Abstract
We describe the new Nançay Radioheliograph (version II) which is a multicorrelator system. The main characteristics of this instrument are high space and time resolutions and flexible on-line data processing. At present it produces one-dimensional images at 169 MHz. This instrument is mainly intended for solar observations.
An accurate calibration of the instrument has been carried out leading to a precise fringe stopping and to a proper knowledge of the grating response. Preliminary solar results are presented: existence of apparent motions in noise storms with a velocity of the order of 5000 km s−1; observations of radiobursts as narrow as 0.7′ (Kerdraon, 1977); observations of spikeburst activity.
Similar content being viewed by others
References
Bonmartin, J.: 1977, Thèse d'Ingénieur Docteur.
Kerdraon, A.: 1977,Astron. Astrophys., to be submitted.
MacKay, H. A., Kwong, C. K., Jones, I. G., and Symonds, W. A.: 1973,Proceedings of the IREE, Vol. 34, No. 8.
Riddle, A. C.: 1972,Proc. Astron. Soc. A2, 98.
Steinberg, J. L., Aubier-Giraud, M., Leblanc, Y., and Boischot, A.: 1971,Astron. Astrophys. 10, 362.
Author information
Authors and Affiliations
Additional information
Presently in Sydney, Australia.
Rights and permissions
About this article
Cite this article
Bonmartin, J., Jones, I., Kerdraon, A. et al. The mark II Nançay radioheliograph. Sol Phys 55, 251–261 (1977). https://doi.org/10.1007/BF00150888
Received:
Revised:
Issue Date:
DOI: https://doi.org/10.1007/BF00150888