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Table 2.

Measured solar radii at several frequencies in the range 18 − 26 GHz with the Grueff Radio Telescope and SRT radio telescopes, obtained through the modelling described in Sects. 3.1 and 3.2.

Frequency Telescope Type radius HP method IP method ECB model 2GECB model
(GHz) (arcsec) (arcsec) (arcsec) (arcsec)
18.1 Grueff Rc
18.1 Grueff Req

18.1 Grueff Rpol
18.3 Grueff Rc
18.3 Grueff Req
18.3 Grueff Rpol
18.3 Grueff Rc (averaged) 981.7 ± 0.3 976.4 ± 0.3
18.3 Grueff Req (averaged) 984.9 ± 0.6 977.8 ± 0.8

18.3 Grueff Rpol (averaged) 978.8 ± 0.6 974.0 ± 0.8
18.8 SRT Rc
18.8 SRT Req
18.8 SRT Rpol

23.6 Grueff Rc
23.6 Grueff Req
23.6 Grueff Rpol

24.7 SRT Rc
24.7 SRT Req
24.7 SRT Rpol

25.8 Grueff Rc
25.8 Grueff Req
25.8 Grueff Rpol
25.8 Grueff Rc (averaged) 979.3 ± 0.4 972.1 ± 0.4
25.8 Grueff Req (averaged) 979.9 ± 0.9 971.9 ± 0.9
25.8 Grueff Rpol (averaged) 977.9 ± 0.9 973.1 ± 0.9

26.1 Grueff Rc
26.1 Grueff Req
26.1 Grueff Rpol

Notes. As specified at 18.3 and 25.8 GHz, we also report the measured values obtained from the averaged solar maps.

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