Observation of muon intensity variations by season with the MINOS far detector

P. Adamson; C. Andreopoulos; K. E. Arms; R. Armstrong; D. J. Auty; D. S. Ayres; C. Backhouse; J. Barnett; G. Barr; W. L. Barrett; B. R. Becker; M. Bishai; A. Blake; B. Bock; G. J. Bock; D. J. Boehnlein; D. Bogert; C. Bower; S. Cavanaugh; J. D. Chapman; D. Cherdack; S. Childress; B. C. Choudhary; J. H. Cobb; S. J. Coleman; D. Cronin-Hennessy; A. J. Culling; I. Z. Danko; J. K. De Jong; N. E. Devenish; M. V. Diwan; M. Dorman; C. O. Escobar; J. J. Evans; E. Falk; G. J. Feldman; T. H. Fields; M. V. Frohne; H. R. Gallagher; A. Godley; M. C. Goodman; P. Gouffon; R. Gran; E. W. Grashorn; K. Grzelak; A. Habig; D. Harris; P. G. Harris; J. Hartnell; R. Hatcher; K. Heller; A. Himmel; A. Holin; J. Hylen; G. M. Irwin; Z. Isvan; D. E. Jaffe; C. James; D. Jensen; T. Kafka; S. M S Kasahara; G. Koizumi; S. Kopp; M. Kordosky; K. Korman; D. J. Koskinen; Z. Krahn; A. Kreymer; K. Lang; J. Ling; P. J. Litchfield; L. Loiacono; P. Lucas; J. Ma; W. A. Mann; M. L. Marshak; J. S. Marshall; N. Mayer; A. M. McGowan; R. Mehdiyev; J. R. Meier; M. D. Messier; C. J. Metelko; D. G. Michael; W. H. Miller; S. R. Mishra; J. Mitchell; C. D. Moore; J. Morfín; L. Mualem; S. Mufson; J. Musser; D. Naples; J. K. Nelson; H. B. Newman; R. J. Nichol; T. C. Nicholls; J. P. Ochoa-Ricoux; W. P. Oliver; T. Osiecki; R. Ospanov; S. Osprey; J. Paley; R. B. Patterson; T. Patzak; G. Pawloski; G. F. Pearce; E. A. Peterson; R. Pittam; R. K. Plunkett; A. Rahaman; R. A. Rameika; T. M. Raufer; B. Rebel; J. Reichenbacher; P. A. Rodrigues; C. Rosenfeld; H. A. Rubin; V. A. Ryabov; M. C. Sanchez; N. Saoulidou; J. Schneps; P. Schreiner; P. Shanahan; W. Smart; C. Smith; A. Sousa; B. Speakman; P. Stamoulis; M. Strait; N. Tagg; R. L. Talaga; J. Thomas; M. A. Thomson; J. L. Thron; G. Tinti; R. Toner; V. A. Tsarev; G. Tzanakos; J. Urheim; P. Vahle; B. Viren; M. Watabe; A. Weber; R. C. Webb; N. West; C. White; L. Whitehead; S. G. Wojcicki; D. M. Wright; T. Yang; M. Zois; K. Zhang; R. Zwaska

