Time of firing: 1000 MST
Agency: Applied Physics Laboratory, Johns Hopkins
University
Altitude: 62.5 miles
UPPER AIR INSTRUMENTS
Composition: One air-sample bottle (Signal Corps,
Mich. U.)
Cosmic radiation: Three arrays of three Geiger tubes
each surrounded by various
thicknesses of aluminum.
Single pulse ionization chamber in nose extension.
Fourfold Geiger tube specific
ionization telescope (APL).
Solar radiation: Two thermoluminescent detectors
(NRL)
High altitude photography: Three K-25 cameras with
black and white, infrared, and
aero kodacolor film
Biological experiment: Fruit flies
DATA RECOVERY INSTRUMENTS
Telemeter: NRL telemetering
Physical recovery: Warhead blowoff by radio command
ROCKET INFORMATION
Unfueled rocket weight: 9652 lb
Gross weight at takeoff: 29,217 lb
ROCKET PERFORMANCE
Program angle: Seven degrees
Time to burnout: 63.5 sec.
Velocity at burnout: 4440 ft/sec
Altitude at burnout: 20.6 miles
Time to zenith: 205 sec.
Altitude to zenith: 79.5 miles
Time to tail blowoff: 321.2 sec
Altitude at tail blowoff: 39.1 miles
Flight duration: 568.5 sec
Impact Coordinates: 37.4 mi. north, 1.4 mi east
BALLISTIC INSTRUMENTS
Theodolites: Mitchell - good images from 0 to 70
sec; Askania - data reduced from
0 to 75 sec
Cameras: Bowen-Knapp - operations satisfactory;
ballistic - satisfactory some
images obscured by vapor
trail
Telescopes: Good operation
Radar: To 568 sec
DATA RECOVERY
Physical recovery: Air-sampling bottle punctured
by fragment. All cameras
recovered. Thermoluminescent
detectors recovered, one operated
satisfactorily.
COMMENTS
Rocket performance: Roll rate - 1 Rev/10.9 sec at
70 sec, 1 Rev/10.2 sec at 107 sec
Other: Impact predictor operated
REPORTS AND PAPERS
"The Specific Ionization of the Cosmic Radiation
Above the Atmosphere," S. F.
Singer, Phys. Rev. 76:701
(1949)
"The Zenith Angle Dependence of the Cosmic Radiation
Above the Atmosphere at
lambda = 41°N," S. F.
Singer, Phys. rev. 77:729 (1950)
"On the Nature of the Cosmic Radiation Near the
Pfotzer Maximum at lambda = 41°N,"
S. F. Singer, Phys. Rev.
77:730 (1950)