Fine-Scale Anisotropy of the Cosmic Microwave Background Radiation

Paul E. Boynton
1974 Symposium - International astronomical union  
In keeping with the title of Symposium No. 63, I would like to confront the assembly with a short review of observational upper limits on the amplitude of intensity fluctuations in the microwave background radiation on angular scales of less than one degree. These fluctuations are presently of interest for at least two important cosmological concerns:
doi:10.1017/s007418090023550x fatcat:frjf2lldtfhrxdqc2dhgpyb7ym