A discussion of the history of scientific computing for Radio Astronomy in the Cavendish Laboratory of the University of Cambridge in the decades after the Second World War. This covers the development of the aperture synthesis technique for Radio Astronomy and how that required using the new computing technology developed by the University's Mathematical Laboratory: the EDSAC, EDSAC 2 and TITAN computers. It looks at the scientific advances made by the Radio Astronomy group, particularly the assembling of evidence which contradicted the Steady State Hypothesis. It also examines the software advances that allowed bigger telescopes to be built: the Fast Fourier Transform (FFT) and the degridding algorithm. Throughout, the contribution of women is uncovered, from the diagrams they drew for scientific publications, through programming and operating computers, to writing scientific papers.
翻译:讨论第二次世界大战后数十年剑桥大学卡文迪什实验室射电天文学科学计算的历史,包括发展射电天文学孔径合成技术,以及需要如何使用该大学数学实验室开发的新计算机技术:EDSAC、EDSAC 2和TITAN计算机;研究射电天文学小组的科学进步,尤其是与稳定的国家假设相矛盾的成套证据;还研究能够建造更大望远镜的软件进步:快速的Fourier变换(FFT)和解密算法;从她们为科学出版物绘制的图表中,通过编程和操作计算机,从她们为撰写科学论文而绘制的图表中,发现妇女的贡献。