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Table 1: Parameters of best fits using the modified two-ray model with corresponding rms errors wrt measured data. r = MS receding from the BS, a = MS approaching the BS.
"... In PAGE 3: ...4 dB. For the 18 street sections that were studied, model parameters for the best fits with the associated rms modelling errors are shown in Table1 . The value of h0 was in the range of 0.... ..."
Cited by 3
Table 1: Parameters used in ns-2 simulations. Propagation Two-ray Antenna height 1.5 m
2006
"... In PAGE 8: ...11 DCF [16], we have carried out simulation in ns-2 in a variety of network scenarios. Table1 gives the default parameter setting used in the simulation study. With the parameter setting the transmission range is approximately 100 m and the carrier sense range is 220 m.... ..."
Cited by 7
Table 2: Results of direct 3D point determination at independent check points (ICP) using two-ray points and single reference stations, image scale 1:10.000
Table 3: Results of direct 3D point determination at independent check points (ICP) using two-ray points and single reference stations and the network solution, individual strips, image scale 1:10.000
Table 1. Simulation parameters. Receiver threshold Distance
2005
"... In PAGE 3: ... 3. The carrier sense range is 1783 meters which is slightly greater than 5 hops distance, and other parameters are given in Table1 . We have a 3-hop CBR flow running in the center of the grid.... In PAGE 5: ...ixed at 15 dbm. RTS/CTS is disabled 2. ACKs are trans- mitted using the basic rate of 1 Mbps. The receiver thresh- olds and the corresponding effective distances are shown in Table1 , which are obtained by using the two-ray ground reflection propagation model [8]. Table 1.... ..."
Cited by 7
Table 5.2: Labelling a face 5.4.3.4 A Labelling Example The intersection of two cubes example of Figure 5.2 requires four rays to be cast in order to label the entire object. The rst two rays label the faces of ObjectA, and the second two the faces of ObjectB. The results of these four rays can be propagated to all
1995
Cited by 7
Table 1: Clown face model ratios, = 0:5.
1996
"... In PAGE 2: ... We instrumented both the initial and modi ed ray tracer to record the number of calls to Intersect and Shade. Table1 presents the results for the clown model with 1ivray was developed for the MIT undergraduate graphics course 6.837.... In PAGE 2: ... Figure 4 presents the regions where the alias- ing tests fail and cause ner subdivision of the linetree2. In Table1 , the second column presents the ratio of Intersect calls made by the interpolant algorithm to those made by the unmodi ed ray tracer. The third column presents the ratio of Shade calls made by the two ray tracers.... ..."
Cited by 17
Table 4. Amplitude of Fluctuations, a7 8
"... In PAGE 9: ... Once the redshift distribution of the background galaxies is known, this technique directly probes gravitational potential fluctuations, and therefore can be easily compared with our CMB model pre- dictions for the amplitude of dark matter fluctuations. Several groups have reported weak shear measure- ments within the past year (see Table4 and Van Waerbeke et al. (2002a) for recent review): while there is significant scatter in the reported amplitude, the best fit model to the WMAP data lies in the middle of the reported range.... ..."
Table 1: Physical layer and propagation models available in GloMoSim, ns-2 and OPNET
2001
"... In PAGE 2: ... 2.4 Physical layer models of common simulation tools Table1 summarizes the physical layer models currently available in GloMoSim (2.02), ns-2 (2.... ..."
Cited by 78
Table 1: Physical layer and propagation models available in GloMoSim, ns-2 and OPNET
2001
"... In PAGE 2: ... 2.4 Physical layer models of common simulation tools Table1 summarizes the physical layer models currently available in GloMoSim (2.02), ns-2 (2.... ..."
Cited by 78
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