LOFAR - A European VLBI-array for radio astronomy
O. Wucknitz [1]
- Argelander-Institut für Astronomie, Auf dem Hügel 71, 53121 Bonn, Germany
Abstract
The LOw Frequency ARray (LOFAR) is a new radio interferometry array that
is currently being completed in the Netherlands and a couple of other
countries. LOFAR covers the frequency range 10-270 MHz in which radio
astronomy has started but which has been largely neglected since then. The
stations outside of the Netherlands (currently four of them in Germany)
are particularly important to reach sub-arcsec resolution and turn LOFAR
into a true VLBI array.
This talk gives an introduction into the principles of radio
interferometry and LOFAR and shows some early successes with an emphasis
on long-baseline, high-resolution work. LOFAR has already produced the
first ever high-resolution images of the sky at wavelengths of several
metres.
download original presentation
PDF file (6.6 MB, last change 12 Sep 2010)
75 pages (including 17 with supplementary material), suitable for presentation with acroread. This version also includes some hyperlinks for quick navigation and links to references.
download printable version (small)
PDF file (4.6 MB, last change 12 Sep 2010)
Paper saving version. 9 pages, text in b/w, colour figures. 8 slides per A4 page.
download movie 1: ionospheric TEC movie
GIF file (982.6 kB, last change 1 Dec 2006)
download movie 2: single-band delay/rate 3C196 20 Aug 2009, DE-NL
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download movie 3: the Sun with 1 sec integration time per step, real duration 30
sec, about 10:17:10 - 10:17:40 on 9-Jun-2010, plays in real-time
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download movie 4: incoherent all-band delay/rate 3C48 NL-NL with CygA+CasA
GIF file (21.3 MB, last change 29 Sep 2009)
download movie 5: the Sun with 10 sec integration time per step, real duration ca. 10
min, about 10:16:30 - 10:26:20 on 9-Jun-2010, plays 100 times
faster than real-time
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Script last modified on 7 Sep 2010
Last change to this data base entry on 12 Sep 2010