UDK 53
UDK 520
UDK 521
UDK 523
UDK 524
UDK 52-1
UDK 52-6
GRNTI 41.00
GRNTI 29.35
GRNTI 29.31
GRNTI 29.33
GRNTI 29.27
GRNTI 29.05
OKSO 03.06.01
OKSO 03.05.01
OKSO 03.04.03
BBK 2
BBK 223
TBK 614
TBK 6135
BISAC SCI004000 Astronomy
BISAC SCI005000 Physics / Astrophysics
The influence of inclination angle to electron-positron pairs production in inner gap and polar cap heating by reverse positron current in case of J0901-4046 radiopulsar is considered. It is shown that J0901-4046 pulsar ``work" may be explained by the presence of a highly curved small scale surface magnetic field without the substantial increasing of its dipolar magnetic field at inclination angle values $\chi \lesssim 30^{\circ}$.
pulsars: general, individual (J0901-4046)
1. Barsukov D., Morozov I., and Popov A., 2023, Astronomy Letters, 49, p. 806
2. Beskin V. and Istomin A., 2022, Monthly Notices of the Royal Astronomical Society, 516, p. 5084
3. Caleb M., Heywood I., Rajwade K., et al., 2022, Nature Astronomy, 6, p. 828
4. Kantor E. and Tsygan A., 2003, Astronomy Reports, 47, p. 613
5. Malov I. and Nikitina E., 2011, Astronomy Reports, 55, p. 878
6. Manchester R., Hobbs G., Teoh A., et al., 2005, The Astronomical Journal, 129, p. 1993
7. Rankin J., 1990, Astrophysical Journal, 352, p. 247
8. Sob'yanin D., 2023, Physical Review D, 107, id. L081301.