Results of new absolute measurements of the solar flux density at 9500 MHz

In the wavelength range of about lambda =3.2 cm a discrepancy existed between the absolute calibrations made by the Nagoya University and by the Heinrich-Hertz-Institut (HHI) respectively. In this paper a new calibration carried out at the HHI is described, which results in a corrective multiplier of 1.087 for the values published in the 'HHI Solar Data'. Employing this factor the results of the Nagoya group and of the HHI are in good agreement.