Abstract
In radio astronomy, as in astronomy in general, a wide range of frequencies is observed as each spectral band o_ers 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 inuence of the Earth's ionosphere this is not possible from Earth. Thus, the only option to observe low frequencies is a telescope in space
Original language | English |
---|---|
Title of host publication | 38th COSPAR Scientific Assembly |
Place of Publication | Bremen |
Publisher | Committee on Space Research (Cospar) |
Pages | 1-2 |
Number of pages | 2 |
Publication status | Published - 21 Jul 2010 |
Event | 38th Scientific Assembly of the Committee on Space Research, COSPAR 2010 - Bremen, Germany Duration: 18 Jul 2010 → 25 Jul 2010 Conference number: 38 http://cospar2010.zarm.uni-bremen.de/ |
Conference
Conference | 38th Scientific Assembly of the Committee on Space Research, COSPAR 2010 |
---|---|
Abbreviated title | COSPAR |
Country/Territory | Germany |
City | Bremen |
Period | 18/07/10 → 25/07/10 |
Internet address |