CME interactions with coronal holes and their interplanetary consequences

By Nat Gopalswamy, P. Mäkelä, Hong Xie, S. Akiyama, S. Yashiro. 2009

188 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics

View Paper: https://www.semanticscholar.org/paper/9dcbf8b3850e9cde82ad21c6f8208a6283ad231c

How researchers see this paper

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In Astronomy and Astrophysics

1. M. Temmer
2. N. Lugaz
3. B. Vršnak
4. W. Manchester IV
5. C. Farrugia
6. Pete Riley
7. Tibor Török
8. J. Davies

Citations in the corpus

• The Physical Processes of CME/ICME Evolution (2017, background): “Gopalswamy et al. (2009a) and Mohamed et al. (2012) estimated the magnitude and direction of the resultant magnetic force exerted by all coronal holes present on the solar disk during the time of the CME eruption (defined as the CHIP parameter in Mohamed et al. 2012) and compared this with CME…”
• Coronal Mass Ejections: Observations (2012, background): “LASCO has detected well over 104 CMEs during its lifetime (Yashiro et al., 2004; Gopalswamy et al., 2009b; http://cdaw.gsfc.nasa.gov/CME_list/).”
• CONNECTING SPEEDS, DIRECTIONS AND ARRIVAL TIMES OF 22 CORONAL MASS EJECTIONS FROM THE SUN TO 1 AU (2014, background): “CMEs are known to be deflected in the corona by coronal holes (Gopalswamy et al. 2009) and possibly through CME-CME interaction in IP space (Lugaz et al. 2012).”