Astronomy and Astrophysics – Astrophysics
Scientific paper
2002-10-15
Astronomy and Astrophysics
Astrophysics
9 pages, 1 figure, submitted to MNRAS Letters
Scientific paper
Using the formulation of relativistic reconnection by Lyutikov & Uzdensky (2002) we estimate the upper possible rates of reconnection in pulsar winds using Bohm prescription for resistivity. We find that the velocity of plasma inflow into the reconnection layer may be relativistic, of the order of the speed of light in the plasma rest-frame. This in principle may allow efficient dissipation of the magnetic field energy in the wind and/or destruction of the toroidal magnetic flux. The efficiency of reconnection realized in pulsar winds remains an open question: it should depend both on the microphysical properties of plasma and on the three-dimensional structure of the reconnection flow.
No associations
LandOfFree
Rates of reconnection in pulsar winds does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Rates of reconnection in pulsar winds, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Rates of reconnection in pulsar winds will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-569065