Abstract
Results are presented for a simulation carried out to test the precision with which a detector design (HERON) based on a superfluid helium target material should be able to measure the solar pp and 7Be fluxes. It is found that precisions of ±1.68% and ±2.97% for pp and 7Be fluxes, respectively, should be achievable in a 5-year data sample. The physics motivation to aim for these precisions is outlined as are the detector design, the methods used in the simulation and sensitivity to solar orbit eccentricity.
Original language | English |
---|---|
Pages (from-to) | 1-11 |
Number of pages | 11 |
Journal | Astroparticle Physics |
Volume | 30 |
Issue number | 1 |
DOIs | |
State | Published - Aug 2008 |
Funding
We are grateful to the US Department of Energy for support of R&D on this project through grant DE-FG02-8840452. We are indebted to J.R. Klein for his close reading and valuable suggestions, R.B. Vogelaar for comments and A.W. Poon for assistance in providing additional computing resources at Lawrence Berkeley National Laboratory.