The causes of mid-latitude F layer behavior

Details The causes of mid-latitude F layer behavior The causes of mid-latitude F layer behavior

Aug 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008jgra..11308310o&link_type=abstract

Journal of Geophysical Research, Volume 113, Issue A8, CiteID A08310

Other

10

Ionosphere: Midlatitude Ionosphere, Ionosphere: Ionosphere/Atmosphere Interactions (0335), Ionosphere: Ionospheric Dynamics, Ionosphere: Ionization Processes (7823), Atmospheric Processes: Thermospheric Dynamics (0358)

Scientific paper

Ten years of measurements of the ionospheric F-layer peak height h max and peak density n max and of the horizontal neutral wind at these heights with the Japanese MU Radar are analyzed to detail the causes of the temporal variations of the peak parameters. In the absence of winds h max rides the height of a constant product of the atomic and molecular densities of the thermosphere. Since the mean wind does not change with solar activity, the h max change with solar activity is driven almost solely by a thermal expansion of the thermosphere. The seasonal variation of h max, on the other hand, is driven almost solely by the seasonal change in winds. The diurnal variation of h max is driven most importantly by winds, secondarily by thermal expansion. n max is proportional to the ratio of the atomic and molecular densities of the thermosphere at altitude h max but that ratio is insensitive to thermal expansion. The solar-activity change in n max is largely due to the change in solar EUV intensity, secondarily due to changes in neutral composition at the base of the thermosphere. The seasonal change in n max is semiannual in response to the semiannual change in neutral O density. The wind itself shows features of ion-drag control in almost every facet of its behavior except that its diurnal amplitude does not change with season, a result consistent with the explanation that one day is insufficient time to set up a nondivergent circulation pattern in the upper atmosphere. Our numerical results are valid only for the location of the MU Radar, but the understandings involved are broadly applicable to the midlatitude ionosphere.

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