Chemical composition measurements of the atmosphere of Jupiter with the Galileo Probe mass spectrometer.

The Galileo Probe entered the atmosphere of Jupiter on December 7, 1995. Measurements of the chemical and isotopic composition of the Jovian atmosphere were obtained by the mass spectrometer during the descent over the 0.5 to 21 bar pressure region over a time period of approximately 1 hour. The sampling was either of atmospheric gases directly introduced into the ion source of the mass spectrometer through capillary leaks or of gas, which had been chemically processed to enhance the sensitivity of the measurement to trace species or noble gases. The analysis of this data set continues to be refined based on supporting laboratory studies on an engineering unit. The mixing ratios of the major constituents of the atmosphere hydrogen and helium have been determined as well as mixing ratios or upper limits for several less abundant species including: methane, water, ammonia, ethane, ethylene, propane, hydrogen sulfide, neon, argon, krypton, and xenon. Analysis also suggests the presence of trace levels of other 3 and 4 carbon hydrocarbons, or carbon and nitrogen containing species, phosphine, hydrogen chloride, and of benzene. The data set also allows upper limits to be set for many species of interest which were not detected. Isotope ratios were measured for 3He/4He, D/H, 13C/12C, 20Ne/22Ne, 38Ar/36Ar and for isotopes of both Kr and Xe.

The Galileo probe mass spectrometer: composition of Jupiter's atmosphere.

The composition of the jovian atmosphere from 0.5 to 21 bars along the descent trajectory was determined by a quadrupole mass spectrometer on the Galileo probe. The mixing ratio of He (helium) to H2 (hydrogen), 0.156, is close to the solar ratio. The abundances of methane, water, argon, neon, and hydrogen sulfide were measured; krypton and xenon were detected. As measured in the jovian atmosphere, the amount of carbon is 2.9 times the solar abundance relative to H2, the amount of sulfur is greater than the solar abundance, and the amount of oxygen is much less than the solar abundance. The neon abundance compared with that of hydrogen is about an order of magnitude less than the solar abundance. Isotopic ratios of carbon and the noble gases are consistent with solar values. The measured ratio of deuterium to hydrogen (D/H) of (5 +/- 2) x 10(-5) indicates that this ratio is greater in solar-system hydrogen than in local interstellar hydrogen, and the 3He/4He ratio of (1.1 +/- 0.2) x 10(-4) provides a new value for protosolar (solar nebula) helium isotopes. Together, the D/H and 3He/4He ratios are consistent with conversion in the sun of protosolar deuterium to present-day 3He.

Evaluation of carbamazepine and carbamazepine-epoxide protein binding in patients undergoing epilepsy surgery.

Carbamazepine (CBZ) serum concentrations increase after epilepsy surgery. A possible mechanism may be acute changes in protein binding, specifically those involving the acute phase reactant alpha(1)-acid glycoprotein (AAG). We prospectively evaluated 16 adults (11 receiving CBZ) with epilepsy (mean age 30 +/- 9.9 years, 8 women and 8 men) undergoing temporal lobe resections and characterized AAG, albumin, CBZ, and CBZ-epoxide (CBZ-E) free fractions over time. AAG, ALB, CBZ, and CBZ-E free fractions were determined before surgery (baseline) and on postoperative days 1-5, 14, and 30. AAG was measured with a radial immunodiffusion assay method, CBZ and CBZ-E serum concentrations were determined by high-performance liquid chromatography (HPLC). Free fractions of CBZ and CBZ-E were calculated as the ratio of unbound (determined after ultracentrifugation) to total serum drug concentrations. Statistical analysis included analysis of variance (ANOVA) and Student's t test for paired data when appropriate, with significance assigned at p<0.05. All data are mean +/- SD. AAG concentrations increased significantly from baseline 61.9 +/- 21.3 mg/dl), peaking at postoperative day 3 (116.8 +/- 20.6 mg/gl) and decreasing to baseline levels between days 14 and 30. CBZ serum concentrations were significantly increased in the immediate postoperative period (day 3), but albumin concentrations and CBZ and CBZ-E free fractions did not differ significantly between baseline and the postoperative time points. Temporal lobe resection results in an acute phase reaction which is manifested in part by significant changes in AAG. Although CBZ and CBZ-E total serum concentrations increased significantly in the immediate postoperative period, epilepsy surgery did not appear to result in significant overall changes in drug binding to plasma proteins.

