Adamson, P.Andreopoulos, C.Ayres, D.S.Backhouse, C.Barr, G.Barrett, W.L.Bishai, M.Blake, A.Bock, B.Bock, G.J.Boehnlein, D.J.Bogert, D.Bower, C.Budd, S.Cavanaugh, S.Cherdack, D.Childress, S.Choudhary, B.C.Cobb, J.H.Coelho, J.A.B.Coleman, S.J.Corwin, L.Cronin-Hennessy, D.Danko, I.Z.de Jong, J.K.Devenish, N.E.Diwan, M.V.Dorman, M.Escobar, C.O.Evans, J.J.Falk, E.Feldman, GaryFrohne, M.V.Gallagher, H.R.Godley, A.Gomes, R.A.Goodman, M.C.Gouffon, P.Gran, R.Grant, N.Grashorn, E.W.Grzelak, K.Habig, A.Harris, D.Harris, P.G.Hartnell, J.Hatcher, R.Himmel, A.Holin, A.Huang, X.Hylen, J.Ilic, J.Irwin, G.M.Isvan, Z.Jaffe, D.E.James, C.Jensen, D.Kafka, T.Kasahara, S.M.S.Koizumi, G.Kopp, S.Kordosky, M.Krahn, Z.Kreymer, A.Lang, K.Lefeuvre, G.Ling, J.Litchfield, P.J.Litchfield, R.P.Loiacono, L.Lucas, P.Mann, W.A.Marshak, M.L.Marshall, J.S.Mayer, N.McGowan, A.M.Mehdiyev, R.Meier, J.R.Messier, M.D.Michael, D.G.Miller, W.H.Mishra, S.R.Mitchell, J.Moore, C.D.Mualem, L.Mufson, S.Musser, J.Naples, D.Nelson, J.K.Newman, H.B.Nichol, R.J.Nicholls, T.C.Oliver, W.P.Orchanian, M.Paley, J.Patterson, R.B.Pawloski, G.Pearce, G.F.Peterson, E.A.Pittam, R.Plunkett, R.K.Ratchford, J.Raufer, T.M.Rebel, B.Reichenbacher, J.Rodrigues, P.A.Rosenfeld, C.Rubin, H.A.Ryabov, V.A.Sanchez, M.C.Schneps, J.Schreiner, P.Semenov, V.K.Shanahan, P.Sousa, A.Strait, M.Tagg, N.Talaga, R.L.Thomas, J.Thomson, M.A.Thron, J.L.Tinti, G.Toner, R.Tzanakos, G.Urheim, J.Vahle, P.Viren, B.Weber, A.Webb, R.C.White, C.Whitehead, L.Wojcicki, S.G.Wright, D.M.Yang, T.Zwaska, R.2016-09-132011Adamson, P., C. Andreopoulos, D.S. Ayres, C. Backhouse, G. Barr, W.L. Barrett, M. Bishai, et al. 2011. “Observation in the MINOS Far Detector of the Shadowing of Cosmic Rays by the Sun and Moon.” Astroparticle Physics 34 (6) (January): 457–466. doi:10.1016/j.astropartphys.2010.10.010.0927-6505http://nrs.harvard.edu/urn-3:HUL.InstRepos:28449881The shadowing of cosmic ray primaries by the moon and sun was observed by the MINOS far detector at a depth of 2070 mwe using 83.54 million cosmic ray muons accumulated over 1857.91 live-days. The shadow of the moon was detected at the 5.6 σ level and the shadow of the sun at the 3.8 σ level using a log-likelihood search in celestial coordinates. The moon shadow was used to quantify the absolute astrophysical pointing of the detector to be 0.17 ± 0.12°. Hints of interplanetary magnetic field effects were observed in both the sun and moon shadowen-USCosmic raysMoon shadowSun shadowMuonsInterplanetary magnetic fieldJournal Article2016-09-1310.1016/j.astropartphys.2010.10.010