The middle and upper (MU) atmosphere radar IS observations
of electron density Ne profiles for 1986 - 1995 at Shigaraki
(34.85N, 136.10E) show a forenoon density depression
(bite-out) in summer both on individual days and in statistical
averages. The depression takes place generally between 7-12 LT,
above the F2-peak for low solar activity and around the F2-peak
for high solar activity. The maximum electron density NmF2 shows,
inboth percentage and time duration, a greater depression for
low solar activity than for high solar activity. With increasing
altitude, the forenoon Ne depression develops earlier for low
solar activity. In combination with the MU radar observations of
ion drifts and plasma temperatures, our modeling indicates that,
(1) transport processes such as the enhancement of electron temperature
Te, the poleward neutral wind, and the reduced upper boundary ionization
density, help to reduce Ne and result in a negative
in the morning hours in summer. Among those processes, the morning
enhancement of Te is found to be most important for the presence of
the forenoon bite-out, since it greatly increases the O+ diffusion
such that ionization outflow is significantly intensified; (2) the
forenoon bite-out occurs only in summer, not in other seasons,
because a) the smaller atmospheric composition ratio [O]/[N2] in
summer leads to a smaller daytime background Ne and thus to an enhanced
Te; b) the after-sunrise photochemical contributions (mainly the O+
production) are so small that
also tends
to be smaller. These two conditions give prominence to the transport
contributions; (3) the solar activity dependences of the forenoon
bite-out can be explained basically in terms of the low-electron-density
background; (4) the height of formation of the forenoon bite-out is also
related to the sunrise effect on photoionization.
AGU Index Terms: 2437 Ionospheric dynamics; 2443; 2419; 2447
Keywords/Free Terms: electron density, electron temperature, atmospheric composition, bite-out, MU radar.
ja 95JA00000