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Lunar surface magnetometersDiscussion of the properties of both the stationary and portable magnetometers used in the Apollo program to measure static and dynamic fields on the lunar surface. A stationary magnetometer is described in which the three orthogonal vector components of the magnetic field are measured by three fluxgate sensors which are located at the ends of three orthogonal booms and contain ferromagnetic cores driven to saturation by means of a periodic current. In the Apollo 16 magnetometer special high-stability ring-core sensors were used which provided an output voltage to the analog-to-digital converter which is proportional to the magnetic field. A portable magnetometer is described which consists of a set of three orthogonal fluxgate sensors mounted on top of a tripod connected to an electronics box by a ribbon cable. The above-mentioned stationary magnetometer simultaneously measured the time-varying components of the field which were later subtracted from the portable magnetometer measurements to give the desired resultant steady field values caused by the magnetized crustal material.
Document ID
19740027256
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Dyal, P.
(NASA Ames Research Center Space Sciences Div., Moffett Field, Calif., United States)
Gordon, D. I.
(U.S. Navy, Naval Ordnance Laboratory, Silver Spring Md., United States)
Date Acquired
August 7, 2013
Publication Date
September 1, 1973
Subject Category
Instrumentation And Photography
Accession Number
74A10006
Distribution Limits
Public
Copyright
Other

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