doi:10.1103/PhysRevD.81.012001

Observation of muon intensity variations by season with the MINOS far detector

P. Adamson, C. Andreopoulos, K. E. Arms, R. Armstrong, D. J. Auty, D. S. Ayres, C. Backhouse, J. Barnett, G. Barr, W. L. Barrett, B. R. Becker, M. Bishai, A. Blake, B. Bock, G. J. Bock, D. J. Boehnlein, D. Bogert, C. Bower, S. Cavanaugh, J. D. ChapmanD. Cherdack, S. Childress, B. C. Choudhary, J. H. Cobb, S. J. Coleman, D. Cronin-Hennessy, A. J. Culling, I. Z. Danko, J. K. De Jong, N. E. Devenish, M. V. Diwan, M. Dorman, C. O. Escobar, J. J. Evans, E. Falk, G. J. Feldman, T. H. Fields, M. V. Frohne, H. R. Gallagher, A. Godley, M. C. Goodman, P. Gouffon, R. Gran, E. W. Grashorn, K. Grzelak, A. Habig, D. Harris, P. G. Harris, J. Hartnell, R. Hatcher, K. Heller, A. Himmel, A. Holin, J. Hylen, G. M. Irwin, Z. Isvan, D. E. Jaffe, C. James, D. Jensen, T. Kafka, S. M S Kasahara, G. Koizumi, S. Kopp, M. Kordosky, K. Korman, D. J. Koskinen, Z. Krahn, A. Kreymer, K. Lang, J. Ling, P. J. Litchfield, L. Loiacono, P. Lucas, J. Ma, W. A. Mann, M. L. Marshak, J. S. Marshall, N. Mayer, A. M. McGowan, R. Mehdiyev, J. R. Meier, M. D. Messier, C. J. Metelko, D. G. Michael, W. H. Miller, S. R. Mishra, J. Mitchell, C. D. Moore, J. Morfín, L. Mualem, S. Mufson, J. Musser, D. Naples, J. K. Nelson, H. B. Newman, R. J. Nichol, T. C. Nicholls, J. P. Ochoa-Ricoux, W. P. Oliver, T. Osiecki, R. Ospanov, S. Osprey, J. Paley, R. B. Patterson, T. Patzak, G. Pawloski, G. F. Pearce, E. A. Peterson, R. Pittam, R. K. Plunkett, A. Rahaman, R. A. Rameika, T. M. Raufer, B. Rebel, J. Reichenbacher, P. A. Rodrigues, C. Rosenfeld, H. A. Rubin, V. A. Ryabov, M. C. Sanchez, N. Saoulidou, J. Schneps, P. Schreiner, P. Shanahan, W. Smart, C. Smith, A. Sousa, B. Speakman, P. Stamoulis, M. Strait, N. Tagg, R. L. Talaga, J. Thomas, M. A. Thomson, J. L. Thron, G. Tinti, R. Toner, V. A. Tsarev, G. Tzanakos, J. Urheim, P. Vahle, B. Viren, M. Watabe, A. Weber, R. C. Webb, N. West, C. White, L. Whitehead, S. G. Wojcicki, D. M. Wright, T. Yang, M. Zois, K. Zhang, R. Zwaska

Research output: Contribution to journal › Article › peer-review

Abstract

The temperature of the upper atmosphere affects the height of primary cosmic ray interactions and the production of high-energy cosmic ray muons which can be detected deep underground. The MINOS far detector at Soudan, MN, has collected over 67×106 cosmic ray induced muons. The underground muon rate measured over a period of five years exhibits a 4% peak-to-peak seasonal variation which is highly correlated with the temperature in the upper atmosphere. The coefficient, αT, relating changes in the muon rate to changes in atmospheric temperature was found to be αT=0.873±0. 009(stat)±0.010(syst). Pions and kaons in the primary hadronic interactions of cosmic rays in the atmosphere contribute differently to αT due to the different masses and lifetimes. This allows the measured value of αT to be interpreted as a measurement of the K/π ratio for Ep 7TeV of 0.12-0.05+0.07, consistent with the expectation from collider experiments. © 2010 The American Physical Society.

