scholarly journals On a relation between the refractive and dispersive constants of the inert gases

1927 ◽  
Vol 114 (769) ◽  
pp. 659-661
Keyword(s):  
Accurate Determination ◽  
Inert Gases ◽  
Critical Temperatures ◽  
Philosophical Magazine ◽  
Empirical Relations ◽  
Five Elements ◽  
Made In

In 1911 I published in the ‘Philosophical Magazine’ a paper on new determinations of some constants of the inert gases, and drew attention to the remarkable empirical relations which subsist between (1) the calculated numbers of “dispersion” electrons in the atoms of these five elements, (2) their “viscosity diameters” as determined by Prof. A. O. Rankine, and (3) their critical temperatures. Since that time the figures used have undergone revision. The accurate determination of the value of ε by Millikan has enabled us to give absolute, instead of relative, values to the apparent numbers of dispersion electrons ( q , see Table I). Chapman has recalculated the viscosity diameters, and Rankine has revised Chapman’s values, in the light of corrections to be made in his own values of Sutherland’s constants for argon, krypton and xenon. But these alterations have not affected the validity of the relations then published.

scholarly journals III. On the determination, at sea, of the specific gravity of sea-water

1875 ◽  
Vol 23 (156-163) ◽  
pp. 301-308 ◽  
Keyword(s):  
Specific Gravity ◽  
Physical Condition ◽  
Sea Water ◽  
Accurate Determination ◽  
Actual Difference ◽  
Made In

In the investigation of the physical condition of the ocean the accurate determination of the specific gravity of the water holds a first place. The tolerably numerous observations which have been made in this direction, in a more or less connected manner, are sufficient to prove that the density of the water varies, not only with the latitude and longitude, but also with the distance from the surface of the source from which it is taken. This difference of density depends partly on an actual difference in saltness, and partly on a difference in temperature of the water.

scholarly journals Discussion on the structure of atomic nuclei

1929 ◽  
Vol 123 (792) ◽  
pp. 373-390 ◽  
Keyword(s):  
Accurate Determination ◽  
Essential Point ◽  
Whole Numbers ◽  
Atomic Nuclei ◽  
Whole Number ◽  
Nuclear Atom ◽  
The Individual ◽  
The Masses ◽  
Made In

Sir Ernest Rutherford: It was on March 19, 1914, that the Royal Society held its last discussion on the constitution of the atom—just fifteen years ago. I had the honour to open the discussion on that occasion, and the other speakers were Mr. Moseley, Profs. Soddy, Nicholson, Hicks, Stanley Allen, S. P. Thomp­son. In my opening remarks I put forward the theory of the nuclear atom and the evidence in support of it, while Mr. Moseley gave an account of his X-ray investigations, which defined the atomic numbers of the elements, and showed how many gaps were present between hydrogen number 1 and uranium number 92. Prof. Soddy drew attention to the existence of isotopes in the radioactive series, and also to a remarkable observation by Sir Joseph Thomson and Dr. Aston, who had obtained two parabolas in the positive ray spectrograph of neon, and he suggested that possibly the ordinary elements might also consist of mixture of isotopes. I think you will find that the remarks and suggestions made in this discussion fifteen years ago have a certain pertinence to-day. In particular Hicks and Stanley Allen drew attention to the importance of taking into account the magnetic fields in the nucleus, although at that time we had very little evidence on that point, and even to-day our information is very scanty. What has been accomplished in the intervening period ? On looking back we see that three new methods of attack on this problem have been developed. The first, and in some respects the most important, has been the proof of the isotopic constitution of the ordinary elements, and the accurate determination of the masses or weights of the individual isotopes, mainly due to the work of Dr. Aston. This has led in a sense to an extension of the original ideas of Moseley. The experiments of the latter fixed the number of possible nuclear charges, while Aston has shown that there are a large number of species of atoms each defined by its nuclear charge, although their masses and their nuclear constitution may be different. The essential point brought out in the earlier work of Dr. Aston was that the masses of the elements are approxi­mately expressed by whole numbers, where oxygen is taken as 16—with the exception of hydrogen itself. But the real interest, as we now see it, is not the whole number rule itself, but rather the departures from it.

