Rocket measurements of S sub q currents at midlatitude.
Midlatitude ionospheric currents detected by rocketborne rubidium vapor magnetometers in Nike- Apache rockets
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Midlatitude ionospheric currents detected by rocketborne rubidium vapor magnetometers in Nike- Apache rockets
Chemical composition and origin of moldavites, noting densities, refractive indices, oxide content, rubidium-strontium ratio, etc
Filling and covering for potassium, rubidium, and cesium vapor absorption chambers of radiooptical resonance magnetometers
Root-mean-square differences between measured magnetic field values obtained by rubidium vapor magnetometer aboard OGO-2 satellite and values derived from spherical harmonic expansions
Rocket borne rubidium magnetometer measurements for latitude determination of equatorial electrojet
Geomagnetic field values obtained from OGO-2 SATELLITE-MOUNTED rubidium vapor magnetometer
Electromagnetic interactions in hyperfine structure of vibrational and rotational states in rubidium and potassium /isotopes/ fluorides, using electric resonance method
Analog and digital circuits, optical package, and power supply of rubidium atomic time and frequency reference system for manned spacecraft
Rubidium-strontium isotope measurements of Lemumbo igneous monocline associated acid and basic rocks to determine earth mantle or crust origin
Salts of heptavalent bromine were synthesized by a hot atom process, the beta decay of radioactive selenium-83 incorporated into a selenate. Formation of an unreactive perbromate ion led to preparation of macro amounts of perborate. A rubidium salt was isolated.
Microwave frequency probes of ionized helium, rubidium lasers, cesium spectrum, and ruby crystals
Magnetometers of rubidium vapor for space measurement on OGO-E
Magnetospheric field distortions observed from rubidium magnetometer measurements on OGO 3 and 5
OGO-2 rubidium vapor magnetometer measurements comparison with surface magnetic observatory data during geomagnetic storms, considering asymmetric ring current
Electrojet currents association with visible aurorae, using sounding rockets with rubidium vapor magnetometers
The Alouette 2 resonances observed near the harmonics of the electron cyclotron frequency f sub H reveal frequency shifts (relative to the n(f sub H) values derived from model field calculations) which can be interpreted in terms of plasma wave dispersion effects. These effects are observed on the 2(f sub H) resonance when it is near the resonance observed close to the upper hybrid frequency f sub T. The observations suggest that an oblique echo model may be required to give a proper interpretation of the 2(f sub H) resonance. Cyclotron damping can be ignored only when the angle between the propagation vector and the direction perpendicular to the earth's magnetic field B is less than a few degrees for the 2(f sub H) wave, and less than a few tenths of a degree for the n(f sub H) waves with n 2. The negative offset of the absolute value of B inferred from the plasma resonance observations is consistent with expectations based on recent OGO 3 and OGO 5 rubidium magnetometer observations at higher altitudes in the equatorial regions.
Results are presented of computer calculations on the relativistic time corrections relative to a ground-based clock of on-board clock readings for a lunar mission, using simple Newtonian gravitational potentials of earth and moon and based on actual trajectory data for Apollo 12 and Apollo 13. Although the second order Doppler effect and the gravitational red shift give rise to corrections of opposite sign, the net accumulated time corrections, namely a gain of 560 (+ or - 1.5) microseconds for Apollo 12 and gain of 326 (+ or - 1.3) microseconds for Apollo 13, are still large enough that with present day atomic frequency standards, such as the rubidium clock, they can be measured with an accuracy of about + or - 0.5 percent.
The rubidium vapor magnetometer data of the scalar magnetic-field intensity obtained by the OGO 3 and 5 satellites are analyzed to study the magnetospheric-field distortions in terms of the observed field magnitude under quiet and slightly disturbed conditions minus the magnitude of the reference geomagnetic field (delta B). Average contours of equal delta Bs are shown in the geomagnetic noon-midnight and dawn-dusk meridian planes for magnetically quiet and slightly disturbed conditions. The equatorial distribution of observed delta Bs as a function of geocentric distance differs substantially from that expected from the well-known models of the quiet-time ring current. Other findings suggest that there must be a population of low-energy particles with substantial total energy near the equator at distances of 2 to 5 earth radii that has not been recognized as having sufficient energy to inflate the magnetic field.