In satellite–ground laser communications, atmospheric turbulence in the link degrades the performance of the system, so it is very important to estimate its influence on the performance of the system. The bit-error rate (BER) is an important parameter to indicate the communication performance of the system, which is directly used to judge the quality of the communication system. Using the results of our two previous papers, we analyze the joint influence of Kolmogorov turbulence from the ground up to 6 km and non-Kolmogorov turbulence above 6 km on the BER. These kinds of turbulence are associated respectively with the uplink and the downlink propagation channels for the geosynchronous orbit satellite communication system. 相似文献
The quercetin molecularly imprinted polymer microspheres were prepared by reversible addition-fragmentation chain transfer free radical polymerization combined with precipitation method (RAFTPP) with the dibenzyl trithiocarbonate (DBTTC) as RAFT reagent and quercetin as template molecule. The effects of solvents and cross-linking agent on the morphology and size of polymers were investigated, and the polymers were preliminarily screened by scanning electron microscope. The adsorption experiment and adsorption model analysis were carried out on the molecularly imprinted polymers (R-MIP) prepared under optimal condition and on the molecularly imprinted polymers prepared with a traditional precipitation polymerization (T-MIP). Consequently it was determined that, QR-MIP max was 37.71 mg g?1 and QT-MIP max was 29.61 mg g?1. The results showed that the R-MIP had a good adsorptive property and was obviously superior to T-MIP. R-MIP was used as solid-phase extraction filler in combination with the HPLC method to conduct enrichment, separation and measurement of the quercetin in honeysuckle and clove leaves, which effectively removed the matrix interference and the recovery rate of this method was 93.8–102.9%.
We investigate the out of equilibrium dynamics of global chiral supersymmetry at finite energy density. We concentrate on two specific models. The first is the massive Wess–Zumino model which we study in a self-consistent one-loop approximation. We find that for energy densities above a certain threshold, the fields are driven dynamically to a point in field space at which the fermionic component of the superfield is massless. The state, however, is found to be unstable, indicating a breakdown of the one-loop approximation. To investigate further, we consider an O(N) massive chiral model which is solved exactly in the large N limit. For sufficiently high energy densities, we find that for late times the fields reach a nonperturbative minimum of the effective potential degenerate with the perturbative minimum. This minimum is a true attractor for O(N) invariant states at high energy densities, and this provides a mechanism for determining which of the otherwise degenerate vacua is chosen by the dynamics. The final state for large energy density is a cloud of massless particles (both bosons and fermions) around this new nonperturbative supersymmetric minimum. By introducing boson masses which softly break the supersymmetry, we demonstrate a see-saw mechanism for generating small fermion masses. We discuss some of the cosmological implications of our results. 相似文献