On-orbit Servicing, Assembly and Manufacturing (OSAM) Near-Term in-Space Developmental Test Persistent Platform: ESPA-Star Based Implementation
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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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Explore the source record for details and available documents.
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Explore the source record for details and available documents.
Firehose instability behavior in highly relativistic plasmas is not highly sensitive to exact particle velocity distribution
Spacecraft libration point motion in restricted four body model including earth-moon orbit plane inclination to ecliptic, noting solar effects
Daily rhythm in concentration of tyrosine in plasma of normal human males
Solar protons delayed access into polar regions during 2 November 1967 solar particle event, discussing north-south asymmetry
An experiment was conducted with the NCAR Sabreliner to measure the ice water content (IWC) and the total ice budget within its contrail. Particle size distributions were measured with an optical-array particle size spectrometer. The experiment was performed in a region of the atmosphere void of natural ice crystals (cirrus) but estimated to be above ice saturation and favorable to ice crystal growth. The IWC measured was found to be in excess of 0.1 g/cu m near the contrail axis with average values of a few hundredths of a gram throughout the contrail. The measured water mass within the contrail was found to be four orders of magnitude greater than that computed as a combustion product. Average crystal sizes of nearly 0.5 mm allow for a transfer of moisture at generation level to much lower levels before reevaporation. Because of the magnitude of the measured effect and its believed frequent occurrence, the overall effect of subtropopause jet traffic is likely to lower the water abundance at the most traveled levels.
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The paper is concerned with the anisotropy of 1.3 to 2.3 MeV protons measured with an electron/isotope spectrometer aboard the IMP 7 satellite during 317 six-hour periods, excluding periods when prompt solar particle events are observed. It is found that the diffusive streaming is predominantly toward the sun, indicating an essentially positive radial gradient in the particle density. The long-term average radial component of this anisotropy and its dependence on the solar wind speed are consistent with the anisotropy calculated with a steady-state propagation model including adiabatic energy loss.
The Skylab white light coronagraph observed a coronal streamer during five successive limb passages between June 1 and August 6, 1973. Measurements of the streamer's latitude, brightness and polarization during three east-limb passages show that: (1) the streamer's axis migrated southward from 25 deg N at first east-limb passage to 11 deg N at second east-limb passage to 8 deg N at third east-limb passage, (2) the streamer's mass and mass gradient with height varied by 20-50% from one east-limb passage to the next, (3) the streamer's longitudinal extent was observed to be less on successive east-limb passages, and (4) mass changes (distinct from coronal transients) occurring over hours were detected during at least two limb passages. The streamer was found to be associated with a complex of solar activity consisting of active regions and filaments.
Thermal maps of Venus on 16 days during a span of 43 days just before inferior conjunction were obtained during 1973-1974 and are described. The research represents a first step towards the goal of using ground-based observations to determine the time and space scales of dynamical events taking place in the Venus clouds. The described average limb darkening differs from that reported by Ingersoll and Orton (1974). Real day-to-day changes in limb darkening, one occasion of a 4-day repetition of a thermal anomaly, solar-related anomalies, and a southern hemisphere solar-related disturbance are discussed.
A field experiment designed to further understand the formation and transport of visibility reducing aerosols and to characterize regional scale air masses and urban plumes is described. Measurements were made primarily in the Ohio River Valley region. The NASA participation included obtaining measurements for the determination of mixing layer height and ozone profiles by using airborne remote sensor systems such as the ultraviolet differential absorption lidar, the high spectral resolution lidar, and the laser absorption spectrometer. Other NASA systems included the microwave atmospheric remote sensor, tethered balloons, an in situ measurements aircraft, and several photometer/transmissiometer systems.