All Tables

Table 1: Observationally inferred pulsar data. Note that in Esamdin et al. (2005) no value for $\beta$ is quoted. Also, we infer P₃ from their values of P₂ and using the relation for the drift rate $D (^\circ /P_1) = P_2(^\circ )/P_3(P_1)$ , which is a good approximation for this system, as it is nearly aligned. Positive and negative values are obtained due to the definition of drift rate.
Table 2: The results of Q and $\tilde{\Gamma}$ for possible beam configurations for PSR B0943+10 by assuming l = 20 and $\tilde{\omega}_{\rm pat} = 0.973$ . The charge density difference is found to be $h \approx 19.5$ . Initial guess for R₁/R₃ and R₂/R₃ is taken from Fig. 10 in DR01.