ROCKET MEASUREMENT OF THE ELECTRON DENSITY DISTRIBUTION IN THE TOPSIDE IONOSPHERE
Rocket measurement of the electron density distribution in the topside ionosphere
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Rocket measurement of the electron density distribution in the topside ionosphere
Electron density probes to perform measurements in flow fields at high altitudes
Simple model atom selection for electron density calculation in low temperature nonequilibrium Cs plasmas
Spatial resolution in measurement of electron density and temperature variation in thermal plasma of cylindrical cross section using millimeter waves
The differential absorption technique of measuring electron densities as a function of height in the D region is discussed. In the basic experiment, pulses of medium or high frequency, usually at a fixed frequency (2 to MHz), are radiated upwards with known wave polarizatin (usually linear or circular) from a transmitter at ground level. Partial reflections, from ionospheric scatterers at heights below the E region, are received at the ground, and are resolved into two characteristic components, the ordinary (0) and extraordinary (E) modes whose amplitude ration A(x)/A(o) is then measured as a function of height, h. The heights of these are determined by delay times, the group retardation being minimal in the undisturbed D-region. The electronic system can be very simple. Power splitters and quadrature networks to separate the A(x) and A(o) components are commercially available at low prices and an A-D converter, height-gate system, and microcomputer allows the real-time calculation of mean amplitudes. The ratio of the coefficients of reflection of the two modes, as they originate at each reflection height is then calculable.
Topside ionogram reduction for ionospheric electron density determination, using geomagnetic strength at all heights, iteration and change of variables
Lower ionosphere electron density changes with solar zenith angle during active sun year
Recent progress made in modeling the electron density profile in the topside ionosphere is reviewed. The results of different F2 peak models are addressed in the light of the data, and the outlook for further progress in this area is discussed. Efforts made toward determining the topside profile shape are reviewed and assessed.
F-layer nightglow 6300 angstrom emission intensity and electron density data, noting variations in emissions
Electron density profiles in lower atmosphere due to solar cosmic rays
Atmosphere and electron density distribution above f2 peak
Problems encountered during efforts to reformulate the IRI description of the electron density profile are examined. Consideration is given to Booker's (1979) proposal that the unique, analytic profile functions should cover the entire ionospheric height range. The IRI topside model is reviewed and the electron density profile of the middle and lower ionosphere are discussed. Rawer's (1983) procedure for combining the topside, middle, and lower ionospheric profiles into one analytic profile is reviewed.
This paper reviews the ground-based and rocket techniques that are presently being used to determine electron density profiles in the ionospheric D region. Ground-based techniques include VLF, LF, and MF sounding; differential absorption and differential phase measurements using partial reflections; wave interaction; and incoherent scatter. Rocket techniques include differential absorption and Faraday rotation in association with high-resolution dc probes calibrated by means of the radio measurements. The characteristics of the aforementioned techniques are presented, including time and height resolution, accuracy estimates, preferred height ranges, and problems encountered. Electron density profiles obtained with these techniques are presented for comparable solar zenith angles and undisturbed solar and geophysical conditions.
Langmuir probes for determining electron density surrounding reentry vehicles
Electron density and temperature profiles measured in exhaust of magnetoplasma-dynamic source
A study is made of the effect on theoretical electron-density profiles of vibrational enhancement in the rate of the reaction O(+) + N2 yields NO(+) + N. It is shown that the F-region electron-density depression that is observed in stable auroral red (SAR) arcs may be caused by vibrational excitation of molecular nitrogen.
Obtaining electron density profiles from capacitive ionospheric rocket probes
Electron density and temperature measured in exhaust of magnetoplasmadynamic /MPD/ source, using Langmuir probe and spectrometry