Skip to main content
Log in

Observed form and action of the magnetic field in flares

Extended abstract

  • Published:
Solar Physics Aims and scope Submit manuscript

This is a preview of subscription content, log in via an institution to check access.

Access this article

Price excludes VAT (USA)
Tax calculation will be finalised during checkout.

Instant access to the full article PDF.

Author information

Authors and Affiliations

Authors

Additional information

Moore, R. L.: 1988, “Evidence that Magnetic Energy Shedding in Solar Filament Eruptions is the Drive in Accompanying Flares and Coronal Mass Ejections,” Astrophys. J., in press.

Rights and permissions

Reprints and permissions

About this article

Cite this article

Moore, R.L. Observed form and action of the magnetic field in flares. Sol Phys 113, 121–124 (1987). https://doi.org/10.1007/BF00147689

Download citation

  • Published:

  • Issue Date:

  • DOI: https://doi.org/10.1007/BF00147689

Keywords

Navigation