作者: T. H. LEGG , J. L. LOCKE , C. W. MCLEISH , R. S. RICHARDS , J. L. YEN
DOI: 10.1038/216044A0
关键词: Quasar 、 Optics 、 Physics 、 Wavelength 、 Interferometry 、 Astrophysics 、 Radio wave 、 Astronomical interferometer 、 Range (statistics)
摘要: THE measurement of the diameter radio sources in range 10−2 sec arc or less has recently been made possible by a new technique interferometry. Independent stable local oscillators are used to convert signals at two stations frequencies which recorded on magnetic tapes. In principle, these long baseline interferometers (LBI) can operate any separation.