HAWC observations from 2016 to 2018 show the 10-200 TeV cosmic-ray Sun Shadow shrinking during the solar cycle 24 decline, with a linear dependence on the median photospheric magnetic field below 8 G.
U., and 104 colleagues 2014.\ Sensitivity of HAWC to high-mass dark matter annihilations.\ Physical Review D 190 , 122002
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Galactic Cosmic Ray Sun Shadow during the declining phase of cycle 24 observed by HAWC
HAWC observations from 2016 to 2018 show the 10-200 TeV cosmic-ray Sun Shadow shrinking during the solar cycle 24 decline, with a linear dependence on the median photospheric magnetic field below 8 G.