Speaker
Alec Habig
(University of Minnesota Duluth)
Description
The MINOS and NOvA long baseline neutrino experiments have near detectors 100m underground at Fermilab and far detectors in Minnesota 700m underground (MINOS) and on the surface with minimal overburden (NOvA). They are large highly segmented scintillator detectors like MACRO for good cosmic ray tracking and timing, and have followed up on MACRO measurements of the cosmic ray seasonal variations and moon and sun shadows. Addtionally, the NOvA far detector would be sensitive to supernova neutrinos and magnetic monopoles amongst all those cosmics, continuing all the letters in MACRO.
