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Low Frequency Radio Signals from Giant Air Showers

Research Project

Project/Area Number 02452023
Research Category

Grant-in-Aid for General Scientific Research (B)

Allocation TypeSingle-year Grants
Research Field 核・宇宙線・素粒子
Research InstitutionTokyo Institute of Technology

Principal Investigator

KAKIMOTO Fumio  Tokyo Institute of Technology, Department of Physics, Assistant Professor, 理学部, 助教授 (00092544)

Co-Investigator(Kenkyū-buntansha) MATSUBARA Yutaka  Nagoya University, STE Laboratory, Assistant Professor, 理学部(助手) 現名古屋大学・太陽・地球環境研究所, 助教授 (80202323)
Project Period (FY) 1990 – 1991
Project Status Completed (Fiscal Year 1991)
Budget Amount *help
¥7,000,000 (Direct Cost: ¥7,000,000)
Fiscal Year 1991: ¥300,000 (Direct Cost: ¥300,000)
Fiscal Year 1990: ¥6,700,000 (Direct Cost: ¥6,700,000)
Keywordsthe most energetic cosmic rays / air showers / a new technique / radio signals with low frequencies / 超高エネルギ-宇宙線 / 空気シャワ-
Research Abstract

We have observed radio signals associated with large air showers. For showers with primary energies of 10^<19>eV, radio signals can be observed at core distances within about 5km. Negative unipolar signals are mainly observed, while positive unipolar and bipolar signals are also obtained with rather low frequency and their pulse widths distribute from 1 to 5mus. We made a calculation with a new emission model in which radio signals are emitted due to deacceleration of negative charge excess electrons with a process of ionization loss and by the effect of the atmospheric electric field. The excess of negative charge electrons is significant at lower energies than several MeV. Then we have assumed that negative charge excess electrons have energies of 1MeV and are deaccelerated during passing through the atmosphere with thickness of 1g/cm^2. Even though primary cosmic rays have the same energies, calculated field intensities at same R depend on zenith angles(theta) of arrival directions and phi and are much consistent with observed intensities The distribution are also consistent with this model, since a shower with phi of 180 degrees gives the largest field intensities among showers with the same primary energies and theta of arrival direction. Furthermore, this model predicts positive and negative unipolar and bipolar signals according to R, theta and phi. This result is also consistent with observed results. However calculated pulse widths are smaller than those of observed signals by about three times. Some parts of this difference can be explained if we take into account of pulse deformation due to time response of the system and the employed method in the analysis. Our calculation shows that arrival directions and primary energies(E) of cosmic rays with energies above 10^<20>eV can be measured within an accuracy of 3 degrees and 0.1 in log(E) respectively.

Report

(3 results)
  • 1991 Annual Research Report   Final Research Report Summary
  • 1990 Annual Research Report
  • Research Products

    (14 results)

All Other

All Publications (14 results)

  • [Publications] F.Kakimoto et al.: "LF-MF Signals from Large Air Showers" Proceedings of 21st.International Cosmic Ray Conference. 9. 213-216 (1990)

    • Description
      「研究成果報告書概要(和文)」より
    • Related Report
      1991 Final Research Report Summary
  • [Publications] 垣本 史雄: "超大AS,MF,LF,VLF電磁パルス観測" 東京大学宇宙線研究所共同利用報告集. 56-61 (1990)

    • Description
      「研究成果報告書概要(和文)」より
    • Related Report
      1991 Final Research Report Summary
  • [Publications] Y.Matsubara et al.: "LF-MF Radio Signals From Large Air Showers" Astrophysical Aspects of the Most Energetic Cosmic Rays(published by World Scientific Co.). 366-372 (1991)

    • Description
      「研究成果報告書概要(和文)」より
    • Related Report
      1991 Final Research Report Summary
  • [Publications] 垣本 史雄: "超大AS,MF,LF,VLF電磁パルス観測" 東京大学宇宙線研究所共同利用報告集. 10-13 (1991)

    • Description
      「研究成果報告書概要(和文)」より
    • Related Report
      1991 Final Research Report Summary
  • [Publications] 垣本 史雄: "超大AS,MF,LF,VLF電磁パルス観測" 東京大学宇宙線研究所共同利用報告集. 8-11 (1992)

    • Description
      「研究成果報告書概要(和文)」より
    • Related Report
      1991 Final Research Report Summary
  • [Publications] F.Kakimoto et al.: "LM-MF Radio Signals from Large Air Showers" Proceedings of 23rd.International Cosmic Ray Conference. (1993)

    • Description
      「研究成果報告書概要(和文)」より
    • Related Report
      1991 Final Research Report Summary
  • [Publications] Fumio Kakimoto et al.: "LF-MF Signals from Large Air Showers" Proceedings of 21st. International Cosmic Ray Conference. 9. 213-216 (1990)

    • Description
      「研究成果報告書概要(欧文)」より
    • Related Report
      1991 Final Research Report Summary
  • [Publications] Fumio Kakimoto: "Observation of MF,LF,VLF Radio Signals from Large Air Showers" ICRR Report. ICRR-82-90-3. 56-61 (1990)

    • Description
      「研究成果報告書概要(欧文)」より
    • Related Report
      1991 Final Research Report Summary
  • [Publications] Yutaka Matsubara et al.: "LF-MF Radio Signals from Large Air Showers" Astrophysical Aspects of the Most Energetic Cosmic Rays (published by World Scientific Co.). 366-372 (1991)

    • Description
      「研究成果報告書概要(欧文)」より
    • Related Report
      1991 Final Research Report Summary
  • [Publications] Fumio Kakimoto: "Observation of MF,LF,VLF Radio Signals from Large Air Showers" ICRR Report. ICRR-93-91-4. 10-13 (1991)

    • Description
      「研究成果報告書概要(欧文)」より
    • Related Report
      1991 Final Research Report Summary
  • [Publications] Fumio Kakimoto: "Observation of MF,LF,VLF Radio Signals from Large Air Showers" ICRR Report. ICRR-99-92-2. 8-11 (1992)

    • Description
      「研究成果報告書概要(欧文)」より
    • Related Report
      1991 Final Research Report Summary
  • [Publications] Fumio Kakimoto et al.: "LF-MF Radio Signals from Large Air Showers" Proceedings of 23rd. International Cosmic Ray Conference.

    • Description
      「研究成果報告書概要(欧文)」より
    • Related Report
      1991 Final Research Report Summary
  • [Publications] Y.Matsubara,T.Umezawa,F.Kakimoto and K.Nishi: "LFーMF Radio Signals from Large Air Showers" Proceedings of the ICRR International Symposium. 1. 366-372 (1991)

    • Related Report
      1991 Annual Research Report
  • [Publications] F.Kakimoto,T.Umezawa,T.Nishiyama,and K.Nishi: "LFーMF Signals from Large Air Showers" Proceedings of 21st International Cosmic Ray Conference. 9. 213-217 (1990)

    • Related Report
      1990 Annual Research Report

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Published: 1990-04-01   Modified: 2016-04-21  

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