Multiple magnetic clouds: Several examples during March-April 2001

By Yuming Wang, P. Ye, Shui Wang. 2003

156 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics

View Paper: https://www.semanticscholar.org/paper/9f4659d47f5965817d699e8d7211bcb6355bd92c

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

In Astronomy and Astrophysics

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

Citations in the corpus

• The Physical Processes of CME/ICME Evolution (2017, background): “In situ measurements at 1 AU of shocks propagating inside CMEs (Lugaz et al. 2015) revealed the compression of the leading CME by the overtaking shock and CME (Wang et al. 2003b; Farrugia and Berdichevsky 2004; Liu et al. 2012, 2014c).”
• Geoeffective Properties of Solar Transients and Stream Interaction Regions (2017, background): “Complex ejecta, in general, do not have well-ordered magnetic fields, but may have a sustained period of enhanced southward magnetic fields produced by CME-CME interactions (e.g., Farrugia and Berdichevsky 2004; Wang et al. 2003; Liu et al. 2014a; Lugaz and Farrugia 2014).”
• The Interaction of Successive Coronal Mass Ejections: A Review (2016, background): “The two MCs are separated by a short period of large plasma β, corresponding to hot plasma with weaker and more turbulent magnetic field (Wang, Ye, and Wang, 2003), which may be an indication of reconnection between the ejecta (see Figure 10a).”