Band-splitting of coronal and interplanetary type II bursts - I. Basic properties

By B. Vršnak, H. Aurass, Jasmina Magdalenic, Nat Gopalswamy. 2001

140 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Oceanography

View Paper: https://www.semanticscholar.org/paper/bdf6b49e7b2ff687ceff25e51f06f8c78192c592

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In Astronomy and Astrophysics

1. B. Vršnak
2. Jasmina Magdalenic
3. P. Zlobec
4. W. Manchester IV
5. L. Green
6. Tibor Török
7. Astrid Veronig
8. G. Mann

In Oceanography

1. B. Vršnak
2. Jasmina Magdalenic
3. W. Manchester IV
4. Tibor Török
5. Astrid Veronig
6. L. Green

Citations in the corpus

• Band-splitting of coronal and interplanetary type II bursts - II. Coronal magnetic field and Alfvén velocity (2002, methodology): “The proposed upstream/downstream interpretation apparently had serious drawbacks and some other explanations seemed to be more appropriate (for a review and discussion see Vršnak et al. 2001b; hereinafter Paper I).”
• Band-splitting of coronal and interplanetary type II bursts - III. Physical conditions in the upper corona and interplanetary space (2004, background): “…and theoretical arguments were presented favouring the hypothesis that the band-split is a consequence of the plasma emission from the upstream and downstream shock regions (see also Wild & Smerd 1972; Smerd et al. 1974; Mann et al. 1995; Magdalenić et al. 2002; Vršnak et al. 2001, 2002a, 2002b).”
• The Origin, Early Evolution and Predictability of Solar Eruptions (2018, result): “This is consistent with conclusions drawn by (e.g., Chen, 1989; Vršnak, 1990) and confirmed by observations (e.g., Vršnak et al, 1991; Chen and Krall, 2003).”