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First observation of rising-tone magnetosonic waves

Fu, H. S. (author)
Cao, J. B. (author)
Zhima, Z. (author)
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Khotyaintsev, Yuri V. (author)
Uppsala universitet,Institutet för rymdfysik, Uppsalaavdelningen
Angelopoulos, V. (author)
Santolik, O. (author)
Omura, Y. (author)
Taubenschuss, Ulrich (author)
Uppsala universitet,Institutet för rymdfysik, Uppsalaavdelningen
Chen, L. (author)
Huang, S. Y. (author)
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 (creator_code:org_t)
2014
2014
English.
In: Geophysical Research Letters. - 0094-8276 .- 1944-8007. ; 41:21, s. 7419-7426
  • Journal article (peer-reviewed)
Abstract Subject headings
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  • Magnetosonic (MS) waves are linearly polarized emissions confined near the magnetic equator with wave normal angle near 90 degrees and frequency below the lower hybrid frequency. Such waves, also termed equatorial noise, were traditionally known to be "temporally continuous" in their time-frequency spectrogram. Here we show for the first time that MS waves actually have discrete wave elements with rising-tone features in their spectrogram. The frequency sweep rate of MS waves, similar to 1 Hz/s, is between that of chorus and electromagnetic ion cyclotron (EMIC) waves. For the two events we analyzed, MS waves occur outside the plasmapause and cannot penetrate into the plasmasphere; their power is smaller than that of chorus. We suggest that the rising-tone feature of MS waves is a consequence of nonlinear wave-particle interaction, as is the case with chorus and EMIC waves.

Subject headings

NATURVETENSKAP  -- Geovetenskap och miljövetenskap -- Geologi (hsv//swe)
NATURAL SCIENCES  -- Earth and Related Environmental Sciences -- Geology (hsv//eng)

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