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Astronautical and Aeronautical Events of 1962 - NASA's History Office

Astronautical and Aeronautical Events of 1962 - NASA's History Office

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ASTRONAUTICAL AND AERONAUTICAL EVENTS OF <strong>1962</strong> 225<br />

production <strong>of</strong> nine live flight stages, one inert flight stage, <strong>and</strong><br />

several ground-test units for the Advanced Saturn vehicle.<br />

October SO: Oran W. Nicks, NASA Director <strong>of</strong> Lunar <strong>and</strong> Planetary<br />

Programs, summarized results obtained from MARINER 11 scientific<br />

experiments, at Eighth Tri-Service Conference on Electromagnetic<br />

Compatibility in Chicago: “One <strong>of</strong> the primary scientific objec-<br />

tives in measuring magnetic fields in interplanetary space is to<br />

determine the magnitude <strong>and</strong> direction <strong>of</strong> the steady field com-<br />

ponent. . . . The Mariner has indicated a typical steady<br />

state transverse component <strong>of</strong> ten gamma or less, <strong>and</strong> it has<br />

clearly shown how the transverse field becomes large (as high as<br />

25 gamma) during geomagnetic storms. In addition to this, the<br />

Mariner 2 has provided information on the steady interplanetary<br />

field indicating that the radial component is apparently more<br />

stable, even under storm conditions, <strong>and</strong> that there are quiet<br />

times when the radial component from the sun is essentially<br />

constant. . . . Measurements from the ion chamber [onboard<br />

MARINER 111 have indicated an average radiation level as expected,<br />

corresponding to about 1.1 milli-roentgen per hour (about 100<br />

times the cosmic ray intensity at the surface <strong>of</strong> the earth). . . .<br />

It has been reported by measurements [<strong>of</strong> the probe’s cosmic dust<br />

detector] thus far that the flux <strong>of</strong> interplanetary dust particles is<br />

at least one thous<strong>and</strong> times less in interplanetary space than in<br />

the near vicinity <strong>of</strong> the earth. The cause <strong>of</strong> this is unknown.<br />

. . . Preliminary data from the [solar plasma detector in the]<br />

Mariner indicate abrupt changes in the velocity <strong>and</strong> intensity <strong>of</strong><br />

solar winds, <strong>and</strong> correlated effects on the magnetic fields in space.<br />

Measurements show that the particle energies generally range<br />

from about 750 electron volts to 2500 electron volts, although<br />

some lasma with an energy <strong>of</strong> 3225 electron volts has been ob-<br />

serve2 These variations almost certainly were the results <strong>of</strong><br />

events on the sun, but the exact nature <strong>of</strong> these events is not yet<br />

understood. . . .<br />

9,<br />

0 NASA announced 19 experiments would be included on Pogo satellite<br />

(Polar Orbiting Geophysical Observatory) to be orbited by<br />

Thor-A ena vehicle launched from Pacific Missile Range. Pogo<br />

wouId %. e second in Ogo (Orbiting Geophysical Observatory)<br />

series <strong>and</strong> first Ogo in polar orbit; it was scheduled for launch in<br />

early 1964.<br />

October $1: Sudden drop in voltage on MARINER 11 Venus probe was<br />

reported by Jet Propulsion Laboratory scientists. JPL turned <strong>of</strong>f<br />

the probe’s four interplanetary experiments to conserve on-board<br />

power for experiments in the vicinity <strong>of</strong> Venus. Discounting<br />

any probability <strong>of</strong> the solar cells being affected by radiation,<br />

e erts indicated the problem could have come from faulty<br />

vo 7l tage regulators.<br />

ANNA IB geodetic satellite launched into orbit by Thor-Able-Star<br />

vehicle from Cape Canaveral (apogee, 727 mi.; perigee, 670 mi.;<br />

inclination, 50° to the equator). Mounted on the 350-lb.) 36-in.<br />

spherical satellite were four high-intensity lights that would<br />

flash on <strong>and</strong> <strong>of</strong>f; by comparing simultaneous observations <strong>of</strong> the<br />

satellite from various points on earth, scientists could measure<br />

earth’s size, shape, <strong>and</strong> surface features with accuracy never

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