Radar studies of Venus.
Radar studies of Venus, noting values for rotation vector, latitudes and longitudes of several features and Earth influence on Venus rotation
PLANETARY MOTION↗
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Search indexed NASA NTRS and DOE OSTI research on propulsion, heat transfer, battery materials and energy systems. Follow report and document links to the original sources.
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A rapidly moving spot on Jupiter's North Temperate Belt.
Rapid drift in longitude of small dark spot on south edge of Jupiter North Temperate Belt, noting sinusoidal displacement characteristics and measurement with blue and UV photography
PHOTOGRAPHIC MEASUREMENT↗
Almost-continuous radio emission from Jupiter at 8.9 and 10 MHz.
Jupiter radiation recorded almost every night with antenna arrays shows emission dependency on Jupiter longitude and Io position
JUPITER /PLANET/↗
GMT/local-time conversion chart
GMT/local-time conversion is made by a longitude pocket instrument that automatically indicates desired information by simply manipulating the moveable portion of the instrument in accordance with a set of simple instructions imprinted on the reverse side of the instrument.
Creveling, C. J.↗
Single and double integration in the method of variation of parameters.
Single and double integration in method of variation of parameters for mean longitude or anomaly analyzed for influence on set not including such function
VARIATION METHOD↗
X-ray spectra of several cosmic sources.
X-ray spectral distributions and fluxes in low kev range of five cosmic sources at low galactic latitude and longitude, noting effective temperature
RADIATION DETECTOR↗
Theoretical description of trapped electron diffusion in the South American anomaly.
Fokker-Planck equation for geomagnetically trapped electron distribution as function of longitude, time, energy and mirror-point field intensity
GEOMAGNETICALLY TRAPPED PARTICLE↗
Radar studies of Venus.
Radar studies of Venus noting values for rotation vector, latitudes and longitudes of several features and Earth influence on Venus rotation
VENUS↗
Summary of Apollo and Lunar Logistics System Plans
The basic mission objective of Project Apollo is to land men on the Moon and return them to Earth at the earliest practicable date. The Apollo crew will consist of three men, two of whom will land on the surface of the Moon, conduct surface operations for up to 24 hr, and then rejoin the third crew member in lunar orbit for return to Earth. Initial Apollo spacecraft capabilities will require the early landings to be within +or-lO deg of the lunar equator on the visible side of the Moon, with preference for landing sites in the leading quadrant (between 270 and 360 deg lunar longitude). As presently planned, the Apollo spacecraft will be capable of carrying approximately 200 lb of scientific equipment to the lunar surface and of bringing approximately 80 lb of lunar material back to Earth. A detailed plan for utilization of crew capabilities while on the lunar surface is not expected to be complete for some time. The first Apollo lunar mission is now scheduled for the late 1960's with additional launches planned at reasonable intervals. i
Taylor, W. B.↗
Gemini Program Mission Report: Gemini IV
The second manned mission of the Gemini Program, Gemini IV, was launched from Complex 19 at Cape Kennedy, Florida, at 10:16 a.m. e.s.t. on June 3, 1965. The mission was successfully concluded on June 7, 1965, with the recovery of the spacecraft by the prime recovery ship, the aircraft carrier U.S.S. Wasp, at 27 deg 44' N. latitude, 74 deg 11' W. longitude at 2:28 p.m. e.s.t. This manned long-duration flight was accomplished 10 weeks after the three-orbit manned flight which qualified the Gemini spacecraft and systems for orbital flight. The spacecraft was manned by Astronaut James A. McDivitt, command pilot, and Astronaut Edward H. White II, pilot. The flight crew completed the 4-day mission in excellent physical condition, and demonstrated full control of the spacecraft and competent management of all aspects of the mission.
Source record↗
Theory of a refined earth model
Refined equations are derived relating the variations of the earths gravity and radius as functions of longitude and latitude. They particularly relate the oblateness coefficients of the old harmonics and the difference of the polar radii /respectively, ellipticities and polar gravity accelerations/ in the Northern and Southern Hemispheres.
Krause, H. G. L.↗
On the computation of solar elevation angles and the determination of sunrise and sunset times
Computation of solar elevation angles and determination of sunrise and sunset times as function of latitude, longitude, and date
Woolf, H. M.↗
The spectra of several X-ray sources in Cygnus and Scorpio.
X ray spectra from sources in Cygnus and Scorpio, noting three strongest in Cygnus and six at low galactic longitude
Giacconi, R.↗
The microwave phase effect of Mercury.
Mercury brightness temperatures from contact conduction and radiative transfer equation solutions, noting dependence on heliocentric longitude and phase angle
Morrison, D.↗
Jupiter's Red Spot in 1965-1966.
Jupiter Red Spot latitude and longitude measured from photographic plates /1965-1966/
Solberg, H. G., Jr.↗
The use of resonant librating orbits in satellite geodesy.
Long term effects of longitude gravity harmonics on semimajor axis of circular orbits, discussing resonant librating orbits use in satellite geodesy
Wagner, C. A.↗
Simplified Analytical Model for Use in Design of Pump-Inlet Accumulators for the Prevention of Liquid-Rocket Longitudinal Oscillation (POGO)
Analytical model for use in design of pump inlet accumulators for prevention of liquid rocket longitudal oscillation
Lewis, William↗
Local interstellar reddening.
Interstellar reddening in solar vicinity, analyzing roles of galactic latitude and longitude and heliocentric distance
Gottlieb, D. M.↗