UV-sensitive photoemitters.
Far UV transmitting windows, particularly lithium fluoride, and response measurements below 2000 angstroms, noting fabrication on solar blind materials
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Far UV transmitting windows, particularly lithium fluoride, and response measurements below 2000 angstroms, noting fabrication on solar blind materials
Charge compensation defects influence on UV EXCITATION spectrum of rare earth doped crystals fluorescence
Far UV twilight airglow by rocket photometer measurements noting height profile similarity to dayglow
Comparison of UV scanner/photomultiplier tubes with image orthicons
UV-2T film evaluated for effects of advanced exposure on sensitivity to shortwave ultraviolet radiation
Design and calibration of far UV photometers
Interferometric technique for measuring atomic or molecular oscillator strengths in vacuum UV
Venus photography in UV by 61-inch telescope, discussing low contrast clouds recognition technique
Solar UV flash spectrum by spectroheliographs flown aboard Aerobee 170 mission during total solar eclipse
ZnO coating pigment for spacecraft thermal control, examining UV irradiation effects on electrical properties
Supergiant alpha Car UV spectrophotometry from Gemini 11, comparing with model atmosphere
Determining solar absorptance stability of metallized Teflon second surface mirror thermal control coatings as function of electron, proton, and UV radiation dosage
Oxygen and carbon dioxide continua absorption cross sections in Schumann and far UV regions by photoelectric technique with vacuum monochromator
Solar UV radiation data during 7 March 1970 eclipse from photometers sensitive to narrow bands, discussing sources, atmospheric absorption and D region ionosphere
Atomic oxygen and hydrogen identification in Mars upper atmospheric emission spectra by Mariner UV spectrometer, inferring carbon monoxide presence by self absorption
The design, construction, testing, calibration, flight performance and flight data of an Ebert ultraviolet spectrometer are described which is an accurate representation of the conceptual design of the Apollo 17 UV spectrometer. The instrument was flown in an Aerobee 350 rocket from Wallops Island, Va., at 7:10 p.m. EDT on June 10, 1971 to an altitude of 328 km with a solar elevation angle of about 11 deg.
Reactions of various polymers, such as polystyrene and its stereo-specific isomers, butylrubber, nylon, etc., with nitrogen dioxide and sulfur-dioxide were studied over the past few years. More recently, work has been initiated on the influence of polymer morphology on degradation of polymers in presence of these gases, near UV radiation and oxygen. Unexpected effects have been observed during chain scission near room temperature. Thus, for instance, isotactic polystyrene of various crystallinities, as far as extent and type are concerned, show marked differences in their degradation characteristics. Thus, for instance, crystalline polymers show faster degradation than amorphous ones, which seems to be contrary to expectations. However, this phenomenon can be explained in quite a consistent manner. The importance of all these reactions in connection with air pollution is briefly discussed.
This experiment obtained imagery of the earth and the moon at a series of wavelength intervals in the near ultraviolet. These photographs were used to aid in the interpretation of the UV appearance of other planets in the solar system, especially mars and venus. The filter and film characteristics are described, as well as the ozone absorption coefficient curve.