Instability of the pulsar surface in strong constant fields and generation of additional components due to combination scattering

Instability of the pulsar surface in strong constant fields and generation of additional components due to combination scattering

Periodic structures on polar caps, arising due to instability of the pulsar surface in a strong magnetic field, can be responsible both for the appearance of additional components in pulsar radiation and the formation of sickle shaped hot spots arising as a possible result of Mandelstam–Raman scatte...

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Veröffentlicht in:Low temperature physics (Woodbury, N.Y.) N.Y.), 2021-07, Vol.47 (7), p.596-604
1. Verfasser: Kontorovich, V. M.
Format: Artikel
Sprache:eng
Schlagworte:
Physical Sciences
Physics
Physics, Applied
Science & Technology
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Zusammenfassung:Periodic structures on polar caps, arising due to instability of the pulsar surface in a strong magnetic field, can be responsible both for the appearance of additional components in pulsar radiation and the formation of sickle shaped hot spots arising as a possible result of Mandelstam–Raman scattering of the reflected radiation by returned positrons.
ISSN:1063-777X
1090-6517
DOI:10.1063/10.0005188