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A Study Of Atmospheric Ozone Near The Surface Of The Earth, Irby Gerald Bowen
A Study Of Atmospheric Ozone Near The Surface Of The Earth, Irby Gerald Bowen
Physics & Astronomy ETDs
It is the primary purpose of this thesis to describe the method used for measuring ozone at the earth’s surface. There is also a report on a brief series of surface ozone measurements. An attempt is made at a preliminary explanation on the basis of meteorological conditions of the diurnal variations which were found.
A New Method Of Measuring The Intensity Of The Zodiacal Light, Raymond Grenchik
A New Method Of Measuring The Intensity Of The Zodiacal Light, Raymond Grenchik
Physics & Astronomy ETDs
The two theories that have been presented for the zodiacal light show that it is due to light scattered (and perhaps emitted) from an extensive lenticular cloud of particles lying in the plane of the ecliptic. The basic difference of the two theories is the position of the center of this cloud. One, the planetary theory, places the sun at the center of this cloud. The other, the atmospheric theory, places the earth at the center of the cloud.
A Nuclear Magnetic Resonance Absorption Experiment, Richard Runge
A Nuclear Magnetic Resonance Absorption Experiment, Richard Runge
Physics & Astronomy ETDs
In nuclear magnetic resonance absorption work, the detection of the absorption of energy by protons situated in a steady strong magnetic field and subject to a weak radiofrequency (RF) magnetic field is attempted. The protons are present in a sample placed inside an RF coil. A radiofrequency current, present in this coil, produces a rapidly oscillating magnetic field which is capable of supplying energy to the system of protons in the steady strong magnetic field. This absorption of energy by the protons alters their relative numerical distribution among the energy levels available to them.
A Cosmic Ray Experiment Using Nuclear Photographic Emulsions, Mercedes Merner
A Cosmic Ray Experiment Using Nuclear Photographic Emulsions, Mercedes Merner
Physics & Astronomy ETDs
A "camera" containing thirty-six nuclear plates was carried into the upper atmosphere to an altitude of twelve miles by a free balloon flight. These plates were arranged in four groups separated by successively thicker layers of steel so that nuclear events under different amounts of matter could be observed.
After recovery of the equipment these plates were developed and examined under the microscope. Four plates were selected for intensive investigation, and data was collected on the tracks found in the areas examined.
In the first part of this report nuclear plate technique will be discussed in general together with the …