• DocumentCode
    1099765
  • Title

    Effects of Sun Spots and Terrestrial Magnetism on Long-Distance Reception of Low-Frequency Waves

  • Author

    Yokoyama, Eitaro ; Nakai, Tomozo

  • Author_Institution
    Electrotechnical Laboratory, Ministry of Communications, Tokyo, Japan
  • Volume
    19
  • Issue
    5
  • fYear
    1931
  • fDate
    5/1/1931 12:00:00 AM
  • Firstpage
    882
  • Lastpage
    890
  • Abstract
    Daily average variations of sun spots and field intensity are not simply related. What mostly occurs are the effects which vary as the period of the sun´s rotation and one-half thereof. Phase relations are generally found in about 180 degrees and 90 degrees. There is no indication of different effects between daylight and darkness waves. The relation between their monthly average variations is, in general, not obvious. However, direct relation is observed on some stations in summer, whereas inverse relation is noted in winter in several cases, the relation being less clear in the latter season. Daily average variations of terrestrial magnetism and field intensity are also not simply related. However, field intensity usually reaches its maximum from two to four days before the day of occurrence of magnetic disturbance and then gradually decreases until it reaches its minimum from two to four days after that day. There is also no indication of different effects between daylight and darkness waves. The relation is not clearly found for monthly average variations.
  • Keywords
    Atmospheric waves; Frequency measurement; Laboratories; Magnetic field measurement; Magnetic separation; Solar radiation; Storms; Sun; Temperature; Time series analysis;
  • fLanguage
    English
  • Journal_Title
    Radio Engineers, Proceedings of the Institute of
  • Publisher
    ieee
  • ISSN
    0731-5996
  • Type

    jour

  • DOI
    10.1109/JRPROC.1931.222396
  • Filename
    1670989