Original language	English
Article number	012001
Journal	Physical Review D - Particles, Fields, Gravitation and Cosmology
Volume	81
Issue number	1
DOIs	https://doi.org/10.1103/PhysRevD.81.012001
Publication status	Published - 6 Jan 2010

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10.1103/PhysRevD.81.012001

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Adamson, P., Andreopoulos, C., Arms, K. E., Armstrong, R., Auty, D. J., Ayres, D. S., Backhouse, C., Barnett, J., Barr, G., Barrett, W. L., Becker, B. R., Bishai, M., Blake, A., Bock, B., Bock, G. J., Boehnlein, D. J., Bogert, D., Bower, C., Cavanaugh, S., ... Zwaska, R. (2010). Observation of muon intensity variations by season with the MINOS far detector. Physical Review D - Particles, Fields, Gravitation and Cosmology, 81(1), Article 012001. https://doi.org/10.1103/PhysRevD.81.012001

@article{6a399a19bf6e4c9d8f786bfe90d23e33,

title = "Observation of muon intensity variations by season with the MINOS far detector",

abstract = "The temperature of the upper atmosphere affects the height of primary cosmic ray interactions and the production of high-energy cosmic ray muons which can be detected deep underground. The MINOS far detector at Soudan, MN, has collected over 67×106 cosmic ray induced muons. The underground muon rate measured over a period of five years exhibits a 4% peak-to-peak seasonal variation which is highly correlated with the temperature in the upper atmosphere. The coefficient, αT, relating changes in the muon rate to changes in atmospheric temperature was found to be αT=0.873±0. 009(stat)±0.010(syst). Pions and kaons in the primary hadronic interactions of cosmic rays in the atmosphere contribute differently to αT due to the different masses and lifetimes. This allows the measured value of αT to be interpreted as a measurement of the K/π ratio for Ep 7TeV of 0.12-0.05+0.07, consistent with the expectation from collider experiments. {\textcopyright} 2010 The American Physical Society.",

author = "P. Adamson and C. Andreopoulos and Arms, {K. E.} and R. Armstrong and Auty, {D. J.} and Ayres, {D. S.} and C. Backhouse and J. Barnett and G. Barr and Barrett, {W. L.} and Becker, {B. R.} and M. Bishai and A. Blake and B. Bock and Bock, {G. J.} and Boehnlein, {D. J.} and D. Bogert and C. Bower and S. Cavanaugh and Chapman, {J. D.} and D. Cherdack and S. Childress and Choudhary, {B. C.} and Cobb, {J. H.} and Coleman, {S. J.} and D. Cronin-Hennessy and Culling, {A. J.} and Danko, {I. Z.} and {De Jong}, {J. K.} and Devenish, {N. E.} and Diwan, {M. V.} and M. Dorman and Escobar, {C. O.} and Evans, {J. J.} and E. Falk and Feldman, {G. J.} and Fields, {T. H.} and Frohne, {M. V.} and Gallagher, {H. R.} and A. Godley and Goodman, {M. C.} and P. Gouffon and R. Gran and Grashorn, {E. W.} and K. Grzelak and A. Habig and D. Harris and Harris, {P. G.} and J. Hartnell and R. Hatcher and K. Heller and A. Himmel and A. Holin and J. Hylen and Irwin, {G. M.} and Z. Isvan and Jaffe, {D. E.} and C. James and D. Jensen and T. Kafka and Kasahara, {S. M S} and G. Koizumi and S. Kopp and M. Kordosky and K. Korman and Koskinen, {D. J.} and Z. Krahn and A. Kreymer and K. Lang and J. Ling and Litchfield, {P. J.} and L. Loiacono and P. Lucas and J. Ma and Mann, {W. A.} and Marshak, {M. L.} and Marshall, {J. S.} and N. Mayer and McGowan, {A. M.} and R. Mehdiyev and Meier, {J. R.} and Messier, {M. D.} and Metelko, {C. J.} and Michael, {D. G.} and Miller, {W. H.} and Mishra, {S. R.} and J. Mitchell and Moore, {C. D.} and J. Morf{\'i}n and L. Mualem and S. Mufson and J. Musser and D. Naples and Nelson, {J. K.} and Newman, {H. B.} and Nichol, {R. J.} and Nicholls, {T. C.} and Ochoa-Ricoux, {J. P.} and Oliver, {W. P.} and T. Osiecki and R. Ospanov and S. Osprey and J. Paley and Patterson, {R. B.} and T. Patzak and G. Pawloski and Pearce, {G. F.} and Peterson, {E. A.} and R. Pittam and Plunkett, {R. K.} and A. Rahaman and Rameika, {R. A.} and Raufer, {T. M.} and B. Rebel and J. Reichenbacher and Rodrigues, {P. A.} and C. Rosenfeld and Rubin, {H. A.} and Ryabov, {V. A.} and Sanchez, {M. C.} and N. Saoulidou and J. Schneps and P. Schreiner and P. Shanahan and W. Smart and C. Smith and A. Sousa and B. Speakman and P. Stamoulis and M. Strait and N. Tagg and Talaga, {R. L.} and J. Thomas and Thomson, {M. A.} and Thron, {J. L.} and G. Tinti and R. Toner and Tsarev, {V. A.} and G. Tzanakos and J. Urheim and P. Vahle and B. Viren and M. Watabe and A. Weber and Webb, {R. C.} and N. West and C. White and L. Whitehead and Wojcicki, {S. G.} and Wright, {D. M.} and T. Yang and M. Zois and K. Zhang and R. Zwaska",

