SPEX (astronomy)

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The SPEX (Spectropolarimeter for Planetary Exploration) is a single-channel, high-precision polarimeter for the characterization of planetary atmospheres. [1] It is intended for planetary science missions, but it could, with minor modifications, also be used for Earth observation by a microsatellite, such as the Dutch FAST-D project. [2]

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References

Cross-reference

  1. SRON 2011.
  2. Maessen et al. 2010, p. 160.

Sources used

  • "SPEX Spectropolarimeter for Planetary EXploration". Netherlands Institute for Space Research. 2011.
  • Maessen, D.C.; Guo, J.; Gill, E.; Gunter, B.; Chu, Q.P.; Bakker, G.; Laan, E.; Moon, S.; Kruijff, M.; Zheng, G.T. (2009). "Conceptual Design of the FAST-D Formation Flying Spacecraft". In Sandau, Rainer; Roeser, Hans-Peter; Valenzuela, Arnoldo (eds.). Small Satellites for Earth Observation: 7th International Symposium of the International Academy of Astronautics (IAA), 4–8 May 2009, Berlin, Germany (2010 ed.). Springer. ISBN   9783642035005. uuid: 23f6c40a-5756-4a46-bc3e-ee8727c9806a.

Further reading