Characteristics of the Spacecraft Local Environment During NSTAR Ion Propulsion System Operations on Deep Space One
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Engineering topics
Publications and source records attributed to Glassmeier, K..
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This paper describes a small-weight and low-power magnetometer that was designed and built for the Mars '94 mission.
The existence of hydromagnetic waves in the mass-loaded solar wind upstream from the bow shock of a comet is well-established both for comet Giacobini-Zinner and for comet Halley. Whereas previous reports have been concerned either with the magnetic field observations or with plasma observations, here observations of the magnetic field with the solar wind proton and alpha particle distributions are combined. This allows the three possible modes of propagation for these waves to be separated. The magnetic component is predominantly transverse to the magnetic field and linearly polarized. The flow vector also has a substantial amount of power parallel to the magnetic field. An examination of the pressure variations shows that slow magnetosonic waves are more common than the fast mode.