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arXiv · 1204.0943

Observations of Low Frequency Solar Radio Bursts from the Rosse Solar-Terrestrial Observatory

P. Zucca·E. P. Carley·J. McCauley·P. T. Gallagher·C. Monstein·R. T. J. McAteer
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Abstract

The Rosse Solar-Terrestrial Observatory (RSTO; www.rosseobservatory.ie) was established at Birr Castle, Co. Offaly, Ireland (53 05'38.9", 7 55'12.7") in 2010 to study solar radio bursts and the response of the Earth's ionosphere and geomagnetic field. To date, three Compound Astronomical Low-cost Low-frequency Instrument for Spectroscopy and Transportable Observatory (CALLISTO) spectrometers have been installed, with the capability of observing in the frequency range 10-870 MHz. The receivers are fed simultaneously by biconical and log-periodic antennas. Nominally, frequency spectra in the range 10-400 MHz are obtained with 4 sweeps per second over 600 channels. Here, we describe the RSTO solar radio spectrometer set-up, and present dynamic spectra of a sample of Type II, III and IV radio bursts. In particular, we describe fine-scale structure observed in Type II bursts, including band splitting and rapidly varying herringbone features.

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P. Zucca, E. P. Carley, J. McCauley, P. T. Gallagher, C. Monstein, R. T. J. McAteer. 2012-04-04. Observations of Low Frequency Solar Radio Bursts from the Rosse Solar-Terrestrial Observatory. https://doi.org/10.1007/s11207-012-9992-x

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