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Article
Origin of the Solar Corona
IF the distributions of electron density and temperature in the sun's atmosphere are known, thermal emission at any frequency in the radio spectrum may be calculated. Conversely, properties of the atmosphere m...
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Article
Eruptive Prominence of February 26, 1953, and Associated Radio Noise-Burst: Radio Observations at the Time of an Ascending Solar Prominence
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Article
A Method for the Measurement of the Distance of Radio Stars
THE existence of a large number of discrete sources of extraterrestrial radio radiation (radio stars) has now been established. For the majority of the sources there is no information about their distance; onl...
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Article
An Alternative Identification of the Radio Source in the Direction of the Galactic Centre
A RADIO source the co-ordinates of which agree closely with those of the centre of the Galaxy has been reported by several observers, and it has been suggested that it may be identified with the nucleus of the...
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Article
Red-Shift Absorption Spectrum of the Cygnus-A Radio Source
A MEASUREMENT to check the 21-cm. hydrogen line absorption spectrum of Cygnus-A (19N4A) reported by Lilley and McClain1 is important in view of the cosmological significance of their result. The absorption was ob...
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Article
Amateur Radio Astronomy
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Article
Measurement of Magnetic Fields in Interstellar Clouds
PREVIOUS attempts1β3 with the 250-ft. radio telescope at Jodrell Bank to measure magnetic fields in interstellar clouds in the Milky Way by observing the Zeeman splitting of their neutral hydrogen line profiles f...
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Article
Measurements of OH Emission Sources with an Interferometer of High Resolution
PREVIOUS experiments at Lincoln Laboratories, M.I.T.1, California Institute of Technology2 and Jodrell Bank (to be published) to determine the angular size of the OH emission regions have used interferometers wit...
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Article
Today's Radio Telescopes
Radioastronomical Methods of Antenna Measurements
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Article
Structure of the Galactic Magnetic Field
Faraday rotation measurements have shown that there is a basic order in the galactic magnetic field which can be fitted by simple models. The data also indicate the presence of irregularities in electron densi...
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Article
Interstellar Magnetic Fields determined from Zeeman Effect Measurements
THE Zeeman splitting of the 21 cm line in interstellar neutral hydrogen clouds provides the only direct measure of the line of sight component of the magnetic fields in the interstellar medium. It gives the fi...
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Article
Neutral Hydrogen Asymmetry in the Galaxy M101 as Evidence for Tidal Effects
Measurements of the distribution of neutral hydrogen in the galaxy M101 reveal an asymmetry which raises interesting points about tidal effects in galaxies due to nearby companions.
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Article
Our Galaxy
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Article
The Jodrell Bank Radio Frequency Digital Autocorrelation Spectrometer
A versatile digital autocorrelation spectrometer designed and built at Jodrell Bank is described, together with some examples of observations made with the new instrument.
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Article
Distance of Pulsars and the Interstellar Electron Gas
Information about the interstellar distribution of hydrogen can help to refine estimates of pulsar distances.
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Article
Solar Radio Astronomy
Radio Emission of the Sun and Planets
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Book
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Chapter
The Relative Density of H, OH and H2CO in Interstellar Clouds
I have attempted to obtain an answer to the question βIn which gas (neutral hydrogen) clouds do we find molecules?β By limiting the investigation to those clouds which might be considered normal (i.e. specific...
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Article
Spiral Arms in Space
The Spiral Structure of Our Galaxy
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Article
Outer Spiral Structure and High Velocity Clouds in the Galaxy
New observations of high velocity clouds show that these may be interpreted in terms of an extension of the outermost spiral arm, confirming and extending the model of Habing.