Imaging solar flares in hard X-rays and gamma raysfrom balloon-borne platforms

Details Imaging solar flares in hard X-rays and gamma raysfrom balloon-borne platforms Imaging solar flares in hard X-rays and gamma raysfrom balloon-borne platforms

Nov 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988fnsm.work..164c&link_type=abstract

In its Max 1991: Flare Research at the Next Solar Maximum. Workshop 1: Scientific Objectives p 164-176 (SEE N89-15854 07-92)

Physics

Balloon-Borne Instruments, Fourier Transformation, Gamma Rays, Imaging Techniques, Solar Flares, X Rays, Angular Resolution, Field Of View, Solar Maximum Mission, Temporal Resolution

Scientific paper

Hard X-rays and gamma rays carry the most direct evidence available for the roles of accelerated particles in solar flares. An approach that employs a spatial Fourier-transform technique for imaging the sources of these emissions is described and plans for developing a balloon-borne gamma ray imaging device (GRID) based on this instrumental approach is presented. This instrument, GRID on a balloon, would enable observations with a 1.6 arcsecond angular resolution, 10 millisecond time resolution, and whole-Sun field of view on long-duration balloon flights during MAX 1991.

Affiliated with

Also associated with

No associations

Rating

Imaging solar flares in hard X-rays and gamma raysfrom balloon-borne platforms does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Imaging solar flares in hard X-rays and gamma raysfrom balloon-borne platforms, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Imaging solar flares in hard X-rays and gamma raysfrom balloon-borne platforms will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1826002