1. OLFAR - orbiting low frequency array; using a satellite swarm for building a space-based radio telescope for low frequencies
- Author
-
Bentum, Marinus Jan, Boonstra, A.J., Verhoeven, C.J.M., van der Veen, A.J., Gill, E.K.A., Saks, N., Falcke, H., Klein-Wolt, M., Rajan, R.T., Rajan, Raj, Wijnholds, S.J., Arts, M., van 't Klooster, K., Beliën, F., Meijerink, Arjan, Monna, B., Rotteveel, J., Boer, M.A., Bongers, E., Boom, E., van Tuijl, Adrianus Johannes Maria, and van Staveren, A.
- Subjects
small satellites ,EWI-19103 ,Astrophysics::High Energy Astrophysical Phenomena ,IR-75278 ,METIS-276738 ,Astrophysics::Instrumentation and Methods for Astrophysics ,Astrophysics::Cosmology and Extragalactic Astrophysics ,Radio astronomy ,low-frequency astronomy ,phased array signal processing ,satellite swarms - Abstract
In radio astronomy, as in astronomy in general, a wide range of frequencies is observed as each spectral band offers a unique window to study astrophysical phenomena. In the recent years, new observatories have been designed and built at the extreme limits of the radio spectrum. For the low frequencies several Earth-based radio telescopes are constructed at this moment. In the Netherlands, the Low Frequency Array (LOFAR) is being constructed at this moment and will be operational later this year. LOFAR observes the sky between 30 and 240 MHz. Observing at even lower frequencies is very interesting, but, due to the influence of the Earth’s ionosphere this is not possible from Earth. Thus, the only option to observe low frequencies is a telescope in space.
- Published
- 2010