Solar control of winter mesospheric echo occurrence at Poker Flat, Alaska

Details Solar control of winter mesospheric echo occurrence at Poker Flat, Alaska Solar control of winter mesospheric echo occurrence at Poker Flat, Alaska

Dec 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983maph....9..145e&link_type=abstract

In International Council of Scientific Unions Middle Atmosphere Program, Vol. 9 p 145-146 (SEE N84-27076 17-42)

Computer Science

Auroras, Mesosphere, Periodic Variations, Radar Echoes, Radar Signatures, Signature Analysis, Decay, Graphs (Charts), Solar Cycles, Solar Position, Sunrise, Sunset

Scientific paper

Winter mesospheric echoes are observed between about 55 and 80 km when auroral absorption is present during daylight hours. Relatively steady auroral absorption during sunrise and sunset periods causes a distinct onset and decay signature in mesospheric echo occurrence. The echo onset and disappearance time are shown versus height by the inclined lines for four different dates. The more vertical lines give the visible sunlight height/time curves for both sunrise (SR) and sunset (SS). The data is combined and replotted to give the morning onset height and the afternoon disappearance height as a function of solar zenith angle. Echoes are not observed at the lowest heights in the morning until the solar zenith angle is less than 90 deg. The afternoon echoes at the lowest heights also start to disappear as soon as the solar zenith angle exceeds 90 deg, implying that the solar component which sustains the mesospheric echo is screened by a layer extending up to about 60 km. The morning echo at 73 km onsets near the time of visible sunrise, but in the afternoon the 73 km echo lasts well past visible sunset.

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