Spectra of atmospheric waves in the dynamo region of the ionosphere at Kamchatka

Details Spectra of atmospheric waves in the dynamo region of the ionosphere at Kamchatka Spectra of atmospheric waves in the dynamo region of the ionosphere at Kamchatka

Feb 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008ge%26ae..48..117m&link_type=abstract

Geomagnetism and Aeronomy, Volume 48, Issue 1, pp.117-123

Computer Science

1

94.20.Dg, 94.10.Jd, E Region

Scientific paper

A spectral analysis of the diurnal variations in the geomagnetic field horizontal component, observed at Kamchatka and Barrow polar observatory in September-October 1999, has been performed. The complete set of oscillations of thermal tidal atmospheric waves with T = 24, 12, 8, and 4 h has been detected in the variation spectral power ( Sq) at Kamchatka, and only the fundamental harmonic with T = 24 h has been distinguished at Barrow. The above periods vary in both directions relative to stable maximums during strong geomagnetic disturbances. The relative spectral intensity at subharmonics also vary toward the fundamental harmonic with a period of 24 h. In the frequency band 0.5-3 h (IGW periods), the maximal intensity in the background spectra is observed at T ˜ 2 h and increases by an order of magnitude with increasing geomagnetic activity at both Kamchatka and Barrow. A day before earthquakes, the intensity of this maximum is below the rms background values, and the spectra widen toward the region of periods shorter than 2 h. A similar effect was previously observed in the power spectra of the diurnal variations in the quasistatic electric field and VLF noise, simultaneously measured in September-October 1999.

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