Radio pulsar emission altitudes
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The Astronomical Society of India
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Abstract
By attributing the often seen longitude offsets between the core and conal component centres of pulsar radio pulses to different emission altitudes, we present a new method for investigating these altitudes. Our method can explain these offsets and also sheds light on them.
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Presented at the 21st meeting of the Astronomical Society of India, Pune, 2002.
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Bulletin of the Astronomical Society of India, 2002, Vol.30, p695-696
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(2002) by the Astronomical Society of India.