Numerical Modeling of Magnetohydrodynamic Wave Propagation and Refraction in Sunspots

By E. Khomenko, Manel Collados. 2006

136 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Oceanography

View Paper: https://www.semanticscholar.org/paper/1d6d910f94b700971b197a69ddc4e89082d29149

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. H. Spruit
2. Laurent Gizon
3. A. Birch
4. E. Khomenko
5. Manel Collados
6. G. Verth
7. R. Morton
8. S. Grant

In Oceanography

1. A. Birch
2. H. Spruit
3. Laurent Gizon
4. E. Khomenko
5. Manel Collados

Citations in the corpus

• Local Helioseismology: Three-Dimensional Imaging of the Solar Interior (2010, methodology): “The first approach is numerical simulations of wave propagation through prescribed background models (e.g. Cally & Bogdan 1997; Cameron, Gizon & Daiffallah 2007; Hanasoge 2008; Khomenko & Collados 2006; Parchevsky & Kosovichev 2009).”
• Oscillations and Waves in Sunspots (2015, methodology): “Figure 16 gives an example of the fast and slow magneto-acoustic wave paths, calculated for a two-dimensional case in the photospheric and chromospheric part of a sunspot model from Khomenko and Collados (2006).”
• Multiwavelength Studies of MHD Waves in the Solar Chromosphere (2015, background): “Khomenko and Collados (2006) produced numerical simulations of the lower solar atmosphere and revealed how ∼3 minute magnetoacoustic oscillations generated at the base of a sunspot umbra can readily propagate upwards through the lower layers and into the transition region.”