Photoelectric spectrophotometry of quasi- stellar sources.
Spectral energy distributions of various quasi- stellar radio sources, using photoelectric spectrum scanner
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Spectral energy distributions of various quasi- stellar radio sources, using photoelectric spectrum scanner
Spectral energy distribution of source 3C 446 between August 17 and December 12, 1966
Radio Astronomy Explorer satellite radiometer system for measuring spectral energy distribution of solar bursts
Electron scattering, bremsstrahlung cross sections, and spectral energy distributions
Nonthermal optical flux from galaxies, estimating total flux emitted and spectral energy distribution
Spectral energy distribution of protons in inner radiation belt by Cosmos 137 satellite
Variable star BL Lacertae absolute spectral energy distribution in visible and IR regions, noting synchrotron features and possible quasar nature
Crab Nebula pulsar NP 0532 photoelectric spectrophotometry results, noting main pulse and interpulse spectral energy distributions similarity to extended synchrotron radiation
Cosmic X ray and gamma ray spectral energy distribution slope change explained by measurement process involving photon spectrum
Quasar 4C 05.34 absolute spectral energy distribution by multichannel photoelectric spectrometry
Omnidirectional cosmic gamma ray flux near one MeV observed by ERS-18 satellite, plotting spectral energy distribution
Solar constant and spectral energy distribution standard values by high altitude aircraft, balloon and spacecraft measurements
UV spectral energy distribution of Jupiter from rocket-borne Cassegrain telescope observation, computing planet geometric reflectivity in 2100- 3600 A range
IR stellar object HD 45677, discussing IR spectral energy distribution in terms of black body temperature range
Shadow band observations during 7 March 1970 solar eclipse, determining spectral energy distribution from magnetic tape recordings of collimated photocells output
Compact spectral irradiance probe has been designed and built which uses wedge filter in conjunction with silicon cell and operational amplifier. Probe is used to monitor spectral energy distribution of solar simulators and other high intensity sources.
The nature and chemical composition of comets as determined by their spectral energy distributions and polarization of the scattered radiation are discussed. The study is divided into two parts: (1) a description of the spectra and, (2) a discussion of the excitation mechanisms responsible for their production.
The spectral energy distribution and size of the source of infrared radiation from Herschel 36 in M8 have been investigated. Radiation from the diffuse source in the vicinity of the hourglass has been measured. It is shown that a significant fraction of the 10-microns flux comes from an unresolved source centered on Herschel 36. Other stars in M8 have also been investigated as potential sources of infrared radiation.