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doc#119 | ideal gas is compressed and kept at constant | temperature | , the work done in compressing it is completely |
doc#118 | surrounding the anode holder to determine its | temperature | . </p><p> Another anode holder used in the |
doc#120 | which disappeared, due to broadening, at low | temperature | . The data reported here are either from |
doc#118 | measuring the characteristic anode surface | temperature | (see below) since only a small region of |
doc#118 | simultaneous measurement of the anode surface | temperature | and the temperature distribution along |
doc#118 | voltages. Simultaneously with the anode surface | temperature | and voltage measurements pyrometer readings |
doc#120 | resonance line which was very narrow at room | temperature | and which disappeared, due to broadening |
doc#117 | is a good approximation to the brightness | temperature | at the center of the lunar disk because |
doc#117 | 600° K. This result suggests a very high | temperature | at the solid surface of the planet, although |
doc#117 | would increase the average disk brightness | temperature | by less than 1° K. At meter wave lengths |
doc#117 | known. The ratio of the measured antenna | temperature | change during a drift scan across the moon |
doc#117 | , and Salomonovich, 1960). The constant- | temperature | contours are much smoother than those observed |
doc#117 | black body, will the apparent black-body | temperature | correspond to the physical temperature |
doc#122 | reaction cells sealed from the same manifold | temperature | dependency corresponding to activation |
doc#118 | all blowing rates, assuming <formul>. The | temperature | dependent value of <egr> was taken from |
doc#118 | of the anode surface temperature and the | temperature | distribution along the anode holder. Three |
doc#118 | in figure 4 was taken as typical for the | temperature | distribution for all blowing rates. </p> |
doc#118 | the plug holder is thereby <formul> The | temperature | distribution of figure 4 gives <formul> |
doc#117 | the narrow antenna beam and because the | temperature | distribution over the central portion of |
doc#125 | blood group antibodies. These include low- | temperature | ethanol (Cohn) fractionation, electrophoresis |