Relationship between valproic acid dosage, plasma concentration and clearance in adult monotherapy patients with epilepsy.

Significant variability has been reported in the plasma concentration-dose relationship for the anticonvulsant compound valproic acid (VPA). Several factors may contribute to this observed variability, including heterogeneous patient populations of children and adults, polytherapy, and timing of plasma concentration sampling. To optimally determine the relationship between trough VPA plasma concentration and dose, we evaluated a homogeneous group of adult ambulatory patients with epilepsy receiving VPA monotherapy. Furthermore, we sought to evaluate whether a relationship existed between VPA dosage and plasma clearance for both total and unbound or free drug. Steady-state trough plasma concentrations were determined in thirty-two patients. Mean VPA dose was 22.8 +/- 10.3 mg/kg/day. Mean total and unbound VPA plasma concentrations were 97.9 +/- 34.9 and 13.2 +/- 10.6 micrograms/ml, respectively. Significant correlations between VPA dose and total and unbound plasma concentrations were found (r = 0.82 and r = 0.85, P < or = 0.001, respectively). Significant relationships were also observed between VPA dose and clearance. A positive correlation was noted for dose and total plasma clearance (r = 0.61, P < or = 0.001), while an inverse correlation existed between dose and unbound VPA plasma clearance (r = -0.51, P < 0.01). Although a statistically significant correlation does exist between VPA dosage and both total and unbound plasma concentrations, significant interpatient variability still remains even under 'optimal' therapeutic drug monitoring conditions.

Venus upper atmosphere neutral gas composition: first observations of the diurnal variations.

Measurements of the composition, temperature, and diurnal variations of the major neutral constituents in the thermosphere of Venus are being made with a quadrupole mass spectrometer on the Pioneer Venus orbiter. Concentrations of carbon dioxide, carbon monoxide, molecular nitrogen, atomic oxygen, and helium are presented, in addition to an empirical model of the data. The concentrations of the heavy gases, carbon dioxide, carbon monoxide, and molecular nitrogen, rapidly decrease from the evening terminator toward the nightside; the concentration of atomic oxygen remains nearly constant and the helium concentration increases, an indication of a nightside bulge. The kinetic temperature inferred from scale heights drops rapidly from 230 K at the terminator to 130 K at a solar zenith angle of 120 degrees , and to 112 K at the antisolar point.

Venus upper atmosphere neutral composition: preliminary results from the pioneer venus orbiter.

Measurements in situ of the neutral composition and temperature of the thermosphere of Venus are being made with a quadrupole mass spectrometer on the Pioneer Venus orbiter. The presence of many gases, incluiding the major constituents CO(2), CO, N(2), O, and He has been confirmed. Carbon dioxide is the most abundant constituent at altitudes below about 155 kilometers in the terminator region. Above this altitude atomic oxygen is the major constituent, with O/CO(2) ratios in the upper atmosphere being greater than was commonly expected. Isotope ratios of O and C are close to terrestrial values. The temperature inferred from scale heights above 180 kilometers is about 400 K on the dayside near the evening terminator at a solar zenith angle of about 69 degrees . It decreases to about 230 K when the solar zenith angle is about 90 degrees .

Composition and structure of the martian atmosphere: preliminary results from viking 1.

Results from the aeroshell-mounted neutral mass spectrometer on Viking I indicate that the upper atmosphere of Mars is composed mainly of CO(2) with trace quantities of N(2), Ar, O, O(2), and CO. The mixing ratios by volume relative to CO(2) for N(2), Ar, and O(2) are about 0.06, 0.015, and 0.003, respectively, at an altitude near 135 kilometers. Molecular oxygen (O(2)(+)) is a major component of the ionosphere according to results from the retarding potential analyzer. The atmosphere between 140 and 200 kilometers has an average temperature of about 180 degrees +/- 20 degrees K. Atmospheric pressure at the landing site for Viking 1 was 7.3 millibars at an air temperature of 241 degrees K. The descent data are consistent with the view that CO(2) should be the major constituent of the lower martian atmosphere.