year = "2010",

month = jan,

day = "6",

doi = "10.1103/PhysRevD.81.012001",

language = "English",

volume = "81",

journal = "Physical Review D - Particles, Fields, Gravitation and Cosmology",

issn = "1550-7998",

publisher = "American Institute of Physics",

number = "1",

}

Adamson, P, Andreopoulos, C, Arms, KE, Armstrong, R, Auty, DJ, Ayres, DS, Backhouse, C, Barnett, J, Barr, G, Barrett, WL, Becker, BR, Bishai, M, Blake, A, Bock, B, Bock, GJ, Boehnlein, DJ, Bogert, D, Bower, C, Cavanaugh, S, Chapman, JD, Cherdack, D, Childress, S, Choudhary, BC, Cobb, JH, Coleman, SJ, Cronin-Hennessy, D, Culling, AJ, Danko, IZ, De Jong, JK, Devenish, NE, Diwan, MV, Dorman, M, Escobar, CO, Evans, JJ, Falk, E, Feldman, GJ, Fields, TH, Frohne, MV, Gallagher, HR, Godley, A, Goodman, MC, Gouffon, P, Gran, R, Grashorn, EW, Grzelak, K, Habig, A, Harris, D, Harris, PG, Hartnell, J, Hatcher, R, Heller, K, Himmel, A, Holin, A, Hylen, J, Irwin, GM, Isvan, Z, Jaffe, DE, James, C, Jensen, D, Kafka, T, Kasahara, SMS, Koizumi, G, Kopp, S, Kordosky, M, Korman, K, Koskinen, DJ, Krahn, Z, Kreymer, A, Lang, K, Ling, J, Litchfield, PJ, Loiacono, L, Lucas, P, Ma, J, Mann, WA, Marshak, ML, Marshall, JS, Mayer, N, McGowan, AM, Mehdiyev, R, Meier, JR, Messier, MD, Metelko, CJ, Michael, DG, Miller, WH, Mishra, SR, Mitchell, J, Moore, CD, Morfín, J, Mualem, L, Mufson, S, Musser, J, Naples, D, Nelson, JK, Newman, HB, Nichol, RJ, Nicholls, TC, Ochoa-Ricoux, JP, Oliver, WP, Osiecki, T, Ospanov, R, Osprey, S, Paley, J, Patterson, RB, Patzak, T, Pawloski, G, Pearce, GF, Peterson, EA, Pittam, R, Plunkett, RK, Rahaman, A, Rameika, RA, Raufer, TM, Rebel, B, Reichenbacher, J, Rodrigues, PA, Rosenfeld, C, Rubin, HA, Ryabov, VA, Sanchez, MC, Saoulidou, N, Schneps, J, Schreiner, P, Shanahan, P, Smart, W, Smith, C, Sousa, A, Speakman, B, Stamoulis, P, Strait, M, Tagg, N, Talaga, RL, Thomas, J, Thomson, MA, Thron, JL, Tinti, G, Toner, R, Tsarev, VA, Tzanakos, G, Urheim, J, Vahle, P, Viren, B, Watabe, M, Weber, A, Webb, RC, West, N, White, C, Whitehead, L, Wojcicki, SG, Wright, DM, Yang, T, Zois, M, Zhang, K & Zwaska, R 2010, 'Observation of muon intensity variations by season with the MINOS far detector', Physical Review D - Particles, Fields, Gravitation and Cosmology, vol. 81, no. 1, 012001. https://doi.org/10.1103/PhysRevD.81.012001

