There are 89 project descriptions currently viewable.

Search:
Search Hints
Options
About Add New Description Order By
Submitter
Help/FAQ View Email List Email Archive
Add Email Address
Comparison of Hard X-ray Source Structure as a Function of Energy View all project descriptions by submitter

Gordon Emslie Submitted: 26-Sep-2002 04:39

As a prelude to high-spatial-resolution imaging spectroscopy and empirical derivation of electron energy loss processes ("do the easy science first, Gordon" - G. Hurford), I'm looking at the structure of hard X-ray sources in different energy bands, to see what similarities/differences there are. For example, in the July 23 event, the source structure changes from principally coronal to principally chromospheric over a quite narrow range of energies around 30 keV. The implications of this for electron acceleration and propagation mechanisms are being considered.

Participants: Gordon Emslie, Eduard Kontar, John Brown

Project Status: images made, analyzing movies and light curves in different regions Go to main RHESSI project descriptions page  Hard X-Ray Polarimetry of Solar Flares  Edit Entry 

Key
Go to main RHESSI project descriptions pageGoto main RHESSI project descriptions page.
Previous Project DescriptionPrevious Project Description.
Next Project DescriptionNext Project Description.
Submitter's HomepageSubmitters Homepage.
Edit EntryEdit Entry.
View All Project Descriptions By SubmitterView all project descriptions by submitter.
Maintained by
Alisdair Davey

Latest Entries

Related Pages
MSU Solar Physics.
Max Millennium Science Mail Archive.
Max Millennium Messge of the Day Mail Archive.
Max Millennium Flare Catalog



© Solar Physics Group - Montana State University