Ørsted is an Earth science satellite launched in 1999 to study the earth's geomagnetic field. It is Denmark's first satellite, named after Hans Christian Ørsted (1777–1851), a Danish physicist and professor at the University of Copenhagen, who discovered electromagnetism in 1820.
The spacecraft's primary science objectives are to perform highly accurate and sensitive measurements of the geomagnetic field and to perform global monitoring of the high energy charged particle environment.
The instrumentation consisted of two magnetometers (proton precession and fluxgate), a star imager for attitude determination, a solid-state charged particle detector package, and a GPS receiver. The Science Instrument Team is responsible for the design of the instruments, while the Science Team is responsible for the science mission planning and international science participation. The science data obtained during the planned one-year mission will be used to derive an updated model of the geomagnetic field and its secular variation and to study the magnetospheric field-aligned currents and their relationship to ionospheric and solar wind conditions.
The principal research topics are in two areas: 1° studies of the generation of the magnetic field in the fluid core and the magnetic and electrical properties of the solid Earth; and 2° studies of Earth's magnetic field as the controlling parameter of the magnetosphere and of all the physical processes that take place in the Earth's plasma environment, including phenomena like aurora and magnetic storms.
The primary scientific instruments on the Ørsted satellite are:
An Overhauser Effect Scalar Magnetometer provides extremely accurate measurements of the strength of the geomagnetic field. The Overhauser magnetometer is situated at the end of an 8 meter long boom, in order to minimize disturbances from the satellite's electrical systems.
A Compact Spherical Coil (CSC) Fluxgate Vector Magnetometer, used to measure the strength and direction of the geomagnetic field.
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