Skip to main content
Log in

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

  • ADVANCES IN EUROPEAN SOLAR PHYSICS
  • Published:
Solar Physics Aims and scope Submit manuscript

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 in Transportable Observatory (CALLISTO) spectrometers have been installed, with the capability of observing in the frequency range of 10 – 870 MHz. The receivers are fed simultaneously by biconical and log-periodic antennas. Nominally, frequency spectra in the range of 10 – 400 MHz are obtained with four sweeps per second over 600 channels. Here, we describe the RSTO solar radio spectrometer set-up, and present dynamic spectra of samples of type II, III and IV radio bursts. In particular, we describe the fine-scale structure observed in type II bursts, including band splitting and rapidly varying herringbone features.

This is a preview of subscription content, log in via an institution to check access.

Access this article

Price excludes VAT (USA)
Tax calculation will be finalised during checkout.

Instant access to the full article PDF.

Figure 1
Figure 2
Figure 3
Figure 4
Figure 5
Figure 6
Figure 7
Figure 8

Similar content being viewed by others

Notes

  1. www.e-CALLISTO.org .

  2. soleil.i4ds.ch/solarradio/CALLISTOQuicklooks/ .

  3. www.rosseobservatory.ie/presentations/birr_radio_survey.pdf .

  4. www.lofar.ie .

References

  • Benz, A.O., Monstein, C., Meyer, H.: 2005, Callisto – a new concept for solar radio spectrometers. Solar Phys. 226, 143 – 151. doi: 10.1007/s11207-005-5688-9 .

    Article  ADS  Google Scholar 

  • Benz, A.O., Guedel, M., Isliker, H., Miszkowicz, S., Stehling, W.: 1991, A broad-band spectrometer for decimetric and microwave radio bursts: First results. Solar Phys. 133, 385 – 393. doi: 10.1007/BF00149896 .

    Article  ADS  Google Scholar 

  • Benz, A.O., Monstein, C., Meyer, H., Manoharan, P.K., Ramesh, R., Altyntsev, A., Lara, A., Paez, J., Cho, K.-S.: 2009, A world-wide net of solar radio spectrometers: e-CALLISTO. Earth Moon Planets 104, 277 – 285. doi: 10.1007/s11038-008-9267-6 .

    Article  ADS  Google Scholar 

  • Cane, H.V.: 2003, Near-relativistic solar electrons and type III radio bursts. Astrophys. J. 598, 1403 – 1408. doi: 10.1086/379007 .

    Article  ADS  Google Scholar 

  • Cliverd, M.A., Rodger, C.J., Thomson, N.R., Yearby, K.H.: 2001, Investigating the possible association between thunderclouds and plasmaspheric ducts. J. Geophys. Res. 106, 29771 – 29782. doi: 10.1029/2001JA000081 .

    Article  ADS  Google Scholar 

  • Cohen, M.B., Inan, U.S., Paschal, E.W.: 2010, Sensitive broadband ELF/VLF radio reception with the AWESOME instrument. IEEE Trans. Geosci. Remote Sens. 48, 3 – 17. doi: 10.1109/TGRS.2009.2028334 .

    Article  ADS  Google Scholar 

  • de Vos, M., Gunst, A.W., Nijboer, R.: 2009, The LOFAR telescope: System architecture and signal processing. Proc. IEEE 97, 1431 – 1437. doi: 10.1109/JPROC.2009.2020509 .

    Article  ADS  Google Scholar 

  • Dulk, G.A., Altschuler, M.D.: 1971, A moving type IV radio burst and its relation to the coronal magnetic field. Solar Phys. 20, 438 – 447. doi: 10.1007/BF00159777 .

    Article  ADS  Google Scholar 

  • Dumas, G., Caroubalos, C., Bougeret, J.-L.: 1982, The digital multi-channel radiospectrograph in Nançay. Solar Phys. 81, 383 – 394. doi: 10.1007/BF00151311 .

    Article  ADS  Google Scholar 

  • Fallows, R.A., Asgekar, A., Bisi, M.M., Breen, A.R., ter-Veeen, S.: 2012, The dynamic spectrum of interplanetary scintillation: First solar wind observations on LOFAR. Solar Phys., in press. doi: 10.1007/s11207-012-9989-5 .

  • Holman, G.D., Pesses, M.E.: 1983, Solar type II radio emission and the shock drift acceleration of electrons. Astrophys. J. 267, 837 – 843. doi: 10.1086/160918 .

