Converging Cylindrical Shocks in Magnetohydrodynamics

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Converging Cylindrical Shocks in Magnetohydrodynamics
Gerald B Whitham
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Ic If p (r), p (r), H (r), refer to the rvosslble equilibrium states that may exist in the uadisturbed medium ahead of the shock, these functions satisfy the relotions (1[|. ) p + p li H + ti, 1 — -— dr = constant, O ^ O v/ J^ (15) S = constant, Pq '" Pq In addition, it will be necessary in this work to have the rela- tions connecting u(r), p(r), p{r), H(r) in steady isentropic flow. From equations (9) to (13) we may write these in tVje dif- ferential form (which is convenient for later purpose...s): Hg u H u r ' z u du + ^ + ^ (H^, dH^ + H dH ) + ii H?, — =, p p'Q Q z z p©r ' dp + du ^ dr ^ Q pur ' dp = a dp where a is the sound speed. Solving these equations we have / 6 _ du _ -j^ ar Hg u r J T T dp _ dp _ z _, , . Dr 727 - ~ - "IT - ^^"^^ ■" a p ^ z ) (I6)''j P / a^ + tidip - Hg) / p where A = —5 5 5 a^ + ^{eI + H^) / p Turning now to the shock relations, the general form piven by Friedrichs simplifies in this case since there is no normal o component of the nia. Iiotic field.

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