Overlooked astrophysical signatures of axion(-like) particles
Overlooked astrophysical signatures of axion(-like) particles
Overlooked astrophysical signatures of axion(-like) particles
You also want an ePaper? Increase the reach of your titles
YUMPU automatically turns print PDFs into web optimized ePapers that Google loves.
Quiet-Sun X-ray observationsRHESSITopic Feasibility Importance (1-10)Micr<strong>of</strong>lares 10 1 (program calibration)Corona itself 1 3 (nonthermal tail?)CRAND halo 1 3 (physics is important)Diffuse background 1 2 (known source)Axions 1 10 (fundamental physics)General 10 2 ( get limits)http://sprg.ssl.berkeley.edu/~hhudson/presentations/ What to do during solar minimum? (Mar. 8, 2006)“…to determine the X-ray spectrumray spectrum <strong>of</strong> thenon-flaring, spotless, active-region-free Sun, i.e. the quiet Sun quiet Sun.”Hannah, I.G., Hurford, G.J, Hudson H.S, Lin, R.P, RHESSI:http://solar.physics.montana.edu/rhessi/projects/full_abstract.pl?entry=335
Change language