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rockets
X-ray data collected by means of rockets, balloons, and satellites during 1964-1979 are listed.
      
We have used temperature data obtained from rockets which are mostly based on the datasonde system throughout the decade 1969-1978.
      
The first planetary missions were based on conventional trajectories obtained with chemical engine rockets.
      
During the perihelion period NASA mounted a successful campaign of four sounding rockets that were launched at the White Sands Missile Range, New Mexico, between March 25 and April 8, 1997.
      
Many of the movies present thoughtful details regarding the actual space travel (rockets), but none of the movies discussed here is entirely realistic in its portrayal of the lunar surface.
      
The protected area was covered with a sufficientnumber of hail suppression rockets, rockets launching was permitted across theSlovenian border aimed at early seeding, and Slovenia in that time had also theoperative hail suppression system.
      
The domestic and foreign literature on microbiological studies in outer space from 1935 through 1970 is reviewed, with separate references to results obtained with balloons, high-altitude rockets and artificial earth satellites.
      
Fungi and Actinomycetes, aside from other microorganisms, have been placed aboard balloons, earth satellites, or high altitude sounding rockets for evaluation of environmental conditions of spaceflight missions.
      
Pinhole camera instrumentation has been carried on stabilized Skylark rockets to record images of the sun at extreme ultraviolet wavelengths.
      
The spectrum of the solar limb has been recorded in the wavelength region 300-2803 ? using instrumentation carried in 'Skylark' rockets.
      
Intensity calibrated grazing incidence spectrographs have been flown on three Skylark sounding rockets to record the solar soft X-ray and XUV spectra over a wide wavelength range.
      
An echelle grating spectrograph has been flown in Skylark sounding rockets to investigate the solar ultraviolet spectrum.
      
The derived solar image compares reasonably well with the EUV and X-ray pictures of the Sun obtained from rockets.
      
The primary data used for this work consisted of X-ray and XUV solar images obtained from rockets.
      
The photographs were taken on 11 March, 1971, and on 2 March, 1972, with Fresnel zone plate cameras which were flown on ESRO and NRL sounding rockets.
      
The data base for this study is the interplanetary plasma/magnetic field data compilation made available by the NSSDC/WDC-A for rockets and satellites (NASA/GSFC-Greenbelt).
      
Topics covered are line identifications, intensities, the continuum and its origin, the sun's surface in Lyman alpha, the profiles of H and K of Mg II, Lyman alpha and beta, and monitoring work conducted from rockets and satellites, including OSO-I.
      
Such conditions are realized during the motion of artificial satellites or space rockets through the ionosphere, or through the interplanetary medium in the immediate neighborhood of the earth.
      
Some results obtained from the study of cosmic rays and radiation belts with Soviet satellites and space rockets
      
This report estimates the amounts of various constituents that would have to be continually injected by rockets into the upper atmosphere in order to double the worldwide natural concentrations there.
      
 

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