Examples of the meteorological capability of the high resolution infrared radiometer on the Nimbus I satellite.
High resolution IR radiometer on Nimbus I satellite for providing detailed night cold information
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High resolution IR radiometer on Nimbus I satellite for providing detailed night cold information
High resolution scanning radiometer for cloud cover and cloud motion observation from Applications Technology Satellites F and G
Color enhancement of Nimbus high resolution infrared radiometer data
Reliability and failure evaluation of high resolution wavelength spectrometer and solar pointing control onboard Aerobee flight
Accuracy of high resolution infrared radiometers on Nimbus 2
Automatic heteroatomic plotting of high resolution mass spectral data, presenting relative intensity vs elemental composition in bar form
High resolution solar spectrometer for airborne IR observations, discussing 4 meter Czerny- Turner scanning spectrometer in NASA Convair 990 aircraft
Large area high resolution cosmic ray charge composition detector
High resolution study of solar atmosphere of H alpha line
Absolute frequency wideband high resolution determination, using frequency synthesizer as phase locked loop local oscillator
High resolution power spectra of 77 years of Zurich daily sunspot numbers were computed using various lags and data point intervals. Major harmonic peaks of the approximately 124-month period showed up strongly as well as the 27-day solar rotational period.
A design study for a high resolution meteor radar system is carried out with the objective of measuring upper atmospheric winds and particularly studying short period atmospheric waves in the 80 to 120 km altitude region. The transmitter that is to be used emits a peak power of 4 Mw. The system is designed to measure the wind velocity and height of a meteor trail very accurately. This is achieved using a specially developed digital reduction procedure to determine wind velocity and range together with an interferometer for measuring both the azimuth and elevation angles of the region with a long baseline vernier measurement being used to refine the elevation angle measurement. The resultant accuracies are calculated to be + or - 0.9 m/s for the wind, + or - 230 m for the range and + or - 0.12 deg for the elevation angle, giving a height accuracy of + or - 375 m. The prospects for further development of this system are also discussed.
High resolution radio observations of Jupiter were investigated with the use of the Stanford synthesis telescope. The best fit disk was computed from the emission of Jupiter and the residual brightness, due to nonthermal mechanisms was measured.
A prototype high resolution, adjustable, lockable mirror mount is described, suitable for use as a resonator end mirror mount in fieldable lasers. The prototype was vibrated to 15g levels, 10-2000 Hz, and was shown to be stable to within 1 arc second and settable to an accuracy of 10 arc seconds. Improvements to be made to the prototype are outlined which will significantly improve the accuracy without sacrificing the other attributes of the prototype.
The High Resolution Imaging Instrument for the HEAO-B X-ray Telescope satellite is designed to reproduce images of celestial X-ray sources in the range of 0.2 to 4.0 keV. It provides both imaging and temporal data. The basic detector is a two-stage microchannel plate with a crossed-grid charge detector. Preamplifiers, detector bias supplies, and some processing circuits are colocated with the detector. The remaining electronic circuits are located in a remote central electronic assembly. The processing system is designed for single-photon processing. The imaging data rate is limited to 100 data points per second. Non-imaging total-field count rate is acquired with a maximum dead time of 14 microseconds per event.
The Advanced High Resolution Radiometer, Mod 2 (AVHRR/2) is a modification of the original AVHRR (AVHRR/1) to expand the number of channels from four to five and provide additional sensing in the infrared region. A comparison of the spectral regions employed in the two instruments is given. Three of the channels are the same on both instruments. The difference in instruments is in the long wave IR region where a single channel was replaced by two channels. The modification from AVHRR/1 to AVHRR/2 was done with a minimum of changes. The areas of change are highlighted and the modifications by module are summarized. It is seen that the primary changes are in the relay optics and in the cooler. In this development program only two models are involved. The first model, the Optical Test Model was constructed and tested to prove the performance and structural integrity of the optical system and the modified cooler. The second model constructed is the Protoflight. Only the areas of the AVHRR/2 which were modified from the AVHRR/1 design are discussed.
The design of a high resolution, field portable spectrometer system is presented. The system provides the spectral resolution previously available only with laboratory based systems. The system's portability allows for essential in situ measurements, provides rapid acquisition and calibration of spectral reflectance data over a wavelength band from about 300 to 1000 nm. Features include a calibration scheme for normalizing data to the incident radiation, and the injection of a spectral calibration signal. Laboratory tests indicate that the system will perform as expected, and plans are being made to integrate the system with a ground based active and passive microwave data acquisition system.
The HEAO-3 high resolution gamma-ray spectrometer observed Cygnus X-1 for a total of 148 days between Sept. 27, 1979 and June 2, 1980. During this period, an upward and a downward transition of the hard X-ray flux in the 48-300 keV range were observed. The time scales of these transitions were long (20-50 days) compared with previous observation of the same source. The second, downward, transition was anticorrelated with the 1-12 keV flux, a type of behavior observed previously; however, the upward transition was accompanied by an upward transition in the low-energy X-ray flux, a result contrary to previous experience.