Abstract
The principles of space-based low-frequency radio astronomy are briefly introduced. As the wavelength range considered does not allow the use of focusing systems, goniopolarimetric (or “direction-finding”) techniques have been developed. These techniques are presented, and their limitations are discussed. An example from a recent study on auroral radio emissions at Saturn from Cassini/RPWS measurements illustrates the techniques.
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Notes
- 1.
This wavelength range is called the short antenna or quasistatic range.
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Acknowledgements
The author wants to thank L. Lamy, R. Prangé and P. Zarka for their helpful discussion during the preparation of the manuscript. He also wants to thank Martin C.E. Huber (advised by M. Pick) for soliciting him to write this chapter.Part of this chapter is based on a presentation “Space-based Radio Measurements: Goniopolarimetry” given at the thirtieth Goutelas Spring school: “Low Frequency Radioastronomy: Instrumentation, Science, Projects”, Marcoux, France, June 2007 (Cecconi 2011).
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Cecconi, B. (2013). Goniopolarimetric techniques for low-frequency radio astronomy in space. In: Huber, M.C.E., Pauluhn, A., Culhane, J.L., Timothy, J.G., Wilhelm, K., Zehnder, A. (eds) Observing Photons in Space. ISSI Scientific Report Series, vol 9. Springer, New York, NY. https://doi.org/10.1007/978-1-4614-7804-1_15
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