Application of control moment gyros in the attitude control of the Apollo Telescope Mount.
Control moment gyro subsystem application in attitude control system of Apollo Telescope Mount for solar phenomena data acquisition
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Control moment gyro subsystem application in attitude control system of Apollo Telescope Mount for solar phenomena data acquisition
Differential energy spectra of high energy primary cosmic ray protons and alpha particles from balloon flight data, noting solar activity effects
Worldwide changes in earth magnetic field determined by examination of magnetic field and interplanetary plasma data for solar wind near earth
Spacecraft instrumentation, biological sampling of Martian soil, Jupiter red spot data and solar wind variations, dielectric function of cold electron gas, and microwave spectra of ion radical
Infrared solar spectrum data for communications 160 to 162
Primordial solar system chemical composition for studies of origin and evolution, compiling solar composition data
Worldwide changes in geomagnetic field, determining causes by examining magnetic field and plasma data for solar wind and classifying as SSC or SI
Solar spectrum data covering wavelength intervals from 13138-14707 and 12187-17731 A and 1.4 micron water band
Solar burst time profiles and dynamic spectra for calculating theoretical values for Type 3 burst characteristics
Observational data for solar X-ray flares measured by Explorer 33 and Explorer 35 satellites
High energy solar flare data from neutron monitor stations supplemented by low energy data from interplanetary space probes Pioneer 6 and 7
Measuring solar irradiance data obtained at 75 to 80 km by X-15 aircraft using narrow band multichannel radiometer
Martian atmospheric temperature and pressure and temperature gradient determination by least squares differential correction of satellite photometric solar eclipse data
Radio spectrum analysis of two active regions based on Laplace transform and brightness temperatures from Nov. 12, 1966 solar eclipse data
Pioneer 9 interplanetary observations, presenting deep space data for solar rotations and radial gradient in VLF electric field behavior
Study of the higher-moment equations for a collisionless fully ionized plasma. For a collisionless, heat-conducting plasma, the distribution function f is cylindrically symmetric about the direction of the magnetic field. It is shown that under a certain assumption the fourth moments of f can be expressed as simple functions of lower moments. Thus no higher-moment terms appear in the third-moment equations. The two third-moment equations, which are obtained in a simple form, join other lower-moment equations to form a closed set of moment equations. The new equations can be used to study the thermal anisotropy and the heat flux of the solar-wind proton. A special case of the cylindrically symmetric distribution function f is found to resemble the proton distribution function reconstructed from solar-wind data, and this resemblance justifies the assumption needed for decoupling the moment equations.
Description of an international comparison of radiometers made on May 10 through 14, 1971, with 24 instruments, each one representing the calibration standard of a different country or a major laboratory. All were pyranometers, viewing the sun and sky, thus bypassing the conventional method of transferring the standard from Angstrom pyrheliometers. This is the first time that pyranometers from all around the globe have been brought together in order to verify the scale on which to report solar radiation data. A highly accurate data collection system measured simultaneously the output of each instrument and that of a reference standard at 20-sec intervals. Over 300,000 radiometric signals were recorded under varying atmospheric conditions, as well as data on turbidity, temperature, and other relevant parameters. Computer programs were developed for overnight analysis of the data and distribution to participants on the following day. Among major findings are that instruments of different types and independent calibration such as those of Eppley, U. S. A., World Radiation Center, Switzerland, and Melbourne, Australia, show better agreement than anticipated, that certain national standards have to be revised by as much as 16% and that the cosine factor is highly dependent on the type of instrument.