4.6 Article

The effect of the geomagnetic field on cosmic ray energy estimates and large scale anisotropy searches on data from the Pierre Auger Observatory

Journal

Publisher

IOP Publishing Ltd
DOI: 10.1088/1475-7516/2011/11/022

Keywords

ultra high energy cosmic rays; cosmic ray experiments; cosmic rays detectors

Funding

  1. Comision Nacional de Energia Atomica
  2. Fundacion Antorchas
  3. Gobierno De La Provincia de Mendoza
  4. Municipalidad de Malargue
  5. NDM Holdings
  6. Valle Las Lenas
  7. Australian Research Council
  8. Conselho Nacional de Desenvolvimento Cientifico e Tecnologico (CNPq)
  9. Financiadora de Estudos e Projetos (FINEP)
  10. Fundacao de Amparo a Pesquisa do Estado de Rio de Janeiro (FAPERJ)
  11. Fundacao de Amparo a Pesquisa do Estado de Sao Paulo (FAPESP)
  12. Ministerio de Ciencia e Tecnologia (MCT), Brazil
  13. AVCR [AV0Z10.100502, AV0Z10100522, GAAV KJB100100904, MSMT-CR LA08016, LC527, 1M06002, MSN10021620859]
  14. Czech Republic
  15. Centre de Calcul [IN2P3/CNRS]
  16. Centre National de la Recherche
  17. Scientifique (CNRS)
  18. Conseil Regional Ile-de-France
  19. Departement Physique Nucleaire et Corpusculaire [PNC-IN2P3/CNRS]
  20. Departement Sciences de l'Univers (SDU-INSU/CNR.S), France
  21. Bundesministerium far Bildung mid Forschung (BMBF)
  22. Deutsche Forschungsgenteinschaft (DFG)
  23. Finanzministerium Baden-Wurttemberg
  24. Helmholtz-Gemeinschaft Deutscher Forschungszentren (HGF)
  25. Ministerium fur Wissenschaft und Forschung
  26. Nordrhein-Westfalen
  27. Forschung und Kunst, Liaden-Wurttemberg, Germany
  28. Istituto Nazionale di Fisica Nucleate Ministero dell'Istruzione, dell'Universita e della Ricerca (MIUR), Italy
  29. Consejo Nacional de Ciencia y Tecnologia (CONACYT), Mexico
  30. Ministerie van Onderwijs, Cultuur en Wetenschap, Nederlandse Organisatie voor \\Tetenschappelijk Onderzoek (NNVO), Stichting voor Rindamenteel Onderzoelc der Materie (FOM), Netherlands
  31. Ministry of Science and Higher Education, Poland [N N202 200239, N N202 207238]
  32. Fundacao para a Ciencia e a 'Tecnologia, Portugal
  33. Ministry for Higher Education, Science, and Technology, Slovenian Research Agency, Slovenia
  34. Comunidad de Madrid, Consejerfa de Educacion de la Comunidad de Castilla La Mancha
  35. FEDER
  36. Ministerio de Ciencia e Innovacion
  37. CPAN
  38. Xunta de Galicia, Spain
  39. Science and Technology Facilities Council, United Kingdom
  40. Department of Energy [DE-AC02-07CH11359, DE-FR02-04ER41300]
  41. National Science Foundation [0450696]
  42. Grainger Foundation USA
  43. ALFA-EC / HELEN
  44. European Union [MEIF-CT-2005-025057, PIEF-GA-2008-220240]
  45. UNESCO
  46. STFC [ST/J000507/1] Funding Source: UKRI
  47. Science and Technology Facilities Council [ST/J000507/1] Funding Source: researchfish
  48. Direct For Mathematical & Physical Scien
  49. Division Of Physics [1068210, 1068696] Funding Source: National Science Foundation

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We present a comprehensive study of the influence of the geomagnetic field on the energy estimation of extensive air showers with a zenith angle smaller than 60 degrees, detected at the Pierre Auger Observatory. the geomagnetic field induces an azimuthal modulation of the estimated energy of cosmic rays up to the similar to 2% level at large zenith angles. We present a method to account for this modulation of the reconstructed energy. We analyse the effect of the modulation on large scale anisotropy searches in the arrival direction distributions of cosmic rays. At a given energy, the geomagnetic effect is shown to induce a pseudo-dipolar pattern at the percent level in the declination distribution that needs to be accounted for.

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