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ABSTRACT Stars with a dipole magnetic field oriented at an angle to the rotation axis may emit pulsating radio signals. Access through your institution Buy or subscribe This is a preview of
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ADDITIONAL ACCESS OPTIONS: * Log in * Learn about institutional subscriptions * Read our FAQs * Contact customer support SIMILAR CONTENT BEING VIEWED BY OTHERS A PULSAR-LIKE POLARIZATION
ANGLE SWING FROM A NEARBY FAST RADIO BURST Article 01 January 2025 STRONG AND WEAK PULSAR RADIO EMISSION DUE TO THUNDERSTORMS AND RAINDROPS OF PARTICLES IN THE MAGNETOSPHERE Article 17
August 2023 DETERMINATION OF X-RAY PULSAR GEOMETRY WITH IXPE POLARIMETRY Article 24 October 2022 REFERENCES * Maran, S. P., and Cameron, A. G. W., _Physics Today_ (August 1968). * Pacini,
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Article ADS Google Scholar Download references AUTHOR INFORMATION AUTHORS AND AFFILIATIONS * Atomic Energy Commission, Washington, DC BERNARD J. EASTLUND Authors * BERNARD J. EASTLUND
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Rotator and Pulsar Radiation. _Nature_ 220, 1293–1296 (1968). https://doi.org/10.1038/2201293a0 Download citation * Received: 21 October 1968 * Issue Date: 28 December 1968 * DOI:
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