TY - JOUR

T1 - Observation of muon intensity variations by season with the MINOS far detector

AU - Adamson, P.

AU - Andreopoulos, C.

AU - Arms, K. E.

AU - Armstrong, R.

AU - Auty, D. J.

AU - Ayres, D. S.

AU - Backhouse, C.

AU - Barnett, J.

AU - Barr, G.

AU - Barrett, W. L.

AU - Becker, B. R.

AU - Bishai, M.

AU - Blake, A.

AU - Bock, B.

AU - Bock, G. J.

AU - Boehnlein, D. J.

AU - Bogert, D.

AU - Bower, C.

AU - Cavanaugh, S.

AU - Chapman, J. D.

AU - Cherdack, D.

AU - Childress, S.

AU - Choudhary, B. C.

AU - Cobb, J. H.

AU - Coleman, S. J.

AU - Cronin-Hennessy, D.

AU - Culling, A. J.

AU - Danko, I. Z.

AU - De Jong, J. K.

AU - Devenish, N. E.

AU - Diwan, M. V.

AU - Dorman, M.

AU - Escobar, C. O.

AU - Evans, J. J.

AU - Falk, E.

AU - Feldman, G. J.

AU - Fields, T. H.

AU - Frohne, M. V.

AU - Gallagher, H. R.

AU - Godley, A.

AU - Goodman, M. C.

AU - Gouffon, P.

AU - Gran, R.

AU - Grashorn, E. W.

AU - Grzelak, K.

AU - Habig, A.

AU - Harris, D.

AU - Harris, P. G.

AU - Hartnell, J.

AU - Hatcher, R.

AU - Heller, K.

AU - Himmel, A.

AU - Holin, A.

AU - Hylen, J.

AU - Irwin, G. M.

AU - Isvan, Z.

AU - Jaffe, D. E.

AU - James, C.

AU - Jensen, D.

AU - Kafka, T.

AU - Kasahara, S. M S

AU - Koizumi, G.

AU - Kopp, S.

AU - Kordosky, M.

AU - Korman, K.

AU - Koskinen, D. J.

AU - Krahn, Z.

AU - Kreymer, A.

AU - Lang, K.

AU - Ling, J.

AU - Litchfield, P. J.

AU - Loiacono, L.

AU - Lucas, P.

AU - Ma, J.

AU - Mann, W. A.

AU - Marshak, M. L.

AU - Marshall, J. S.

AU - Mayer, N.

AU - McGowan, A. M.

AU - Mehdiyev, R.

AU - Meier, J. R.

AU - Messier, M. D.

AU - Metelko, C. J.

AU - Michael, D. G.

AU - Miller, W. H.

AU - Mishra, S. R.

AU - Mitchell, J.

AU - Moore, C. D.

AU - Morfín, J.

AU - Mualem, L.

AU - Mufson, S.

AU - Musser, J.

AU - Naples, D.

AU - Nelson, J. K.

AU - Newman, H. B.

AU - Nichol, R. J.

AU - Nicholls, T. C.

AU - Ochoa-Ricoux, J. P.

