Band-splitting of coronal and interplanetary type II bursts - III. Physical conditions in the upper corona and interplanetary space

By B. Vršnak, Jasmina Magdalenic, P. Zlobec. 2004

148 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Molecular Biology

View Paper: https://www.semanticscholar.org/paper/8e52decae2f877a5619cc170fbd5513833608fa6

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. B. Vršnak
2. W. Manchester IV
3. L. Green
4. Tibor Török
5. Astrid Veronig
6. M. Temmer
7. R. Schwenn
8. G. Aulanier

In Molecular Biology

1. R. Schwenn
2. W. Manchester IV
3. Astrid Veronig
4. L. Green
5. Tibor Török
6. B. Vršnak
7. M. Temmer

Citations in the corpus

• Space Weather: The Solar Perspective (2006, background): “That would have effects on the formation of shocks in the corona and interplanetary space as well as the temporal behavior of the associated energetic particle events (Gopalswamy et al., 2001a; Mann et al., 1999, 2003; Vrs̆nak et al., 2004; Warmuth and Mann, 2005).”
• The Origin, Early Evolution and Predictability of Solar Eruptions (2018, background): “…CME rapidly decreases with distance from the Sun, because both the electric current I and the magnetic field B protruding through the magnetic structure decrease (for the dependence of the magnetic field on height see, e.g., Dulk and McLean, 1978; Gary, 2001; Vršnak et al, 2002, 2004a; Liu, 2008).”