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Pioneer 11

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HELIUM VECTOR MAGNETOMETER
HVM



Instrument Overview
===================
Magnetic fields affect the plasma of electrically charged particles in interplanetary space and control the flow of this plasma as it spreads out from the Sun across the orbits of the planets. Before the mission of Pioneer 10 these effects had been only observed and measured out to the orbit of Mars. Scientists were still uncertain about many specific details about the interplanetary medium and particularly the extent to which the Sun's magnetic field controlled the flow of plasma beyond Mars to the outer regions of the Solar System. The outer boundaries of this influence were vague, and interactions between the plasma and fields of the Solar System and those of the Galactic System puzzled scientists. Pioneer 10 and Pioneer 11 explored the regions beyond the orbit of Jupiter and made measurements that helped to define the transition region of solarinfluence (heliosphere).

This experiment used a sensitive magnetometer at the tip of a lightweight boom, which extended 6.6 meters from the center of the spacecraft to reduce the effects of the residual spacecraft magneticfield, and to assist the balance of this spin stabilized spacecraft.
The helium vector magnetometer measured the fine structure of the interplanetary field, maped the Jovian field, and provided field measurements to evaluate solar wind interaction with Jupiter. The magnetometer operated in one of eight different ranges, the lowest of which covered magnetic fields from +/-0.01 to +/-4.0 gamma; the highest, fields up to +/-140,000 gamma (i.e. +/-l.4 Gauss). The ranges were selected by ground command or automatically by theinstrument itself as it reached the limits of a given range.
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Pioneer 11



Instrument Overview
===================
Magnetic fields affect the plasma of electrically charged particles in interplanetary space and control the flow of this plasma as it spreads out from the Sun across the orbits of the planets. Before the mission of Pioneer 10 these effects had been only observed and measured out to the orbit of Mars. Scientists were still uncertain about many specific details about the interplanetary medium and particularly the extent to which the Sun's magnetic field controlled the flow of plasma beyond Mars to the outer regions of the Solar System. The outer boundaries of this influence were vague, and interactions between the plasma and fields of the Solar System and those of the Galactic System puzzled scientists. Pioneer 10 and Pioneer 11 explored the regions beyond the orbit of Jupiter and made measurements that helped to define the transition region of solarinfluence (heliosphere).

This experiment used a sensitive magnetometer at the tip of a lightweight boom, which extended 6.6 meters from the center of the spacecraft to reduce the effects of the residual spacecraft magneticfield, and to assist the balance of this spin stabilized spacecraft.
The helium vector magnetometer measured the fine structure of the interplanetary field, maped the Jovian field, and provided field measurements to evaluate solar wind interaction with Jupiter. The magnetometer operated in one of eight different ranges, the lowest of which covered magnetic fields from +/-0.01 to +/-4.0 gamma; the highest, fields up to +/-140,000 gamma (i.e. +/-l.4 Gauss). The ranges were selected by ground command or automatically by theinstrument itself as it reached the limits of a given range.

The sensor for the magnetometer consisted of a cell filled with helium that is excited by electrical discharge at radio frequencies and infrared optical pumping. Changes in helium absorption caused by magnetic fields passing through the magnetometer are measured by aninfrared optical detector.

['Instrument Overview' was adapted from FIMMELETAL pp. 49-50.]

The Planetary Plasma Interactions (PPI) Node of the Planetary Data System (PDS)





External Reference

 
  • Fimmel, R.O., W. Swindell, E. Burgess, Pioneer Odyssey, NASA SP-396, Scientific and Technical Information Office, National Aeronautics and Space Administration, Washington, D.C., 1977.
  • Smith, E.J., L. Davis, Jr., D.E. Jones, P.J. Coleman, Jr., D.S. Colburn, P. Dyal, C.P. Sonett, and A.M.A. Frandsen, The planetary magnetic field and magetosphere of Jupiter: Pioneer 10, J. Geophys. Res., 79, 3501, 1974B.
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