Skip to main navigation Skip to search Skip to main content

Stationary parts of an EIT and Moreton wave: A topological model

  • Royal Observatory of Belgium
  • LESIA - Laboratoire d'Etudes Spatiales et d'Instrumentation en Astrophysique

Research output: Contribution to journalArticlepeer-review

54 Citations (Scopus)

Abstract

Confexf. EIT and Moreton waves came into focus in 1997, when a propagating disturbance on a large area of the solar disc was discovered. The process generating the EIT and Moreton waves has been frequently discussed. Aims. On May 2, 1998, a halo CME was observed related to an EIT wave, a Moreton wave, a X1 flare, radio emission sources, and dimmings. We studied this event to find the relation between all these structures. Methods. We use and co-align multi-wavelength observations and the online potential field source surface (pfss) package. Results. The observed EIT and Moreton waves present some brightenings that remain at the same location. We relate the connectivity of the coronal potential magnetic field to the stationary brightenings. We find that the areas where the magnetic field lines have drastic jumps of connectivity are cospatial to the stationary brightenings of the waves. Conclusions. We conclude that the BIT and Moreton waves may be due to Joule heating resulting from the generation of electric currents in the neighboring area of the drastic jumps of magnetic connectivity, while the magnetic field lines are opening during a CME.

Original languageEnglish
Pages (from-to)603-612
Number of pages10
JournalAstronomy and Astrophysics
Volume465
Issue number2
DOIs
Publication statusPublished - 1 Apr 2007
Externally publishedYes

Keywords

  • Sun: activity
  • Sun: chromosphere
  • Sun: corona
  • Sun: coronal mass ejections (CMEs)
  • Sun: flares
  • Sun: magnetic fields

Fingerprint

Dive into the research topics of 'Stationary parts of an EIT and Moreton wave: A topological model'. Together they form a unique fingerprint.

Cite this