AU - Oliver, W. P.

AU - Osiecki, T.

AU - Ospanov, R.

AU - Osprey, S.

AU - Paley, J.

AU - Patterson, R. B.

AU - Patzak, T.

AU - Pawloski, G.

AU - Pearce, G. F.

AU - Peterson, E. A.

AU - Pittam, R.

AU - Plunkett, R. K.

AU - Rahaman, A.

AU - Rameika, R. A.

AU - Raufer, T. M.

AU - Rebel, B.

AU - Reichenbacher, J.

AU - Rodrigues, P. A.

AU - Rosenfeld, C.

AU - Rubin, H. A.

AU - Ryabov, V. A.

AU - Sanchez, M. C.

AU - Saoulidou, N.

AU - Schneps, J.

AU - Schreiner, P.

AU - Shanahan, P.

AU - Smart, W.

AU - Smith, C.

AU - Sousa, A.

AU - Speakman, B.

AU - Stamoulis, P.

AU - Strait, M.

AU - Tagg, N.

AU - Talaga, R. L.

AU - Thomas, J.

AU - Thomson, M. A.

AU - Thron, J. L.

AU - Tinti, G.

AU - Toner, R.

AU - Tsarev, V. A.

AU - Tzanakos, G.

AU - Urheim, J.

AU - Vahle, P.

AU - Viren, B.

AU - Watabe, M.

AU - Weber, A.

AU - Webb, R. C.

AU - West, N.

AU - White, C.

AU - Whitehead, L.

AU - Wojcicki, S. G.

AU - Wright, D. M.

AU - Yang, T.

AU - Zois, M.

AU - Zhang, K.

AU - Zwaska, R.

PY - 2010/1/6

Y1 - 2010/1/6

N2 - The temperature of the upper atmosphere affects the height of primary cosmic ray interactions and the production of high-energy cosmic ray muons which can be detected deep underground. The MINOS far detector at Soudan, MN, has collected over 67×106 cosmic ray induced muons. The underground muon rate measured over a period of five years exhibits a 4% peak-to-peak seasonal variation which is highly correlated with the temperature in the upper atmosphere. The coefficient, αT, relating changes in the muon rate to changes in atmospheric temperature was found to be αT=0.873±0. 009(stat)±0.010(syst). Pions and kaons in the primary hadronic interactions of cosmic rays in the atmosphere contribute differently to αT due to the different masses and lifetimes. This allows the measured value of αT to be interpreted as a measurement of the K/π ratio for Ep 7TeV of 0.12-0.05+0.07, consistent with the expectation from collider experiments. © 2010 The American Physical Society.

AB - The temperature of the upper atmosphere affects the height of primary cosmic ray interactions and the production of high-energy cosmic ray muons which can be detected deep underground. The MINOS far detector at Soudan, MN, has collected over 67×106 cosmic ray induced muons. The underground muon rate measured over a period of five years exhibits a 4% peak-to-peak seasonal variation which is highly correlated with the temperature in the upper atmosphere. The coefficient, αT, relating changes in the muon rate to changes in atmospheric temperature was found to be αT=0.873±0. 009(stat)±0.010(syst). Pions and kaons in the primary hadronic interactions of cosmic rays in the atmosphere contribute differently to αT due to the different masses and lifetimes. This allows the measured value of αT to be interpreted as a measurement of the K/π ratio for Ep 7TeV of 0.12-0.05+0.07, consistent with the expectation from collider experiments. © 2010 The American Physical Society.

U2 - 10.1103/PhysRevD.81.012001

DO - 10.1103/PhysRevD.81.012001

M3 - Article

SN - 1550-7998

VL - 81

JO - Physical Review D - Particles, Fields, Gravitation and Cosmology

JF - Physical Review D - Particles, Fields, Gravitation and Cosmology

IS - 1

M1 - 012001

ER -

Observation of muon intensity variations by season with the MINOS far detector

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