Solar Flare Onset
Solar Physicist
To determine the conditions that lead to the onset of a solar flare.
Imaging time series data in optical, UV, EUV, SXR and HXR.
Co-spatial and temporal magnetograms and spectroscopic observations.
In order to understand the flare trigger we need observations that precede the actual onset that provide high spatial, temporal and spectral resolution information on the pre-flare plasma. The data needs to be co-spatial, although the FOV may be different, so that relationships between different temperatures and the underlying magnetic field can be determined using overlays.
Gaining a fuller understanding of what triggers a flare will enable suitable flare activity warnings to be given - e.g. to Space Missions -
Japan's Mars probe was recently damaged by a strong solar flare (Newscientist, 27 May 2002).
The current solution is to either try for a co-ordinated campaign of sit-and-stare observations on an active region or to trawl through data to find coincident datasets. Often a good data-set in one wavelength band will have no accompanying data in other ranges, or coincident magnetograms.
To identify flares after occurrence from a flare list and be able to determine which of them have pre-flare coverage of the required type eg. imaging time series at high time resolution in a number of wavelengths, time series of magnetograms, times series of
spectroscopic observations.
Discussion:
type here
type here
GoodStyle: Please add comments below. This area should be used for refinement of the above document. If you want to ask questions or start a dialogue with the author, please use (or create) a topic in the
Science Problems Forum. For other
ScienceProblems, refer to the
ScienceProblemList.
Author: Once the refinements here and comments in the forum die down, perhaps you could rewrite the problem, incorporating the comments and refinements.
--
SarahMatthews - 25 Apr 2002