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e of Physics
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Astrophysics Research

Intraday Variability

UTAS People Involved
The brightness of stars varies as we look at them (they twinkle) because turbulence in Earth's atmosphere acts like many small lenses, sometimes bending the stars light away from us and sometimes towards us.  "Stars twinkle, but planets don't" is a well known phrase.  The planets don't twinkle because they are much closer and their size is larger than the size of the turbulent patches in the Earth's atmosphere.

The space between the stars is often thought of as being empty, but it isn't.  On average there is 1 atom per cubic centimetre and this is the galaxy's atmosphere (called the interstellar medium).  The interstellar medium is also turbulent and affects radio waves in much the same way that the Earth's atmosphere affects light waves and causes some to radio sources to twinkle (called scintillation).  Only the smallest radio sources scintillate, pulsars in our Galaxy and some distant quasars.  The scintillation causes the intensity of these distant quasars to vary on a timescale of hours to days.  The timescale is determined by both the structure of the quasar and the properties of the interstellar medium in the direction of the quasar.

A quasar produces 100's of times more energy than our entire galaxy, from a region about the size of our solar system.  They are powered by stars, gas and dust being drawn into giant blackholes with masses millions of times that of our Sun.  However, all quasars are a very long way away, the nearest is more than 800 million light-years away, their size is about one millionth of an arcsecond.  To put this in perspective, one millionth of an arcsecond is the size of a pinhead on the Moon as seen from the Earth.  Studying the variations of quasars produced by scintillation is the only method we have for studying quasars in such fine detail. 

As part of a project funded by the Australian Research Council, a team consisting of astronomers from the University of Tasmania and the Australia Telescope National Facility have been using the Ceduna radio telescope since March 2003 to continuously monitor a small number of distant quasars.  This unique experiment has already yielded a number of surprises, including sudden changes in the size and timescale of scintillation in some sources and the presence of multiple timescales in others.  One indication of the success of this project is that groups in the USA and Japan are in the process of setting up copy-cat experiments.

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Dr Simon Ellingsen
Simon Picture



Prof Peter McCulloch
Steve Carter

Collaborators
Dave Jauncey (ATNF)
Lucyna Kedziora-Chudczer (Sydney)
Hayley Bignal (JIVE)
J-P. Macquart (NRAO/Caltech)
Created: September 2009 by Tammy Riley
Last modified: September 2009
Copyright School of Mathematics & Physics, University of Tasmania Australia, 2009