SEARCH · Engineering Papers
Search indexed NASA NTRS and DOE OSTI research on propulsion, heat transfer, battery materials and energy systems. Follow report and document links to the original sources.
Quote a phrase for an exact phrase match. Source license links do not imply unrestricted reuse.
Determination of ionospheric electron density by analysis of faraday rotation records received from a transmitting satellite
Polarized EM wave propagation and microwave Faraday rotation in solid state plasma in circular waveguide under strong magnetic field
Faraday rotation of radio beacon satellite signals during traveling ionospheric disturbances simulated for spaced ground stations
Quasi-stationary coronal magnetic field and electron density from Faraday rotation experiment, using theoretical model
Linearly polarized CW signal transmission through near solar corona, measuring Faraday rotation
The effect of Faraday rotation on the circular polarization of an electromagnetic wave propagating through a magnetized plasma is calculated for various limits of the plasma and wave parameters appropriate to a 30-Hz wave in the Crab Nebula. It is shown that a static magnetic field of the proper geometry and only a few times stronger than the wave field can reduce the circular polarization of the nonlinear inverse Compton radiation to a value below the observed upper limit.-
ATS 1 Faraday effect data applied to Pioneer 6 space probe solar corona data
Ionospheric electron content from Faraday rotation measurements of ATS 1 and Pioneer 7 space probe
Ionospheric electron content from Faraday rotation measurements of earth satellite and deep space probe
Geomagnetic field inclination determination by incoherently scattered signal Faraday rotation calibration and simultaneous ionosonde measurements of ionospheric electron density
To enable several orders of magnitude increases in average power and energy handling capability of Faraday rotators, the technology utilizes high speed gas cooling to efficiently remove thermal loading from the Faraday optic faces while minimizing the thermal wavefront and thermal birefringence by creating a longitudinal thermal gradient. A recirculating gas cooling manifold accelerates the gas over the surface of the slab to create a turbulent flow condition which maximizes the surface cooling rate. The technology further provides a spatially uniform thermal profile on the Faraday slabs.
Ionospheric electron content calculations based on satellite measurements of Faraday rotation and phase path length variations
Mean and variance of Faraday rotation and pulsar signal dispersion in galactic turbulent structure, applying to statistically homogeneous disk model of Galaxy
Ionospheric electron content measurements from satellite signals Faraday rotation, criticizing graphical procedure for ambiguity reduction
The rate constant and branching ratios of ethyl reaction with hydroperoxyl radical, C 2 H 5 + HO 2 (1), a key radical-radical reaction for intermediate temperature combustion chemistry, were measured in situ for the first time in a photolysis Herriott cell by using mid-IR Faraday rotation spectroscopy (FRS) and UV-IR direct absorption spectroscopy (DAS). The microsecond time-resolved diagnostic technique in this work enabled the direct rate measurements of the target reaction at 40 and 80 mbar and reduced the experimental uncertainty considerably. C 2 H 5 and HO 2 radicals were generated by the photolysis of (COCl) 2 /C 2 H 5 I/CH 3 OH/O 2 /He mixture at 266 nm. By direct measurements of the transient profiles of C 2 H 5 , HO 2 and OH concentrations, the overall rate constant for this reaction at 297 K was determined as k 1 (40 mbar) = (3.8 ± 0.8) × 10 –11 cm 3 molecule –1 s –1 and k 1 (80 mbar) = (4.1 ± 1.0) × 10 –11 cm 3 molecule –1 s –1 . As a result, the direct observation of hydroxyl radical (OH) indicated that OH formation channel was the major channel with a branching ratio of 0.8 ± 0.1.
Traveling ionospheric disturbances found responsible for irregular variations in electron content using Faraday rotation observations at stations situated by triangulation
Radar astronomical polarization measurements for lunar echoes by exploiting ionospheric Faraday rotation with linearly polarized antenna
The design and performance of a wide bandwidth linear polarization-modulator based on the Faraday effect is described. Faraday Rotation Modulators (FRMs) are solid-state polarization switches that are capable of modulation up to approx 10 kHz. Six FRMs were utilized during the 2006 observing season in the Background Imaging of Cosmic Extragalactic Polarization (BICEP) experiment; three FRMs were used at each of BICEP fs 100 and 150 GHz frequency bands. The technology was verified through high signal-to-noise detection of Galactic polarization using two of the six FRMs during four observing runs in 2006. The features exhibit strong agreement with BICEP fs measurements of the Galaxy using non-FRM pixels and with the Galactic polarization models. This marks the first detection of high signal-to-noise mm-wave celestial polarization using fast, active optical modulation. The performance of the FRMs during periods when they were not modulated was also analyzed and compared to results from BICEP fs 43 pixels without FRMs.