scholarly journals Derivation of the Rotational Frequency of Massive Stars from Seismic Studies

2004 ◽  
Vol 215 ◽  
pp. 199-204 ◽  
Author(s):  
C. Aerts ◽  
R. Scuflaire ◽  
A. Thoul
Keyword(s):  
Main Sequence ◽  
High Spatial Resolution ◽  
Massive Stars ◽  
Accurate Determination ◽  
Rotation Frequency ◽  
Rotational Frequency ◽  
Current Status ◽  
B Stars ◽  
Made In

In this contribution we review the current status of the determination of the rotational frequency in non-radially pulsating B stars, i.e. β Cep stars and slowly pulsating B stars. Considerable progress is currently being made in the understanding of the non-radial oscillations of main-sequence B stars by means of high-temporal, high-spatial resolution spectroscopic time series. This has led to the detection of frequency multiplets, which are interpreted as rotationally splitted non-radial modes and which allow an accurate determination of the surface rotational frequency in some stars. We outline how our future goal, i.e. the derivation of the internal rotation frequency, can be achieved.

scholarly journals II. Magnetic survey of the east of France in 1869

1872 ◽  
Vol 162 ◽  
pp. 7-27
Keyword(s):  
Accurate Determination ◽  
Magnetic Survey ◽  
Sources Of Information ◽  
The West ◽  
Mean Values ◽  
The City ◽  
Central Station ◽  
Previous Occasion ◽  
Made In

This survey, which occupied a considerable portion of the months of August and September 1869, is a continuation of the series of observations made in the west of France during the preceding year. The instruments used were the same on both occasions, the only changes made for the second expedition being (1°) the substitution of a theodolite by Jones in lieu of Cooke’s transit-theodolite, which was slightly too heavy for carrying in the hand, and (2°) the procuring, through the kindness of Dr. Stewart, a second tripod stand similar to our own, which rendered the series of observations with two observers much more rapid than on the previous occasion. The observations were undertaken, as before, by the Rev. W. Sidgreaves and myself, the Vibrations and Deflections falling to his share, and the Declination and Chronometer comparisons remaining in my hands, whilst the Dip was in general observed by both. The method of reduction is almost identical with that adopted for the observations taken in the west of France. The geographical positions of the different stations have been calculated, as far as possible, from the data given in the 'Connaissance des Temps,’ but where this could not be done I have had recourse to the most reliable sources of information at my command. For the accurate determination of the positions of Mont Rolland (near Dôle), of N. D. de Myans (near Chambéry), of Mongré (near Villefranche-sur-Soane), of Iseure (near Moulins), and of our station at Marseilles I am indebted to the kindness of the Rev. N. Larcher, S. J., Membre de la Société Météorologique de France. The coordinates of Vaugirard were readily obtained from a good map of Paris, and for Issenheim and Monaco I have to depend on Cassini’s ‘Carte Générale de la France’ and on Philip’s 'Imperial Atlas.’ The Imperial Observatory at Paris is chosen as the natural position for the origin of coordinates, in lieu of our central station of observation at Vaugirard, which lies on the outskirts of the city; the resulting mean values will thus require no correction, and will be immediately comparable with those of most other observers.

Glomerular permeability in the fetal rabbit

1978 ◽  
Vol 36 (2) ◽  
pp. 681A-681B ◽  
Author(s):  
M. L. Monica ◽  
M. L. Zimny ◽  
S. G. McClugage
Keyword(s):  
New Zealand ◽  
Age Differences ◽  
Accurate Determination ◽  
Ethyl Carbamate ◽  
Lower Abdomen ◽  
Glomerular Permeability ◽  
Small Incision ◽  
New Zealand White Rabbits ◽  
Made In

