High resolution nighttime cloud-cover radiometer Quarterly report, 1 Jan. - 1 Apr. 1967
Environmental test data for high resolution nighttime cloud cover radiometer
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Environmental test data for high resolution nighttime cloud cover radiometer
Meteorological measurements over southern California using airborne medium resolution infrared radiometer
Anisotropy of reflected solar radiation from various surfaces as measured with aircraft-mounted radiometer
Multichannel radiometer measurement of solar irradiance for realizing spacecraft radiative equilibrium
Stabilized cross correlation radiometer for use at decametric wavelength, using two feedback loops controlling four noise diodes
L and S-band radiometer brightness temperature measurements from a salt-water pond were made of as a function of salinity and temperature.
This paper describes the reflector antenna system for the High altitude MMIC sounding radiometer (HAMSR) on a remotely piloted aircraft.
This paper presents the design and performance evaluation of two water vapor radiometers which were developed for the Cassini gravitational wave search experiments.
Recent innovations in ultra-high frequency, semiconductor device/component technology have enabled both traditional and new applications for space-borne millimeter- and submillimeter-wave heterodyne radiometer instruments.
Preliminary design details and laboratory test results of a microwave radiometer operating near the 22.2 GHz water vapor resonance line are presented. Radiometric stability to 10mK for several hours is the design goal. Early indications are that these goals are being met in the prototype system.
An out-of-band correction algorithm is evaluated for the Multi-Angle Imaging Spectro-Radiometer (MISR). The objective for MISR is to report scene radiances, ad averaged over the in-band spectral response region.
The NASA/JPL Airborne Rain Mapping Radar (ARMAR) on board the NASA DC-8 aircraft, several airborne multi-channel radiometers on board the NASA ER-2 aircraft, and the doppler radars on board the NOAA P-3 aircraft were deployed for rainfall observations collected over the Western Pacific Ocean during the TOGA/COARE experiment in January and February of 1993. Results of rain system observations are given.
Winds over the ocean modulate the air-sea fluxes of heat, moisture, gases and particulates, regulating the crucial coupling between atmosphere and ocean that establishes and maintains global and regional climate. Global mapping (using spaceborne scatterometers) of ocean wind is crucial for many oceanographic and atmospheric studies. An overview of polarimetric wind radiometer (new) technology is given.
An NEDT analysis of a Dicke radiometer with noise diode injenction is presented.
Data from terrestrial GPS receivers are being used in growing numbers of applications requiring precise tropospheric sensing. One emerging application is the calibration of water vapor measurements from spaceborne microwave radiometers.
Multi-Angle Imaging Spectro-Radiometer (MISR) is part of an Earth observing system (EOS) payload to be launched in 1998 to study the ecology and climate of Earth. EOS will acquire multi-angle images in reflected sunlight at nine angles.
Weather prediction and hurricane tracking would greatly benefit of a continuous imaging capability of a hemisphere at millimeter wave frequencies. We are developing a synthetic thinned aperture radiometer (STAR) prototype operating from 50 to 56 GHz as a ground-based testbed to demonstrate the technologies needed to do full earth disk atmospheric temperature soundings from Geostationary orbit with very high spatial resolution. The prototype consists of a Y-array of 24 MMIC receivers that are compact units implemented with low noise InP MMIC LNAs, second harmonic I-Q mixers, low power IF amplifiers and include internal digital bias control with serial line communication to enable low cost testing and system integration. Furthermore, this prototype STAR includes independent LO and noise calibration signal phase switching circuitry for each arm of the Y-array to verify the operation and calibration of the system.
Preliminary details of a 2-D synthetic aperture radiometer prototype operating from 50 to 55 GHz will be presented. The laboratory prototype is being developed to demonstrate the technologies and system design needed to do millimeter-wave atmospheric soundings with high spatial resolution from Geostationary orbit. The concept is to deploy a large thinned aperture Y-array on a geostationary satellite, and to use aperture synthesis to obtain images of the Earth without the need for a large mechanically scanned antenna. The laboratory prototype consists of a Y-array of 24 horn antennas, MMIC receivers, and a digital cross-correlation sub-system.