Inferring plasma flow velocities from photospheric vector magnetic field 
observations for the investigation of flare onsets

Santos, J. C.; Büchner, J.; Zhang, H.

doi:10.1016/j.asr.2007.05.082

Item

ITEM ACTIONSEXPORT

Add to Basket

Local TagsRelease HistoryDetailsSummary

Released

Journal Article

Inferring plasma flow velocities from photospheric vector magnetic field observations for the investigation of flare onsets

MPS-Authors

/persons/resource/persons104182

Santos, J. C.
Department Sun and Heliosphere, Max Planck Institute for Solar System Research, Max Planck Society;

/persons/resource/persons103851

Büchner, J.
Department Sun and Heliosphere, Max Planck Institute for Solar System Research, Max Planck Society;
MPI for Aeronomy, Max Planck Institute for Solar System Research, Max Planck Society;

External Resource

No external resources are shared

Fulltext (restricted access)

There are currently no full texts shared for your IP range.

Fulltext (public)

There are no public fulltexts stored in PuRe

Supplementary Material (public)

There is no public supplementary material available

Citation

Santos, J. C., Büchner, J., & Zhang, H. (2008). Inferring plasma flow velocities from photospheric vector magnetic field observations for the investigation of flare onsets. Advances in Space Research, 42(5), 812-821. doi:10.1016/j.asr.2007.05.082.

Cite as: https://hdl.handle.net/11858/00-001M-0000-0015-007D-8

Abstract

There is no abstract available