The purpose of this study was to determine fetal age differences in glomerular permeability using a graded series of dextrans (Pharmacia, Inc., Uppsala, Sweden). The dextran fractions were highly purified and consisted of the following sizes: T-10, T-40 and T-110 (10,000, 40,000 and 110,000 M.W. respectively). The foundation for this study was the work of Caulfield and Farquhar, who showed, using a graded series of dextrans, that the basement membrane was the definitive barrier to permeability.A total of 120 fetuses of pregnant New Zealand white rabbits at the following periods of gestation: 20, 22, 24, 28 days and one day old neonates were utilized. Accurate determination of each fetus' developmental stage was based on weight and crown-rump measurements made at the time of sacrifice. Pregnant rabbits were anesthesized with 20% urethane (ethyl carbamate) and a longitudinal incision was made in the shaved lower abdomen. A small incision was placed in the exposed uterus which penetrated the amniotic sac allowing for removal of the fetus. Viability of the fetus was essential and each fetus remained attached to the placenta throughout the course of dextran injection.

THE IEC METHOD AND CONVERSION COEFFICIENTS OF THE 605-keV TRANSITION IN 134Ba

1966 ◽  
Vol 44 (3) ◽  
pp. 549-562 ◽  
Author(s):  
E. F. Zganjar ◽  
J. H. Hamilton
Keyword(s):  
Beta Decay ◽  
Photon Energy ◽  
Conversion Coefficient ◽  
Theoretical Calculations ◽  
Accurate Determination ◽  
A Value ◽  
Conversion Coefficients ◽  
Double Focusing ◽  
Made In

Tests of the internal–external method of measuring conversion coefficients in the Vanderbilt double-focusing spectrometer have been made in search of possible errors arising from scattering of photoelectrons in the converter for a photon energy of 605 keV. This scattering may affect the factor, f, which corrects for the anisotropic distribution of the photoelectrons. The 605-keV transition in 134Ba populated by the beta decay of 134Cs was used. An accurate determination of the K, L, and M conversion coefficients of the 2+ to 0+, 605-keV, E2 transition in 134Ba was made. Three uranium converters 1.12, 2.19, and 3.71 mg/cm2 thick were used. The results are compared with the new theoretical calculations of f which depend on the converter thickness and consequently consider the effect of scattering. For photons of energy 605 keV or greater, the IEC method used in the Vanderbilt double-focusing spectrometers is insensitive (< 5%) to scattering in uranium converters < 4 mg/cm2 thick. The K, L, and M conversion coefficients were determined to be (5.03 ± 0.20) × 10−3, (7.07 ± 0.50) × 10−4, and (1.64 ± 0.18) × 10−4, respectively. The respective theoretical values of Rose are 5.08 × 10−3, 6.92 × 10−4, and 2.77 × 10−4. Sliv and Band give a value of 5.10 × 10−3 for the K conversion coefficient.

scholarly journals VIII.—On Impact

1892 ◽  
Vol 36 (1) ◽  
pp. 225-252 ◽  
Author(s):  
Tait
Keyword(s):  
Accurate Determination ◽  
Golf Ball ◽  
Complete Proof ◽  
Permanent Record ◽  
The Impact ◽  
Made In

The present inquiry is closely connected with some of the phenomena presented in golf:—especially the fact that a ball can be “jerked” nearly as far as it can be “driven.” For this, in itself, furnishes a complete proof that the duration of the impact is exceedingly short. But it does not appear that any accurate determination of the duration can be made in this way. Measurements, even of a rude kind, are impracticable under the circumstances.In 1887 I made a number of preliminary experiments with the view of devising a form of apparatus which should trace a permanent record of the circumstances of impact. I found that it was necessary that one of the two impinging bodies should be fixed:—at least if the apparatus were to be at once simple and manageable. This arrangement gives, of course, a result not directly comparable with the behaviour of a golf-ball. For pressure is applied to one side only, both of ball and of club; but when one of two impinging bodies is fixed it is virtually struck simultaneously on both sides.

scholarly journals Usefulness of Selected Incisor Characteristics for Determining the Age of Hucul Horses

