The Determination of the Internal Volume of Steel Capillaries for Measurements with Gases

1939 ◽  
Vol 10 (2) ◽  
pp. 57-58 ◽  
Author(s):  
Joseph Kaminsky ◽  
B. Edwin Blaisdell
Keyword(s):  
1983 ◽  
Vol 29 (1) ◽  
pp. 80-85 ◽  
Author(s):  
M Luzzana ◽  
G Dossi ◽  
A Mosca ◽  
A Granelli ◽  
D Berger ◽  
...  

Abstract A new automatic apparatus based on the differential measurement of pH between two solutions has been developed. Two 25-microL (internal volume) glass capillary electrodes are used to measure the results of automated (under microcomputer control) chemical reactions that lead to the liberation or the uptake of hydrogen ions. The sensitivity of the differential pH measurements is better than +/- 0.0001 pH unit, and the change in H+ concentration that can be detected by such an apparatus is 1 mumol/L for plasma and 3 mumol/L for whole blood. The technique has been applied to the measurement of glucose in plasma, giving results in agreement with the specifications of the Food and Drug Administration reference method for quantitative determination of glucose (hexokinase/glucose-6-phosphate dehydrogenase method).


1984 ◽  
Vol 4 (7) ◽  
pp. 551-557 ◽  
Author(s):  
Ronald L. Bartzatt ◽  
David J. Volsky

Sendal virus envelopes (SVE) were isolated from Sendal virus particles by Triton X-100 solubilization and ultracentrifugation. The envelopes were reconstituted in the presence of the fluorescent dye calcein by gradual removal of the detergent with Bio-beads SM-2. The internal volume of reconstituted Sendal virus envelopes (RSVE) was determined by quenching the fluorescence of calcein with cobalt (II) ions. The internal volume of RSVE was found to be proportional to the initial SVE protein concentration in the recon-stitution mixture, reaching about 18% of the total volume with 5.6 mg of SVE protein per ml. When radiolabelled cloned Epstein-Barr virus DNA fragment was included in the reconstitution mixture, the proportion of DNA associated with the vesicles much exceeded the trapping volume, indicating adsorption of DNA to the internal surface of RSVE. These deter-minations will allow optimization of the use of RSVE as gene-transfer vehicles.


2016 ◽  
Vol 0 (5(46)) ◽  
pp. 64-68
Author(s):  
A. V. Stadnichenko ◽  
Yu. M. Krasnopolskyi ◽  
V. I. Shvets ◽  
T. G. Yarnykh
Keyword(s):  

1966 ◽  
Vol 25 ◽  
pp. 93-97
Author(s):  
Richard Woolley

It is now possible to determine proper motions of high-velocity objects in such a way as to obtain with some accuracy the velocity vector relevant to the Sun. If a potential field of the Galaxy is assumed, one can compute an actual orbit. A determination of the velocity of the globular clusterωCentauri has recently been completed at Greenwich, and it is found that the orbit is strongly retrograde in the Galaxy. Similar calculations may be made, though with less certainty, in the case of RR Lyrae variable stars.


1999 ◽  
Vol 190 ◽  
pp. 549-554
Author(s):  
Nino Panagia

Using the new reductions of the IUE light curves by Sonneborn et al. (1997) and an extensive set of HST images of SN 1987A we have repeated and improved Panagia et al. (1991) analysis to obtain a better determination of the distance to the supernova. In this way we have derived an absolute size of the ringRabs= (6.23 ± 0.08) x 1017cm and an angular sizeR″ = 808 ± 17 mas, which give a distance to the supernovad(SN1987A) = 51.4 ± 1.2 kpc and a distance modulusm–M(SN1987A) = 18.55 ± 0.05. Allowing for a displacement of SN 1987A position relative to the LMC center, the distance to the barycenter of the Large Magellanic Cloud is also estimated to bed(LMC) = 52.0±1.3 kpc, which corresponds to a distance modulus ofm–M(LMC) = 18.58±0.05.


1961 ◽  
Vol 13 ◽  
pp. 29-41
Author(s):  
Wm. Markowitz
Keyword(s):  

A symposium on the future of the International Latitude Service (I. L. S.) is to be held in Helsinki in July 1960. My report for the symposium consists of two parts. Part I, denoded (Mk I) was published [1] earlier in 1960 under the title “Latitude and Longitude, and the Secular Motion of the Pole”. Part II is the present paper, denoded (Mk II).


1972 ◽  
Vol 1 ◽  
pp. 27-38
Author(s):  
J. Hers

In South Africa the modern outlook towards time may be said to have started in 1948. Both the two major observatories, The Royal Observatory in Cape Town and the Union Observatory (now known as the Republic Observatory) in Johannesburg had, of course, been involved in the astronomical determination of time almost from their inception, and the Johannesburg Observatory has been responsible for the official time of South Africa since 1908. However the pendulum clocks then in use could not be relied on to provide an accuracy better than about 1/10 second, which was of the same order as that of the astronomical observations. It is doubtful if much use was made of even this limited accuracy outside the two observatories, and although there may – occasionally have been a demand for more accurate time, it was certainly not voiced.


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