Contributions to Grain Yield from Pre-anthesis Assimilation in Tall and Dwarf Barley Phenotypes in Two Contrasting Seasons

Twenty-four barley genotypes were produced from crosses betweentwo sets of parents each having a different, non-allelic dwarfinggene. Four genotypes were phenotypically tall, twelve were singledwarf and eight were double dwarf. By a combination of carbon-14labelling and growth measurement the contribution to grain drymatter from assimilation before anthesis was estimated for eachgenotype in two years, 1976 and 1977. Pre-anthesis assimilation was estimated to have contributed44 per cent of grain dry matter in 1976, a very dry, hot year,but only 11 per cent in 1977, a wetter, cooler year. These percentageswere equivalent to about 133 and 74 g m^–2 in 1976 and1977. It is shown that some previous estimates of the contributionfrom pre-anthesis assimilation are too low for crops of barleygrown in the field in dry years, while in wet years, the contributionis unlikely to be less than 10 per cent. In neither year did the genotypes differ in the extent to whichpre-anthesis assimilation contributed to grain filling. In bothyears, grain yields of the tall genotypes were 8–9 percent greater than those of the double dwarf ones, and stem weightsat maturity 30 per cent greater. Hordeum vulgare L., barley, grain yield, carbon assimilation