2011 ◽  
Vol 11 (4) ◽  
pp. 569-575 ◽  
Author(s):  
Jarosław Łuszczyński ◽  
Magdalena Pieszka
Keyword(s):  
Accurate Determination ◽  
Age Groups ◽  
Age Determination ◽  
Occlusal Surface ◽  
Made In

Usefulness of Selected Incisor Characteristics for Determining the Age of Hucul HorsesThe aim of this study was to assess the suitability of selected characteristics of incisors for age determination in Hucul horses. The study included 173 Hucul horses (137 mares, 28 stallions and 8 geldings) from one day to 27 years of age. Breeding documentation was used to determine the actual age of the horses, which were then divided into age groups. Each group of horses was assigned a specific incisor characteristic to help identify their age. Selected incisor characteristics were used to evaluate the age of the horses according to the method reported by Pruski (2007) and the results were compared with the actual age, indicating the percentage of errors made. It was found that most errors were made in the case of horses over 11 years old, when assessing the changing shape of the occlusal surface of incisors (Table 1). In this group the percentage of errors was significantly higher (P≤0.01) than that found for horses from the first three youngest age groups, in which the eruption time of deciduous incisors, the disappearance of cups on deciduous incisors and the eruption time of permanent incisors were taken into account. Compared to the above traits, errors were made significantly more often (P≤0.01) when age was determined based on the disappearance of permanent incisors, in a group of horses aged between 6 and 11 years. The eruption time of deciduous incisors and permanent incisors were the traits which enabled the most accurate determination of the horses' age. The results obtained suggest that age determination based on dentition is not accurate enough and can only play a subsidiary role, for example when no breeding records are available.

scholarly journals VLBI Observations of Turbulence in the Inner Solar Wind

1996 ◽  
Vol 154 ◽  
pp. 65-75
Author(s):  
Steven R. Spangler
Keyword(s):  
Solar Wind ◽  
Accurate Determination ◽  
The Sun ◽  
Long Baseline ◽  
Vlbi Observations ◽  
Outer Corona ◽  
Very Long Baseline Array ◽  
Made In

AbstractI discuss the use of Very Long Baseline Interferometer (VLBI) phase scintillations to probe the conditions of plasma turbulence in the solar wind. Specific results from 5.0 and 8.4 GHz observations with the Very Long Baseline Array (VLBA) are shown. There are several advantages of phase scintillation measurements. They are sensitive to fluctuations on scales of hundreds to thousands of kilometers, much larger than those probed by IPS intensity scintillations. In addition, with the frequency versatility of the VLBA one can measure turbulence from the outer corona ~ 5 –10 R⊙ to well past the perihelion approach of the Helios spacecraft. This permits tests of the consistency of radio propagation and direct in-situ measurements of turbulence. Such a comparison is made in the present paper. Special attention is dedicated to measuring the dependence of the normalization coefficient of the density power spectrum, on distance from the sun. Our results are consistent with the contention published several years ago by Aaron Roberts, that there is insufficient turbulence close to the sun to account for the heating and acceleration of the solar wind. In addition, an accurate determination of the relationship could aid the detection of transients in the solar wind.

I. On the determination of the specific resistance of mercury in absolute measure

1891 ◽  
Vol 48 (292-295) ◽  
pp. 434-437
Keyword(s):  
Specific Resistance ◽  
Accurate Determination ◽  
Considerable Time ◽  
Absolute Measure ◽  
University College ◽  
Complete Sets ◽  
The University ◽  
Made In ◽  
The Way

In the hope of paving the way for a more accurate determination of the ohm, the author has for a considerable time been engaged in submitting to the test of experiment certain modifications of the method of Lorenz which occurred to him as likely to lead to increased accuracy and certainty. The experiments have been made in the laboratory of the University College, Cardiff, with apparatus for the most part constructed in the College workshop. Five complete sets of observations were taken in the spring of this year, with the following results for the specific resistance of mercury at 0ºC.

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