HR: 1340h
AN: SA13A-0226    [Abstracts]
TI: The Charged Aerosol Release Experiment (CARE)
AU: * Bernhardt, P A
EM: bern@ppd.nrl.navy.mil
AF: Plasma Physics Division Naval Research Laboratory , 4555 Overlook, SW, Washington, DC 20375 United States
AU: Ganguli, G
SA13A-0226 AF: Plasma Physics Division Naval Research Laboratory , 4555 Overlook, SW, Washington, DC 20375 United States
AU: Lampe, M
EM: martin.lampe@nrl.navy.mil
AF: Plasma Physics Division Naval Research Laboratory , 4555 Overlook, SW, Washington, DC 20375 United States
AU: Scales, W A
EM: wscales@vt.edu
AF: Bradley School of Electric and Computer Engineering Virginia Tech, 2212 Burchleaf Lane, Blacksburg, VA 24061 United States
AB: The physics of radar scatter from charged particulates in the upper atmosphere will be studied with the Charged Aerosol Release Experiment (CARE). In 2008, two rocket payloads are being designed for launch North America. The purpose of the CARE program is to identify the mechanisms for radar scatter from polar mesospheric clouds. Polar mesospheric summer echoes (PMSE) are observed at high latitudes when small concentrations of electrons (one-thousand per cubic cm) become attached to sub-micron dust particles. Radar in the VHF (30-300 MHz) frequency range have seen 30 dB enhancements in radar echoes coincident with formation of ice near 85 km altitude. Radar echoes from electrons in the vicinity of charged dust have been observed for frequencies exceeding 1 GHz. Some fundamental questions that remain about the scatting process are: (1) What is the relative importance of turbulent scatter versus incoherent (i.e., Thompson) scatter from individual electrons? (2) What produces the inhomogeneous electron/dust plasma? (3) How is the radar scatter influenced by the density of background electrons, plasma instabilities and turbulence, and photo detachment of electrons from the particulates? These questions will be addressed when the CARE program releases 50 kg of dust particles in an expanding shell at about 300 km altitude. The dust will be manufactured by the chemical release payload to provide particulate sizes in the 10 to 1000 nm range. The expanding dust shell will collect electrons making dense, heavy particles the move the negative charges across magnetic field lines. Plasma turbulence and electron acceleration will be formed from the charge separation between the magnetized oxygen ions in the background ionosphere and the streaming negatively charged dust. Simulations of this process provide estimates of plasma structure which can scatter radar. As the particulates settle through the lower thermosphere into the mesosphere, artificial mesospheric clouds will be formed. Radar scatter form this artificial layer will be compared with natural PMSE observations. Along with the chemical release rocket, in situ probes with a separate instrumented payload will be used to measure dust density, electric fields, plasma density and velocity, and radio wave scattering.
DE: 0305 Aerosols and particles (0345, 4801, 4906)
DE: 2427 Ionosphere/atmosphere interactions (0335)
DE: 7863 Turbulence (4490)
SC: SPA-Aeronomy [SA]
MN: Fall Meeting 2005