ray bright point. The smallest magnetic cloud source-region ever observed (2005, background): “Dimmings, i.e. local decreases in emission that indcate loss and/or depletion of mass, are often observed in connection with eruptive events (Sterling & Hudson 1997; Zarro et al. 1999; Thompson et al. 2000).”
On the nature of EIT waves, EUV dimmings and their link to CMEs (2004, background): “Additionally, dimmings are often extended to larger areas than TCHs (Thompson et al. 2000a).”
Direct Observations of the Magnetic Reconnection Site of an Eruption on 2003 November 18 (2005, background): “Generally, such a dark gap in UVCS images could correspond to the traditional EIT dimming (Harrison et al. 2003; Thompson et al. 2000; references therein), which results from severe stretching of the disrupted magnetic field and the consequent transient depletion of the plasma density.”