4.7 Article

Probing the radio emission from air showers with polarization measurements

期刊

PHYSICAL REVIEW D
卷 89, 期 5, 页码 -

出版社

AMER PHYSICAL SOC
DOI: 10.1103/PhysRevD.89.052002

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资金

  1. Comision Nacional de Energia Atomica, Fundacion Antorchas, Gobierno De La Provincia de Mendoza, Municipalidad de Malargue, NDM Holdings and Valle Las Le as for their continuing cooperation over land access, Argentina
  2. Australian Research Council
  3. Conselho Nacional de Desenvolvimento Cientifico e Tecnologico (CNPq)
  4. Financiadora de Estudos e Projetos (FINEP)
  5. Fundacao de Amparo a Pesquisa do Estado de Rio de Janeiro (FAPERJ)
  6. Sao Paulo Research Foundation (FAPESP) [2010/07359-6, 1999/054043]
  7. Ministerio de Ciencia e Tecnologia (MCT), Brazil
  8. AVCR [MSMT-CR LG13007, 7AMB12AR013, MSM0021620859, TACR TA01010517]
  9. Czech Republic
  10. Centre de Calcul IN2P3/CNRS
  11. Centre National de la Recherche Scientifique (CNRS)
  12. Conseil Regional Ile-de-France
  13. Departement Physique Nucleaire et Corpusculaire [PNC-IN2P3/CNRS]
  14. Departement Sciences de l'Univers (SDU-INSU/CNRS), France
  15. Bundesministerium fur Bildung und Forschung (BMBF)
  16. Deutsche Forschungsgemeinschaft (DFG)
  17. Finanzministerium Baden-Wurttemberg
  18. Helmholtz-Gemeinschaft Deutscher Forschungszentren (HGF)
  19. Ministerium fur Wissenschaft und Forschung, Nordrhein-Westfalen
  20. Ministerium fur Wissenschaft
  21. Forschung und Kunst
  22. Baden-Wurttemberg, Germany
  23. Istituto Nazionale di Fisica Nucleare (INFN)
  24. Ministero dell'Istruzione
  25. dell'Universita e della Ricerca (MIUR)
  26. Gran Sasso Center for Astroparticle Physics (CFA)
  27. CETEMPS Center of Excellence, Italy
  28. Consejo Nacional de Ciencia y Tecnologia (CONACYT), Mexico
  29. Ministerie van Onderwijs
  30. Cultuur en Wetenschap
  31. Nederlandse Organisatie voor Wetenschappelijk Onderzoek (NWO)
  32. Stichting voor Fundamenteel Onderzoek der Materie (FOM), Netherlands
  33. Ministry of Science and Higher Education [N N202 200239, N N202 207238]
  34. The National Centre for Research and Development Grant, Poland [ERA-NET-ASPERA/02/11]
  35. Portuguese national funds
  36. FEDER funds within COMPETE-Programa Operacional Factores de Competitividade through Fundacao para a Ciencia e a Tecnologia, Portugal
  37. Romanian Authority for Scientific Research ANCS
  38. CNDI-UEFISCDI partnership, Romania [20/2012, 194/2012, 1/ASPERA2/2012 ERA-NET, PN-II-RU-PD-2011-3-0145-17, PN-II-RU-PD-2011-3-0062]
  39. Ministry for Higher Education, Science, and Technology, Slovenian Research Agency, Slovenia
  40. Comunidad de Madrid, FEDER funds
  41. Ministerio de Ciencia e Innovacion and ConsoliderIngenio 2010 (CPAN)
  42. Xunta de Galicia, Spain
  43. The Leverhulme Foundation, Science and Technology Facilities Council, United Kingdom
  44. Department of Energy [DE-AC02-07CH11359, DE-FR02-04ER41300, DE-FG02-99ER41107]
  45. National Science Foundation [0450696]
  46. Grainger Foundation USA
  47. NAFOSTED, Vietnam
  48. Marie Curie-IRSES/EPLANET
  49. European Particle Physics Latin American Network
  50. European Union 7th Framework Program [PIRSES-2009-GA-246806]
  51. UNESCO
  52. Division Of Physics
  53. Direct For Mathematical & Physical Scien [1068696, 1068658] Funding Source: National Science Foundation
  54. Division Of Physics
  55. Direct For Mathematical & Physical Scien [1205845, 1361172] Funding Source: National Science Foundation

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The emission of radio waves from air showers has been attributed to the so-called geomagnetic emission process. At frequencies around 50 MHz this process leads to coherent radiation which can be observed with rather simple setups. The direction of the electric field induced by this emission process depends only on the local magnetic field vector and on the incoming direction of the air shower. We report on measurements of the electric field vector where, in addition to this geomagnetic component, another component has been observed that cannot be described by the geomagnetic emission process. The data provide strong evidence that the other electric field component is polarized radially with respect to the shower axis, in agreement with predictions made by Askaryan who described radio emission from particle showers due to a negative charge excess in the front of the shower. Our results are compared to calculations which include the radiation mechanism induced by this charge-excess process.

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