A search for the relationship between flaring activity and subphotospheric flows

E. Dzifčáková, A. Kulinová, A. G. Kosovichev

Research output: Contribution to journalConference articlepeer-review

3 Scopus citations

Abstract

It is believed that subphotospheric shearing flows play important role in creating unstable magnetic topology that leads to initiation of flares and CME. However, the relationship between the flows and flaring activity is not well understood. Using the flow maps obtained by local helioseismology and magnetic and coronal data we attempt to search for this relationship. In particular, we study the evolution of active region NOAA 9393 in the context of changes in magnetic topology and flaring activity. SOHO/MDI and helioseismology data are used for determining the changes in morphology and are compared with changes of the topology as observed by TRACE.

Original languageEnglish (US)
Pages (from-to)263-266
Number of pages4
JournalEuropean Space Agency, (Special Publication) ESA SP
Issue number517
StatePublished - Feb 1 2003
Externally publishedYes
EventPIC7 - Geneva, Switzerland
Duration: Oct 30 2003Nov 3 2003

All Science Journal Classification (ASJC) codes

  • Aerospace Engineering
  • Space and Planetary Science

Keywords

  • Flares
  • Magnetic reconnection
  • Subphotospheric velocity field

Fingerprint

Dive into the research topics of 'A search for the relationship between flaring activity and subphotospheric flows'. Together they form a unique fingerprint.

Cite this