Abstract
Pulsar radio intensities contain a rich range of timescale variations ranging from months down to nanoseconds. The shortest of these fluctuations have been called microstructure . The observational properties of microstructure and the astrophysical value of microstructure are discussed.
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CITATION STYLE
APA
Hankins, T. H. (1996). Microstructure: A Review. International Astronomical Union Colloquium, 160, 197–204. https://doi.org/10.1017/s0252921100041464
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