Susanne
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doc#117 procedures or made the same assumptions about the lunar brightness distribution when
doc#117 diameter with a resultant beam width of only about 2<prime> (Amenitskii, Noskova, and Salomonovich
doc#117 intensity diameter of the antenna beam was about 9<prime>, and the angle subtended by the
doc#117 Research Laboratory. The age of the moon was about 2 days. The half-intensity diameter of
doc#117 diameter of the main lobe of the antenna was about 18<prime>.5, and the brightness temperature
doc#120 symmetric when the <formul> bond length is about 2.4 to 2.5 A, but aside from the possible
doc#120 expected limits and the volume per oxygen is about normal. However, the possible absence of
doc#120 Dr. Douglass was kind enough to lend us about 5 grams of his material. This material
doc#120 for 48 hours. A very fine, gray solid ( about 15 g) is formed, water-washed by centrifugation
doc#120 be composed of nearly isotropic particles about 0.3<mgr> in diameter. The particles appeared
doc#120 the resonance line, defined as the field about which the first moment is zero. </p><p> Second
doc#120 The temperature was maintained to within about <formul> for the period of time required
doc#120 required to make the measurement (usually about one hour). One sample, which had been exposed
doc#120 showed the presence of adsorbed water ( about 0.3 wt %) as evidenced by a weak resonance
doc#120 powder density of the <formul> used here was about <formul>, approximately one-third that
doc#120 corresponds to a paramagnetic ion density of about <formul>. </p><p> Spectra were obtained from
doc#121 formulations based on nonionic actives with about the same amount of phosphate builder; light
doc#122 appears possible to set a lower limit of about <formul> for the activation energy of the
doc#122 <formul> and <formul> and illuminated for about 50 hours with a 1000 watt tungsten lamp
doc#122 Pyrex capillary tubing 2.5 mm. i.d. and about 15 cm. long. In a few experiments the tubes