5,237 research outputs found
Raman anemometry, a method for component-selective velocity measurements of particles in a flow
An anemometer for the measurement of the velocity of particles of different substances in a flow, separate and apart from that of the flow itself, is described. The substances are distinguished by Raman scattering. The velocity is obtained by relating the autocorrelated scattering signal to the known laser beam profile
ISR spectra simulations with electron-ion Coulomb collisions
Incoherent scatter radars (ISR) rely on Thomson scattering of very high frequency or ultrahigh frequency radio waves off electrons in the ionosphere and measure the backscattered power spectra in order to estimate altitude profiles of plasma density, electron temperature, ion temperature, and ion drift speed. These spectra result from the collective behavior of coupled ion and electron dynamics, and, for most cases, existing theories predict these well. However, when the radar points nearly perpendicular to the Earth's magnetic field, the motion of the plasma across the field lines becomes complex and Coulomb collisions between electrons and ions become important in interpreting ISR measurements. This paper presents the first fully kinetic, selfâconsistent, particleâinâcell simulations of ISR spectra with electronâion Coulomb collisions. We implement a gridâbased Coulomb collision algorithm in the Electrostatic Parallel ParticleâinâCell simulator and obtain ISR spectra from simulations both with and without collisions. For radar directions greater than 5° away from perpendicular to the magnetic field, both sets of simulations match collisionless ISR theory well. For angles between 3° and 5°, the collisional simulation is well described by a simplified Brownian motion collision process. At angles less than 3° away from perpendicular the Brownian motion model fails, and the collisional simulation qualitatively agrees with previous single particle simulations. For radar directions exactly perpendicular to the magnetic field the simulated collisional spectra match those from the Brownian motion collision theory, in agreement with previous single particle simulations.This work was supported by NASA grants NNX14AI13G and NNX16AB80G and NSF grant PHY-1500439. This work used the XSEDE and TACC computational facilities, supported by NSF grant ACI-1053575. The work by Alex Fletcher was supported by NSF-AGS Postdoctoral Research Fellowship award 1433536 while at the Center for Space Physics, Boston University. Simulation produced data are archived at TACC and are available upon request. We thank John Swoboda of MIT Haystack Observatory for his suggestions on processing the simulated ISR spectra. (NNX14AI13G - NASA; NNX16AB80G - NASA; PHY-1500439 - NSF; ACI-1053575 - NSF; 1433536 - NSF-AGS Postdoctoral Research Fellowship at the Center for Space Physics, Boston University)First author draf
The White Dwarf -- White Dwarf galactic background in the LISA data
LISA (Laser Interferometer Space Antenna) is a proposed space mission, which
will use coherent laser beams exchanged between three remote spacecraft to
detect and study low-frequency cosmic gravitational radiation. In the low-part
of its frequency band, the LISA strain sensitivity will be dominated by the
incoherent superposition of hundreds of millions of gravitational wave signals
radiated by inspiraling white-dwarf binaries present in our own galaxy. In
order to estimate the magnitude of the LISA response to this background, we
have simulated a synthesized population that recently appeared in the
literature. We find the amplitude of the galactic white-dwarf binary background
in the LISA data to be modulated in time, reaching a minimum equal to about
twice that of the LISA noise for a period of about two months around the time
when the Sun-LISA direction is roughly oriented towards the Autumn equinox.
Since the galactic white-dwarfs background will be observed by LISA not as a
stationary but rather as a cyclostationary random process with a period of one
year, we summarize the theory of cyclostationary random processes, present the
corresponding generalized spectral method needed to characterize such process,
and make a comparison between our analytic results and those obtained by
applying our method to the simulated data. We find that, by measuring the
generalized spectral components of the white-dwarf background, LISA will be
able to infer properties of the distribution of the white-dwarfs binary systems
present in our Galaxy.Comment: 36 pages, 15 figure
Wideband Channel Estimation and Prediction in Single-Carrier Wireless Systems
AbstractâIn this contribution wideband channel estimation and prediction designed for single-carrier wideband wireless communications systems are investigated. Specifically, the single-carrier wideband pilot signal received by the receiver is first converted to the frequency-domain. Then, the envelope of the channel transfer function (CTF) is estimated in the frequency-domain, in order to reduce the effects of background noise on the channel prediction step to be invoked. Finally, channel prediction is carried out based on the estimated CTF in the frequency-domain, where a Kalman filter assisted long-range channel prediction algorithm is employed. Our simulation results show that for a reasonable signal-to-noise ratio (SNR) value the proposed frequency-domain based wideband channel estimator is capable of efficiently mitigating the effects of the background noise, hence enhancing the performance of wideband channel prediction
Optical and radio variability of the BL Lac object AO 0235+16: a possible 5-6 year periodicity
New optical and radio data on the BL Lacertae object AO 0235+16 have been
collected in the last four years by a wide international collaboration, which
confirm the intense activity of this source. The optical data also include the
results of the Whole Earth Blazar Telescope (WEBT) first-light campaign
organized in November 1997. The optical spectrum is observed to basically
steepen when the source gets fainter. We have investigated the existence of
typical variability time scales and of possible correlations between the
optical and radio emissions by means of visual inspection, Discrete Correlation
Function analysis, and Discrete Fourier Transform technique. The major radio
outbursts are found to repeat quasi-regularly with a periodicity of about 5.7
years; this period is also in agreement with the occurrence of some of the
major optical outbursts, but not all of them.Comment: to be published in A&
Digital spectral analysis of bistatic-radar echoes from Explorer 35
Bistatic radar echoes from Explorer 35 using 150 foot dish antenn
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