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GRID calibrating

No, that is not all. You can tell that the —CH2— protons and the —CH3 protons split each other by their coupling constant, the distance between the split peaks of a single group. Coupling constants are called J values, and are usually given in hertz (Hz). You can read them right from the chart, which has a grid calibrated in hertz. If you find protons at different chemical shifts... [Pg.286]

Figure 7. Calibration (O) and validation ( ) plots of glucose in bovine plasma on Clarke error grid. Calibration plot was constructed using 92 data points and validation plot was constructed using 46 data points. Sample was incubated for 2 min in glucose concentrations ranging from 10 - 450 mg/dl with Aex = 785 nm, laser power = 10-30 mW, t= 2 min. RMSEC = 34.3 m dL (1.9 mM) and RMSEP = 83.16 mg/dL (4.62 mM). Reproduced with permission from ref. 10 Copyright 2005 J. Am. Chem. Soc. Figure 7. Calibration (O) and validation ( ) plots of glucose in bovine plasma on Clarke error grid. Calibration plot was constructed using 92 data points and validation plot was constructed using 46 data points. Sample was incubated for 2 min in glucose concentrations ranging from 10 - 450 mg/dl with Aex = 785 nm, laser power = 10-30 mW, t= 2 min. RMSEC = 34.3 m dL (1.9 mM) and RMSEP = 83.16 mg/dL (4.62 mM). Reproduced with permission from ref. 10 Copyright 2005 J. Am. Chem. Soc.
There are several improvements that can be made to the present calibration procedure. First of all the numerical grid in the DST model can be adjusted to yield more accurate results for short time step data. Secondly the accuracy of the calibration can be increased. At present error for any time step of the calibrated temperatures is A0.2-0.4 K, this should probably be decreased to about 0.1-0.2 K. [Pg.191]

Depending on purposes, a plastic film under the vapor-deposited C is dissolved away with a solvent. By this method, a very thin C support-film of smaller than lOnm in thickness can be made easily. An aluminum (Al) support-film can be made similarly, by vapor-deposition of Al onto a plastic film put on a grid and then by dissolving away the plastic film. The reflection rings from the Al support-film can be used as an internal reference to calibrate the camera length of SAED pattern, and this support film does give no amorphous halo. When an ultra-thin C support-film (less than 5nm in thickness) is desired, a microgrid (MG see Section 3.1.2) should be used on which an ultra-thin film made by indirect vapor-deposition of C has been put in advance. [Pg.459]

Fig. 4.25 Map of the locations of an adatom on a W (110) surface after about 300 heating periods. Each dot represents an observed location of the adatom. Only a fraction of the about 300 locations are shown. These dots are clustered, and the clustery are found to register with slightly curved grid lines parallel to the [111] and [111] surface channel directions. Using this map, the length calibration can then be done accurately from the known size of the surface channels. Fig. 4.25 Map of the locations of an adatom on a W (110) surface after about 300 heating periods. Each dot represents an observed location of the adatom. Only a fraction of the about 300 locations are shown. These dots are clustered, and the clustery are found to register with slightly curved grid lines parallel to the [111] and [111] surface channel directions. Using this map, the length calibration can then be done accurately from the known size of the surface channels.
Fig. 2. Mass spectrometer with photoionization 1—built-in hydrogen lamp 2—vacuum monochromator filled with hydrogen 3—LiF window 4—ionic source container 5—photoionization space with the accelerating grids 6—fluorescent layer for intensity calibration of the incident u.v. light 7—photomultiplier 8—magnetic mass analyzer 9—electron multiplier. Fig. 2. Mass spectrometer with photoionization 1—built-in hydrogen lamp 2—vacuum monochromator filled with hydrogen 3—LiF window 4—ionic source container 5—photoionization space with the accelerating grids 6—fluorescent layer for intensity calibration of the incident u.v. light 7—photomultiplier 8—magnetic mass analyzer 9—electron multiplier.
In both the Dunmore and Pope sensors, the element is arranged in an ae-excited Wheatstone bridge so that only allcmating current Hows through the grid. Direct current excitation of either the Dunmore or Pope elements polarizes Ihe sensor, eventually causing loss ol calibration. [Pg.812]

Radiant Flux Dependence. Radiant flux can be measured by utilizing calibrated metallic grids and neutral density filters, or by filtering solutions of various absorbances without changing the geometry of the irradiating beam. For low radiant fluxes , a linear relation between the reaction rate and

values, the rate becomes proportional to... [Pg.90]

This calibration is to be performed with 3 or more replicate samples. The volume of the solution delivered to the planchets should be between 1 mL and 100 X. (The volume used should allow the solution to remain within the location of the usual sample deposit, a radius of about 0.5 cm from the center of the planchet. If the volume used is too large, it will encourage excessive spreading on the planchet.) These samples are dried under a heat lamp. Then, the dried residue is fixed on the surface of the disk by gently flaming the disk over a Meeker burner flame. (Note A Meeker burner is different from a Bunsen burner in that it bums hotter and has a metal grid over the flame that causes the flame and heat from the burner to vibrate as the fuel burns.)... [Pg.48]

The identification of size, shape, and axial ratio can also be done by direct observation in the electron microscope (EM). This is accomplished by depositing single molecules (if they can be obtained) directly on polymer-coated copper grids and then shadowing them with heavy metals or making a replica of the molecular surface on mica. The sample can then be viewed in the transmission EM and photographs can then be taken after calibration of the magnification factor. [Pg.135]

Demyshev SG, Korotaev GK (1992) Numerical energy-balanced model of baroclinic currents in no-flat-bottom ocean on C-grid. In Numerical models and results of calibration calculation of the Atlantic Ocean currents. INM RAS, Moscow, p 163... [Pg.194]

Application of the Hatch equations to a screen analysis is as follows A summation curve is plotted on log-probability grid. The percentage less than calibrated sieve-size is plotted instead of the usual percentage less than stated sieve-size. If the summation curve is a straight line, Eq (5-9) applies. The method is useful where precise information is desired on particle-size of a screened product. [Pg.118]


See other pages where GRID calibrating is mentioned: [Pg.190]    [Pg.190]    [Pg.487]    [Pg.487]    [Pg.244]    [Pg.403]    [Pg.341]    [Pg.537]    [Pg.20]    [Pg.290]    [Pg.133]    [Pg.317]    [Pg.224]    [Pg.163]    [Pg.111]    [Pg.720]    [Pg.22]    [Pg.20]    [Pg.142]    [Pg.143]    [Pg.143]    [Pg.144]    [Pg.145]    [Pg.487]    [Pg.278]    [Pg.267]    [Pg.248]    [Pg.258]    [Pg.349]    [Pg.470]    [Pg.230]    [Pg.261]    [Pg.435]    [Pg.435]    [Pg.117]    [Pg.106]    [Pg.144]    [Pg.256]    [Pg.135]   
See also in sourсe #XX -- [ Pg.16 ]




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Calibrating the GRID Force Field

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