The influence of the major and minor foramen diameters on apical electronic probe measurements

1990 ◽  
Vol 16 (11) ◽  
pp. 520-522 ◽  
Author(s):  
Thomas John Stein ◽  
John F. Corcoran ◽  
Richard M. Zillich
1979 ◽  
Vol 62 (1) ◽  
pp. 69-73 ◽  
Author(s):  
R.H. Foote ◽  
E.A.B. Oltenacu ◽  
J. Mellinger ◽  
N.R. Scott ◽  
R.A. Marshall

1989 ◽  
Vol 54 (13) ◽  
pp. 1212-1214 ◽  
Author(s):  
R. J. von Gutfeld ◽  
R. W. Dreyfus

1992 ◽  
Vol 72 (2) ◽  
pp. 237-244 ◽  
Author(s):  
S. D. M. Jones ◽  
L. E. Jeremiah ◽  
A. K. W. Tong ◽  
W. M. Robertson ◽  
L. L. Gibson

Sixteen hundred and sixty lambs were used to determine the precision of carcass measurements (fat thickness, muscle thickness, tissue depth) and a visual scoring system for muscle and fat thickness to estimate carcass composition. Measurements of fat (F) and muscle (M) thickness were made in warm and cold carcasses and total tissue depth in warm carcasses only between the 10th and 11th ribs and the 12th and 13th ribs using an electronic probe (Hennessy Grading Probe HGP). F explained 40–64% of the variation in carcass lean and 44–72% of the variation in carcass fat depending on the location and number of measurements and whether they were made on a warm or cold carcass. In most cases when M was added to F there was no increase in the variation explained in composition over that provided by F alone. Total tissue depth measurements differed in precision for the prediction of carcass lean content with the 12th rib being superior to the 10th rib (RSD for 12th rib, 33.2 g kg−1; 10th rib, 36.6 g kg−1). Visual assessment of carcasses for fatness had the lowest precision for the prediction of lean content (RSD, 44.5 g kg−1). Loin eye area and fat thickness measured at the 12th rib had similar precision for the estimation of lean content as probe measurements. It was concluded that probe measurements of F or tissue depth between the 12th and 13th ribs would provide a superior method to the visual assessment of carcass fatness used in this study for classifying lamb carcasses for lean content and would allow carcasses to be graded on the slaughter floor. Key words: Lamb, carcass, grading, Hennessy Grading Probe, composition


1989 ◽  
Vol 69 (3) ◽  
pp. 641-648 ◽  
Author(s):  
S. D. M. JONES ◽  
A. K. W. TONG ◽  
W. M. ROBERTSON

Five hundred and thirty-one beef carcasses were used to establish if Hennessy Grading Probe (HGP) measurements provided a more accurate assessment of carcass lean content than a visual scoring system or linear carcass measurements. Carcasses were probed at the 5th/6th, 11th/12th, 12th/13th ribs, 2nd/3rd lumbar and sacral crest position (P8). Carcasses were then visually appraised for overall fat cover and muscle thickness. Following 24 h of cooling, the measurements by HGP and visual scores were repeated. Fat thickness and loin eye area were recorded at the 12th rib. Precision for the prediction of carcass lean by HGP was similar in warm or cold carcasses and the lowest error of prediction for the probe was associated with measurements made at the 12th/13th rib (RSD 31.8 g kg−1). A combined visual score for overall fat cover and muscle thickness was more precise (RSD 28.6 g kg−1) than probe measurements for predicting lean yield in warm and cold carcasses. Canada grade had the lowest precision (RSD 34.7 g kg−1) for predicting lean yield, but measurements of average fat thickness and loin eye area at the 12th rib gave the best overall prediction (RSD 27.1 g kg−1) of carcass lean content. It was concluded that the HGP provided a method to classify warm carcasses for lean content, but the improvement in precision over conventional grading procedures was not large. Key words: Beef, carcass, grading, Hennessy grading probe, composition


1987 ◽  
Vol 67 (1) ◽  
pp. 209-212 ◽  
Author(s):  
W. R. USBORNE ◽  
D. MENTON ◽  
I. McMILLAN

