FAST and MeerKAT pulsar surveys show O-mode mean profiles are wider than X-mode profiles and that orthogonal interpulse pulsar statistics favor the classical BGI vacuum-gap evolutionary model over MHD models.
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Data from FAST and MeerKAT surveys as a test of radio pulsar physics
FAST and MeerKAT pulsar surveys show O-mode mean profiles are wider than X-mode profiles and that orthogonal interpulse pulsar statistics favor the classical BGI vacuum-gap evolutionary model over MHD models.