Of Pulsars, their Winds, their Nebulae and Gamma-Rays

Details Of Pulsars, their Winds, their Nebulae and Gamma-Rays Of Pulsars, their Winds, their Nebulae and Gamma-Rays

Dec 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001ippa....1j...3k&link_type=abstract

Ipparchos, Vol.1, Issue 10, p. 3-4

Physics

Scientific paper

The issue of the structure of pulsar magnetospheres and the associated magneto-hydrodynamic (MHD) winds has remained open since their discovery, mainly because of our inability to construct solutions which would cross smoothly the Light Cylinder and would, thereby, connect the near and far field geometries. A recent solution has achieved precisely that, indicating that the resulting far field geometry is that of a magnetic (split) monopole. It was also shown that the same geometry can, in addition, resolve the issue of conversion of magnetic to particle energy in the associated MHD winds

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