The SOLSPEC instrument has been built to carry out absolute solar spectral
irradiance measurements from space. It was first flown in December 1983 on
mission STS 9 (Spacelab 1), from August 1992 to June 1993 on board the free
-flying EURECA platform with mission STS 46 (deployment) and STS 57 (retrie
val), then flown three times more with the ATLAS missions STS 45, 56 and 66
. Further applications are foreseen in combination with the International S
pace Station Alpha (ISSA). SOLSPEC covers a wavelength range from 180 nm to
3000 nm split into three separate spectrometer channels (ultraviolet, visi
ble and infrared) and has been calibrated pre- and post-flight using a blac
k body at the Landessternwarte Heidelberg with temperatures up to 3300 K. I
n this paper the calibration concept is presented, together with a short in
strument description and suggestions for improvements in order that higher
black-body temperatures can be reached.