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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.
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Linear Estimation of Particle Bulk Parameters from Multi-Wavelength Lidar Measurements
An algorithm for linear estimation of aerosol bulk properties such as particle volume, effective radius and complex refractive index from multiwavelength lidar measurements is presented. The approach uses the fact that the total aerosol concentration can well be approximated as a linear combination of aerosol characteristics measured by multiwavelength lidar. Therefore, the aerosol concentration can be estimated from lidar measurements without the need to derive the size distribution, which entails more sophisticated procedures. The definition of the coefficients required for the linear estimates is based on an expansion of the particle size distribution in terms of the measurement kernels. Once the coefficients are established, the approach permits fast retrieval of aerosol bulk properties when compared with the full regularization technique. In addition, the straightforward estimation of bulk properties stabilizes the inversion making it more resistant to noise in the optical data. Numerical tests demonstrate that for data sets containing three aerosol backscattering and two extinction coefficients (so called 3 + 2 ) the uncertainties in the retrieval of particle volume and surface area are below 45% when input data random uncertainties are below 20 %. Moreover, using linear estimates allows reliable retrievals even when the number of input data is reduced. To evaluate the approach, the results obtained using this technique are compared with those based on the previously developed full inversion scheme that relies on the regularization procedure. Both techniques were applied to the data measured by multiwavelength lidar at NASA/GSFC. The results obtained with both methods using the same observations are in good agreement. At the same time, the high speed of the retrieval using linear estimates makes the method preferable for generating aerosol information from extended lidar observations. To demonstrate the efficiency of the method, an extended time series of observations acquired in Turkey in May 2010 was processed using the linear estimates technique permitting, for what we believe to be the first time, temporal-height distributions of particle parameters.
Long-Wavelength 640 x 486 GaAs/AlGaAs Quantum Well Infrared Photodetector Snap-shot Camera
The performcance of this QWIP camera is reported including indoor and outdoor imaging.
Genetically optimized dual-wavelength all-dielectric metasurface based on double-layer epsilon-near-zero indium-tin-oxide films
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A Formalism for Calibrating the Instrumental Polarization of Radio Interferometric Arrays at Meter Wavelengths Using Unpolarized Sky: A Demonstration Using MWA Observations
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Correction: Dupuy, E., et al. Comparison of XH2O Retrieved from GOSAT Short-Wavelength Infrared Spectra with Observations from the TCCON Network. Remote Sens. 2016, 8, 414
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Wavelengths and Energy Levels of the Upper Levels of Singly Ionized Nickel (Ni ii) from 3d 8 ( 3 F)5f to 3d 8 ( 3 F)9s
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Classical Novae at Radio Wavelengths
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Observations of Venus, the Sun, Moon, and Tau A at 1.18-cm Wavelength
Venus, sun, moon, and tau a radio-astronomical observations
Results of measurements in the 70.16 cm wavelength of radio emission intensity of a series of discrete sources, the moon and jupiter <rezul'taty izmereniy intensivnosti radioizlucheniya ryada diskretnykh istochnikov, luny, i yupitera na volne 70.16
Radio emission measurements of moon and jupiter relating to cassiopeia a
Results of measurements of moon's radio emission in the 1.6 cm wavelength <rezyl'taty izmereniya radioizlucheniya luny na volne lambda equals 1.6 cm<
Radio emission measurements of moon using modulation radiometer with parametric amplifier
Fresnel zone plate forms images at wavelengths below 1000 angstroms
Fresnel zone plate with openings replacing the usual transparent rings produces images in a vacuum ultraviolet. The plate is made by etching and electrodeposition.
Absorption in the atmosphere of radio emission at 70.16 cm wavelength <pogloshcheniye radioizlucheniya na volne 70.16 cm v atmosfere<
Radio emission absorption in atmosphere
<ground-based observations of venus in the wavelength range from 0.90 to 1.40 cm and balloon-borne measurements of microwave emission from molecular oxygen in the terrestrial atmosphere< final report, jun. 1 - dec. 31, 1964
Venus radio spectrum and microwave emission of atmospheric molecular oxygen
Receiver techniques and detectors for use at millimeter and submillimeter wavelengths semiannual report, 1 sep. 1964 - 28 feb. 1965
Signal detection and receiving techniques for millimeter and submillimeter waves
The wavelength dependence of polarization. iii- the lunar surface final report
Photoelectric photometry, luminescence, and polarimetry of lunar surface - selenography