It has been demonstrated that a simple two-compartment kinetic model may account for the changes in plasma concentration of pancuronium after i.v. administration. However, it can be shown that this simple model does not account satisfactory for the observed changes in muscle twitch response. By the addition of a receptor (biophase) compartment, twitch response can be reconciled with model behavior and the characteristics resemble those predicted by animal studies. The complete model is applied to the problem of total renal failure, and shows that patients with this condition are likely to be marginally resistant to small doses of pancuronium, with a normal rate of recovery. However, larger doses are likely to result in delayed recovery, the duration of effect increasing in a dose-dependent manner.

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Osmoregulation of vasopressin secretion was studied in eight healthy women in the follicular and luteal phases of the menstrual cycle. Basal plasma osmolality in the luteal phase was significantly lower than in the follicular period (282.4 +/- 0.6, 285.6 +/- 1.1mmol/kg, respectively, P less than 0.05). Plasma AVP (pAVP) and plasma osmolality (pOsm) were measured during the infusion of 850 mmol/l saline in both phases of the cycle, and linear regression analyses of these data gave the following regression equations (i) follicular, pAVP = 0.43 (pOsm - 284), r = + 0.93, (ii) luteal, pAVP = 0.31 (pOsm - 279), r = + 0.95. Both the slope and abscissal intercept were significantly different (P less than 0.01). Osmotic threshold for thirst sensation in the luteal phase was lower than the follicular (293 +/- 2,297 +/- 1 mmol/kg, P less than 0.005). We conclude that, in the luteal phase, the threshold for AVP release and the gain or sensitivity of the osmostat are reduced together with lowering of the thirst threshold, which account for the lower basal luteal plasma osmolality.

The two-dimensional (horizontal) shear instability of a differentially rotating star is examined. A solar-typc rotation law is investigated. and it is found that for equatorial accelerations there is instability when there is a difference of 29% between the angular velocity of the equator and the poles.