Visualization of ULF waves in SuperDARN data

  • Pavlo V. Ponomarenko
    School of Mathematical and Physical Sciences University of Newcastle NSW Australia
  • Frederick W. Menk
    School of Mathematical and Physical Sciences University of Newcastle NSW Australia
  • Colin L. Waters
    School of Mathematical and Physical Sciences University of Newcastle NSW Australia

書誌事項

公開日
2003-09
権利情報
  • http://onlinelibrary.wiley.com/termsAndConditions#vor
DOI
  • 10.1029/2003gl017757
公開者
American Geophysical Union (AGU)

この論文をさがす

説明

<jats:p>Measurements of ionospheric <jats:bold>E</jats:bold> × <jats:bold>B</jats:bold> drifts obtained with HF radars from the SuperDARN (Super Dual Auroral Radar) Network sometimes show signatures of ULF (few mHz) waves. We present a new data display technique that facilitates the detection of ULF waves in both ground and sea scatter returns. Statistical study of high time resolution data from the SuperDARN TIGER radar in Tasmania, Australia, revealed that ULF wave signatures occur on an everyday basis with ground scatter accounting for about 60% of wave events. About half of these events exhibit high coherence across large spatial distances and are associated with ULF pulsations recorded by a ground magnetometer. These results show that SuperDARN radars may be used to routinely monitor ULF waves in the high‐latitude ionosphere.</jats:p>

収録刊行物

被引用文献 (4)*注記

もっと見る

問題の指摘

ページトップへ