Ultraviolet Events Observed in Active Regions. I. Observations and Scenario
Abstract
UV line data obtained in solar active regions on and near the limb, taken with the Ultraviolet Spectrometer and Polarimeter experiment on the Solar Maximum Mission are examined. The study provides insight into the physical processes behind sudden localized brightenings (or microflares) that occur within these active regions and their relation to surging activity. Time sequences of rasters and rasters through the line (taken in Ly-alpha and N V lines simultaneously) and C IV dopplergrams are the core of these data. They show the brightening events on the disk and Doppler shifts in dynamic events on the disk and above the limb. The study suggests, for the events, a localized energy deposition in a region of the chromosphere that heats the material and produces a pressure pulse. This mechanism explains the brightenings in transition region lines and also the observed surging behavior and jet-like events.
- Publication:
-
The Astrophysical Journal
- Pub Date:
- September 1989
- DOI:
- 10.1086/167870
- Bibcode:
- 1989ApJ...344.1034F
- Keywords:
-
- Line Spectra;
- Solar Activity;
- Solar Maximum Mission;
- Ultraviolet Astronomy;
- Chromosphere;
- Lyman Alpha Radiation;
- Solar Flares;
- Solar Flux;
- Solar Instruments;
- Solar Physics;
- SUN: FLARES;
- SUN: SPECTRA;
- ULTRAVIOLET: SPECTRA