Magnetic effects of the quiet time proton belt
Explorer xii proton detector analysis of magnetic effects of quiet time proton belt
MAGNETIC EFFECT↗
Engineering topics
Hoffman, R. A.
Publications and source records attributed to Hoffman, R. A..
Magnetic effects of the quiet time proton belt
Magnetic effects of quiet time proton belt using data obtained from proton detector aboard Explorer XII satellite
MAGNETIC EFFECT↗
Comparison of the total cosmic radiation in deep space and at the earth during the March- April 1960 events.
Total radiation intensity in interplanetary space before and after solar events of March 29 and April 9, 1960
SOLAR RADIATION↗
PROTONS FROM 0.1 TO 5 MEV AND ELECTRONS OF 20 KEV AT 12 EARTH RADII DURING THE SUDDEN COMMENCEMENT ON SEPTEMBER 30, 1961
Explorer xii ion-electron detection in magnetic storm sudden commencement on sept 30 1961 - 0.1 to 5 mev protons & 20 kev electrons at 12 earth radii
SUDDEN IONOSPHERIC DISTURBANCE /SID/↗
PROTONS OF 0.1 TO 5 MEV AND ELECTRONS OF 20 KEV AT 12 EARTH RADII DURING SUDDEN COMMENCEMENT ON SEPTEMBER 30, 1961
Time and angular variations of particles during solar magnetic storm at 12 earth radii distance, all data was obtained from explorer 12 satellite
SOLAR PROTON↗
OBSERVATIONS OF THE VAN ALLEN RADIATION REGIONS DURING AUGUST AND SEPTEMBER 1959. 6. PROPERTIES OF THE OUTER REGION
Van allen belt in august and september 1959 - properties of outer belt measured by explorer vi
EXPLORER VI SATELLITE↗
OBSERVATIONS OF THE VAN ALLEN RADIATION REGIONS DURING AUGUST AND SEPTEMBER 1959. VI - PROPERTIES OF THE OUTER REGION
Properties and observation of the van allen radiation belt
GEOMAGNETIC FIELD↗
OBSERVATIONS OF THE VAN ALLEN RADIATION REGIONS DURING AUGUST AND SEPTEMBER 1959 5. VISUAL AURORAS, HIGH-ALTITUDE X-RAY BURSTS, AND SIMULTANEOUS SATELLITE OBSERVATIONS
Correlation of variations of explorer vi count rates with simultaneous visual auroras and high- altitude x-ray bursts
EXPLORER VI SATELLITE↗
OBSERVATION OF THE VAN ALLEN RADIATION REGIONS DURING AUGUST AND SEPTEMBER, 1959. 4. THE OUTER-ZONE ELECTRONS
Van allen zone - outer-zone electrons
ELECTRON↗
OBSERVATION OF THE VAN ALLEN RADIATION REGIONS DURING AUGUST AND SEPTEMBER, 1959 4. THE OUTER-ZONE ELECTRONS
Study of energy radiation in outer van allen zone from explorer vi satellite data acquisition during august and september 1959
EXPLORER VI SATELLITE↗
OBSERVATIONS OF THE VAN ALLEN RADIATION REGIONS DURING AUGUST AND SEPTEMBER 1959. 3. THE INNER BELT
Van allen belt - inner belt radiation data from ion chamber and geiger counter aboard explorer vi satellite
ION CHAMBER↗
OBSERVATIONS OF THE VAN ALLEN RADIATION REGIONS DURING AUGUST AND SEPTEMBER 1959. 2. THE CAPETOWN ANOMALY AND THE SHAPE OF THE OUTER BELT
Lack of influence of capetown gravity anomaly on van allen radiation belt
RADIATION BELT↗
SOLAR COSMIC RAYS AND SOFT RADIATION OBSERVED AT 5,000,000 KILOMETERS FROM EARTH
Explore the source record for details and available documents.
Arnoldy, R. L.↗
Solar Cosmic Rays and Soft Radiation Observed at 5,000,000 Km from Earth
No abstract available
Arnoldy, R. L.↗
Observations of the Van Allen Radiation Regions During August and September 1959
An integrating ionization chamber and a single Geiger counter were flown on United States satellite Explorer VI in an elliptical orbit extending to 48,000 km. In addition to the Van Allen inner zone and the great outer zone, a stable and distinct intermediate zone was detected throughout August and September 1959. The outer-zone intensity showed a large decrease following the sudden commencement of a geomagnetic storm. Later in the storm the outer zone increased to much in excess of its prestorm level. During stable periods the outer zone was fairly constant and less intense than it had been observed to be with Pioneer III or Pioneer IV or the first Soviet cosmic rocket. Cosmic-ray background counting rates were reached on most passes in August and Septmeber near apogee of the satellite. The radiation ?dumped? from the outer zone during the geomagnetic storm fits very well with the intensity and latitude distribution required to account for balloon observations of auroral X rays made during the IGY period. This paper is based on preliminary analysis of Explorer VI data.
Arnoldy, R. L.↗