Sentence examples for 2 propagation from inspiring English sources

(2) Propagation paths are estimated from each snapshot of the channel measurements using a high-resolution parameter estimation.

A computationally efficient 3DHZETRN code with enhanced neutron and light ion (Z ≤ 2) propagation was recently developed for complex, inhomogeneous shield geometry described by combinatorial objects.

Material Propagation speed Air 3 × 108 m/s Silica sand 1.745 × 108 m/s Desert sand 1.89 × 108 m/s Table 2 Propagation speed values of materials found in BMI and MWI scan scenarios.

Although it is believed that Pi 2 pulsations or their source disturbances propagate as fast-mode waves in the low-latitude magnetosphere, direct evidence of Pi 2 propagation and its morphology have not been statistically established.

Table 2 Propagation scenarios considered in Monte Carlo simulations for L = 2   SNRd SNRc1 Scenarioenario 1 SNRd SNRd SNRd Scenario 2 SNRd SNRd + 10 dB SNRd Scenario 3 SNRd SNRd + 10 dB SNRd + 10 dB.

Next, we will eliminate the influence of the substrate on the guiding properties of the SHP on the substrate in an effective way. Figure 2 Propagation length and normalized modal area.

The fungus depends on the ants for: (1) supply of plant material essential for its growth; (2) propagation; (3) dispersion and (4) removal of invading microorganisms (weeding), whist the fungus is the sole source of nutrients for the queens, larvae and allates.

Numerical experiments include (1) propagation of a 1-D acoustic pulse without mean flow, (2) propagation of a 2-D acoustic pulse with/without mean flow, (3) reflection of an acoustic pulse from a flat plate with mean flow, and (4) flow-induced noise generated by the an unsteady laminar flow past a 2-D cavity.

(4) Propagation delay: the time for the signal to propagate through the copper-line.

The angular insertion loss of the mound is estimated by using the ISO 9613-2 propagation model, the Pierce barrier diffraction model and the Harmonoise point-to-point model.

WG3 has three subareas of study: 1) Dynamic solar emissions in the increasing and maximum portion of solar cycle 23; 2) Propagation in the interplanetary medium (coronal mass ejections, interplanetary shocks, and energetic particles); and 3) Interaction of coronal mass ejections and solar wind streams with Earth's magnetosphere.