Statistical study of nighttime medium‐scale traveling ionospheric disturbances using midlatitude airglow images

  • K. Shiokawa
    Solar‐Terrestrial Environment Laboratory Nagoya University Toyokawa Japan
  • C. Ihara
    Solar‐Terrestrial Environment Laboratory Nagoya University Toyokawa Japan
  • Y. Otsuka
    Solar‐Terrestrial Environment Laboratory Nagoya University Toyokawa Japan
  • T. Ogawa
    Solar‐Terrestrial Environment Laboratory Nagoya University Toyokawa Japan

書誌事項

公開日
2003-01
権利情報
  • http://onlinelibrary.wiley.com/termsAndConditions#vor
DOI
  • 10.1029/2002ja009491
公開者
American Geophysical Union (AGU)

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説明

<jats:p>We have investigated statistical characteristics of the nighttime medium‐scale traveling ionospheric disturbances (MSTIDs) observed in 630‐nm airglow images at two stations, Rikubetsu (43.5°N, 34.8°MLAT) and Shigaraki (34.9°N, 25.4°MLAT), in Japan for 1998–2000 near the solar maximum period. Most of the observed MSTIDs propagate southwestward in the images. The typical wavelength, velocity, period, and amplitude are 100–300 km, 50–100 m/s, 0.5–1.5 h, and 5–15%, respectively. Seasonal variations in these parameters are not clear. The occurrence rate has a major peak (50–60%) in summer that appears ∼2 months earlier at lower latitudes and a minor peak in winter. Similar occurrence characteristics are obtained from midlatitude spread‐<jats:italic>F</jats:italic> signatures using multipoint ionosonde data in Japan, though the coincidence of the spread‐<jats:italic>F</jats:italic> and the MSTIDs in airglow images is only 10–15%.</jats:p>

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