| 1. |
- Ahn, C.M., et al.
(författare)
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Effect of ibuprofen on thrombin-induced pulmonary edema in the rat
- 1994
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Ingår i: Pulmonary pharmacology. - : Elsevier BV. - 0952-0600. ; 7:6, s. 393-399
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Tidskriftsartikel (refereegranskat)abstract
- The effect of ibuprofen on thrombin-induced pulmonary edema was studied in rats. Thrombin infusion produced a significant increase in lung weight, wet weight/dry weight ratio and relative lung water content, a rise in mean pulmonary arterial pressure and a fall in mean systemic arterial pressure. It also caused a progressive decrease in PaO2 and a continuous increase in pH and PaCO2. Administration of either the S-isomer or R-isomer of ibuprofen at doses of 5 mg/kg body weight prior to thrombin infusion resulted in significant reduction in lung weight, wet weight/dry weight ratio and water content. The wet weight/dry weight ratio and the water content were somewhat lower after infusion of the S-isomer than of the R-isomer. Ibuprofen diminished the thrombin-induced increase in mean pulmonary arterial pressure and attenuated the early and late decrease in mean systemic arterial pressure caused by thrombin. Ibuprofen also stabilized thrombin-induced impairments in PaO2, PaCO2 and pH. The results thus indicate that ibuprofen effectively counteracts hemodynamic changes, stabilizes impairments in arterial blood gas variables and attenuates the increase in lung vascular permeability to protein with pulmonary edema caused by thrombin. The results also indicate a substantial R to S chiral inversion of ibuprofen in vivo in the rat.
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| 2. |
- Knipp, D.J., et al.
(författare)
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Ionospheric Convection Response to Slow, Strong Variations in a Northward Interplanetary Magnetic Field: A Case Study for January 14, 1988
- 1993
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Ingår i: Journal of Geophysical Research. - 0148-0227 .- 2156-2202. ; 98, s. 19273-19292
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Tidskriftsartikel (refereegranskat)abstract
- We analyze ionospheric convection patterns over the polar regions during the passage of an interplanetary magnetic cloud on January 14, 1988, when the interplanetary magnetic field (IMF) rotated slowly in direction and had a large amplitude. Using the assimilative mapping of ionospheric electrodynamics (AMIE) procedure, we combine simultaneous observations of ionospheric drifts and magnetic perturbations from many different instruments into consistent patterns of high-latitude electrodynamics, focusing on the period of northward IMF. By combining satellite data with ground-based observations, we have generated one of the most comprehensive data sets yet assembled and used it to produce convection maps for both hemispheres. We present evidence that a lobe convection cell was embedded within normal merging convection during a period when the IMF B(y) and B(z) components were large and positive. As the IMF became predominantly northward, a strong reversed convection pattern (afternoon-to-morning potential drop of around 100 kV) appeared in the southern (summer) polar cap, while convection in the northern (winter) hemisphere became weak and disordered with a dawn-to-dusk potential drop of the order of 30 kV. These patterns persisted for about 3 hours, until the IMF rotated significantly toward the west. We interpret this behavior in terms of a recently proposed merging model for northward IMF under solstice conditions, for which lobe field lines from the hemisphere tilted toward the Sun (summer hemisphere) drape over the dayside magnetosphere, producing reverse convection in the summer hemisphere and impeding direct contact between the solar wind and field lines connected to the winter polar cap. The positive IMF B(x) component present at this time could have contributed to the observed hemispheric asymmetry. Reverse convection in the summer hemisphere broke down rapidly after the ratio \textbackslashB(y)/B(z)\textbackslash exceeded unity, while convection in the winter hemisphere strengthened. A dominant dawn-to-dusk potential drop was established in both hemispheres when the magnitude of B(y) exceeded that of B(z), with potential drops of the order of 100 kV, even while B(z) remained northward. The later transition to southward B(z) produced a gradual intensification of the convection, but a greater qualitative change occurred at the transition through \textbackslashB(y)/B(z)\textbackslash = 1 than at the transition through B(z) = 0. The various convection patterns we derive under northward IMF conditions illustrate all possibilities previously discussed in the literature: nearly single-cell and multicell, distorted and symmetric, ordered and unordered, and sunward and antisunward.
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