Physics
Scientific paper
Aug 2005
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005spie.5901...25g&link_type=abstract
Solar Physics and Space Weather Instrumentation. Edited by Fineschi, Silvano; Viereck, Rodney A. Proceedings of the SPIE, Volume
Physics
Scientific paper
The glow of interstellar plasma and solar wind pickup ions and solar wind emissions at 30.4 nm provide a way of exploring important physical processes in the heliosphere. Imaging the heliosphere at this wavelength with high spectral resolution will map the heliopause, probe pickup ions in the solar wind, and reveal the three-dimensional flow pattern of the solar wind, including in the regions over the sun's poles. The required high-throughput, high-resolution spectrometer for diffuse radiation should be able to measure 1 milli-Rayleigh irradiance in 10000 seconds with a 0.005-nm spectral resolution across pixels subtending a few degrees of celestial arc. The desired performance characteristics can be achieved by combining multiple entrance slits with an optimized spectrometer design. We present a concept of a space experiment to image the heliosphere at 30.4 nm and discuss the scientific rationale and required instrumentation.
Edelstein Jerry
Gruntman Mike
Lampton Mike
No associations
LandOfFree
Imaging three-dimensional heliosphere in EUV 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 three-dimensional heliosphere in EUV, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Imaging three-dimensional heliosphere in EUV will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-801642