    Article  ADS  Google Scholar 

  • Hoskin, M.: 2002, The Leviathan of Parsonstown: Ambitions and achievements. J. Hist. Astron. 33, 57 – 70.

    ADS  Google Scholar 

  • Kontogeorgos, A., Tsitsipis, P., Caroubalos, C., Moussas, X., Preka-Papadema, P., Hilaris, A., Petoussis, V., Bouratzis, C., Bougeret, J.-L., Alissandrakis, C.E., Dumas, G.: 2006, The improved ARTEMIS IV multichannel solar radio spectrograph of the University of Athens. Exp. Astron. 21, 41 – 55. doi: 10.1007/s10686-006-9066-x .

    Article  ADS  Google Scholar 

  • McLean, D.J.: 1967, Band splitting in type II solar radio bursts. Proc. Astron. Soc. 1, 47.

    ADS  Google Scholar 

  • McLean, D.J., Labrum, N.R.: 1985, Solar Radiophysics: Studies of Emission from the Sun at Metre Wavelengths, Cambridge University Press, Cambridge.

    Google Scholar 

  • Melrose, D.B.: 1975, Plasma emission due to isotropic fast electrons, and types I, II, and V solar radio bursts. Solar Phys. 43, 211 – 236. doi: 10.1007/BF00155154 .

    Article  ADS  Google Scholar 

  • Messmer, P., Benz, A.O., Monstein, C.: 1999, PHOENIX-2: A new broadband spectrometer for decimetric and microwave radio bursts first results. Solar Phys. 187, 335 – 345. doi: 10.1023/A:1005194314845 .

    Article  ADS  Google Scholar 

  • Nelson, G.J., Melrose, D.B.: 1985, In: McLean, D.J., Labrum, N.R. (eds.) Solar Radiophysics: Studies of Emission from the Sun at Metre Wavelengths, Cambridge Univ. Press, Cambridge, 333 – 359.

    Google Scholar 

  • Newkirk, G. Jr.: 1961, The solar corona in active regions and the thermal origin of the slowly varying component of solar radio radiation. Astrophys. J. 133, 983. doi: 10.1086/147104 .

    Article  ADS  Google Scholar 

  • Sheridan, K.V., Labrum, N.R., Payten, W.J.: 1972, Radio heliography – Multiple frequency operation at Culgoora. Nature 238, 115.

    ADS  Google Scholar 

  • Smerd, S.F., Sheridan, K.V., Stewart, R.T.: 1974, On split-band structure in type II radio bursts from the Sun. In: Newkirk, G.A. (ed.) Coronal Disturbances, IAU Symp. 57, 389.

    Chapter  Google Scholar 

  • Takakura, T., Kai, K.: 1961, Spectra of solar radio type IV bursts. Publ. Astron. Soc. Japan 13, 94.

    ADS  Google Scholar 

  • White, O.: 2007, Solar radio bursts and space weather. Asian J. Phys. 16, 189 – 207.

    Google Scholar 

Download references

Acknowledgements

The authors are indebted to the Seventh Earl of Rosse and the Birr Castle Demesne staff, particularly George Vaugh, for their support during the development of the RSTO. We would also like to thank the TCD Centre for Telecommunications Value-chain Research (CTVR) and the School of Physics Mechanical Workshop. P.Z. is supported by a TCD Innovation Bursary. EC is a Government of Ireland Scholar supported by the Irish Research Council for Science, Engineering and Technology. We would also like to thank the Alice Barklie Bequest to the TCD School of Physics. RSTO was established under the auspices of International Heliophysical Year 2007 and the International Space Weather Initiative, supported by the United Nations Basic Space Science Initiative.

Author information

Authors and Affiliations

Authors

Corresponding author

Correspondence to P. Zucca.

Additional information

Advances in European Solar Physics

Guest Editors: Valery M. Nakariakov, Manolis K. Georgoulis, and Stefaan Poedts

Rights and permissions

Reprints and permissions

About this article

Cite this article

Zucca, P., Carley, E.P., McCauley, J. et al. Observations of Low Frequency Solar Radio Bursts from the Rosse Solar-Terrestrial Observatory. Sol Phys 280, 591–602 (2012). https://doi.org/10.1007/s11207-012-9992-x

Download citation

  • Received:

  • Accepted:

  • Published:

  • Issue Date:

  • DOI: https://doi.org/10.1007/s11207-012-9992-x

Keywords

Navigation