Zobrazeno 1 - 10
of 61
pro vyhledávání: '"Melrose, Donald B."'
Autor:
Lower, Marcus E., Johnston, Simon, Lyutikov, Maxim, Melrose, Donald B., Shannon, Ryan M., Weltevrede, Patrick, Caleb, Manisha, Camilo, Fernando, Cameron, Andrew D., Dai, Shi, Hobbs, George, Li, Di, Rajwade, Kaustubh M., Reynolds, John E., Sarkissian, John M., Stappers, Benjamin W.
Radio emission from magnetars provides a unique probe of the relativistic, magnetized plasma within the near-field environment of these ultra-magnetic neutron stars. The transmitted waves can undergo birefringent and dispersive propagation effects th
Externí odkaz:
http://arxiv.org/abs/2311.04195
Publikováno v:
Phys. Rev. E 103, 061201 (2021)
It is shown that the choice of spin-operator affects the form of the response tensor describing a spin-dependent electron gas. The covariant, spin-dependent response tensor for a magnetic dipole moment-polarized electron gas (statistical distribution
Externí odkaz:
http://arxiv.org/abs/2104.00565
Flares produce sudden and permanent changes in the horizontal photospheric magnetic field. In particular flares generally produce increased magnetic shear in the photospheric field along the neutral line. Recent observations show also that flares can
Externí odkaz:
http://arxiv.org/abs/1808.03097
Akademický článek
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Autor:
Melrose, Donald B., Yuen, Rai
We reconsider pulsar electrodynamics for an obliquely rotating pulsar, and propose a way of synthesizing the vacuum dipole model (VDM) and the rotating magnetosphere model (RMM). We first modify the VDM by assuming that the parallel component of the
Externí odkaz:
http://arxiv.org/abs/1310.1134
Autor:
Melrose, Donald B., Yuen, Rai
The inductive electric field is unjustifiably neglected in most models for pulsar electrodynamics; it cannot be screened by the magnetospheric plasma, and it is not small in comparison with the corotation electric field. The perpendicular component o
Externí odkaz:
http://arxiv.org/abs/1210.8225
We discuss the intergalactic propagation of ultra-high-energy cosmic rays (UHECRs) with energies E \geq 10^{18.5} eV. We consider the propagation of UHECRs under the influence of the energy-dependent deflection by a weak random magnetic field in the
Externí odkaz:
http://arxiv.org/abs/astro-ph/9907060
Autor:
Melrose, Donald B.1 (AUTHOR) donald.melrose@sydney.edu.au, Harding, James2 (AUTHOR), Cairns, Iver H.1 (AUTHOR)
Publikováno v:
Solar Physics. Feb2021, Vol. 296 Issue 2, p1-17. 17p.
Akademický článek
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Autor:
Melrose, Donald B., Martinez Pillet, Valentin, Webb, David F., Bougeret, Jean-Louis, Klimchuk, James A., Kosovichev, Alexander, van Driel-Gesztelyi, Lidia, von Steiger, Rudolf
Publikováno v:
Proceedings of the International Astronomical Union. Dec2010, Vol. 6 Issue T27B, p146-157. 12p.