The Destron PG-100 electronic grading probe was evaluated for prediction of lean yield, comparison with the ruler measurement, and precision on 204 pork carcasses representing equal numbers of barrows and gilts and a warm carcass weight range of 56.8–111.4 kg. A complete cutout was done on the left side from each carcass to determine a regression equation for prediction of lean yield from the probe measurements of thickness of fat and muscle between the 3rd and 4th last rib, 7 cm off the mid-line. The Hennessy probe was used as the standard for this study. Both probes performed equally well when compared with the ruler measurement and in their ability to predict lean yield. Key words: Electronic grading, pork carcasses, pork grading


2013 ◽  
Vol 19 (5(84)) ◽  
pp. 16-26
Author(s):  
V.A. Shuvalov ◽  
◽  
D.N. Lazuchenkov ◽  
S.V. Nosikov ◽  
G.S. Kochubey ◽  
...  

2003 ◽  
Vol 770 ◽  
Author(s):  
Nathanael Smith ◽  
Max J. Lederer ◽  
Marek Samoc ◽  
Barry Luther-Davies ◽  
Robert G. Elliman

AbstractOptical pump-probe measurements were performed on planar slab waveguides containing silicon nanocrystals in an attempt to measure optical gain from photo-excited silicon nanocrystals. Two experiments were performed, one with a continuous-wave probe beam and a pulsed pump beam, giving a time resolution of approximately 25 ns, and the other with a pulsed pump and probe beam, giving a time resolution of approximately 10 ps. In both cases the intensity of the probe beam was found to be attenuated by the pump beam, with the attenuation increasing monotonically with increasing pump power. Time-resolved measurements using the first experimental arrangement showed that the probe signal recovered its initial intensity on a time scale of 45-70 μs, a value comparable to the exciton lifetime in Si nanocrystals. These data are shown to be consistent with an induced absorption process such as confined carrier absorption. No evidence for optical gain was observed.


1989 ◽  
Vol 20 (2) ◽  
pp. 109-122 ◽  
Author(s):  
Lotta Andersson

Some commonly used assumptions about climatically induced soil moisture fluxes within years and between different parts of a region were challenged with the help of a conceptual soil moisture model. The model was optimised against neutron probe measurements from forest and grassland sites. Five 10 yrs and one 105 yrs long climatic records, from the province of Östergötland, situated in south-central Sweden, were used as driving variables. It was concluded that some of the tested assumptions should not be taken for granted. Among these were the beliefs that interannual variations of soil moisture contents can be neglected in the beginning of the hydrological year and that soils usually are filled up to field capacity after the autumn recharge. The calculated climatic induced dryness was estimated to be rather insensitive to the choice of climatic stations within the region. Monthly ranges of soil moisture deficits (1883-1987) were shown to be skewed and it is therefore recommended to use medians and standard deviations in statistical analyses of “normal” ranges of soil moisture deficits.


Author(s):  
O. Mousis ◽  
D. H. Atkinson ◽  
R. Ambrosi ◽  
S. Atreya ◽  
D. Banfield ◽  
...  

AbstractRemote sensing observations suffer significant limitations when used to study the bulk atmospheric composition of the giant planets of our Solar System. This impacts our knowledge of the formation of these planets and the physics of their atmospheres. A remarkable example of the superiority of in situ probe measurements was illustrated by the exploration of Jupiter, where key measurements such as the determination of the noble gases’ abundances and the precise measurement of the helium mixing ratio were only made available through in situ measurements by the Galileo probe. Here we describe the main scientific goals to be addressed by the future in situ exploration of Saturn, Uranus, and Neptune, placing the Galileo probe exploration of Jupiter in a broader context. An atmospheric entry probe targeting the 10-bar level would yield insight into two broad themes: i) the formation history of the giant planets and that of the Solar System, and ii) the processes at play in planetary atmospheres. The probe would descend under parachute to measure composition, structure, and dynamics, with data returned to Earth using a Carrier Relay Spacecraft as a relay station. An atmospheric probe could represent a significant ESA contribution to a future NASA New Frontiers or flagship mission to be launched toward Saturn, Uranus, and/or Neptune.


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