Analysis three dispersion compensation techniques using DCF

Dispersion is one of the very important parameters that effect on the performance of optical fiber communication systems. It causes pulse broadening, limiting of transmission distance and low bit rate. Dispersion compensation fiber (DCF) is widespread used in the dispersion compensation scheme. In this paper, the suggested DCF included (pre–post-symmetrical) schemes with various bit rates (10–60 Gbit/s), and the positive dispersion accumulated over the length of the fiber at 100 km of optical fiber with 21.25 km of DCF. Optisystem software version 7 is used to design simulation model. The performances have been compared on the basis of parameters such as Q factor, bit error rate (BER) and eye height which used to evaluate the performance analysis of the system. We concluded that the symmetrical compensation techniques are better than the other compensation schemes when the Q factor is 14.9536 and BER is 1.759842.10−0.22, these at 60 Gbit/s and the input cw laser frequency equal 193.1 THz.

Constraining the fast radio burst properties using the joint distributions of dispersion measure and fluence of the events detected at Parkes, ASKAP, CHIME, and UTMOST

ABSTRACT The Parkes, ASKAP, CHIME, and UTMOST telescopes, which have all detected fast radio bursts (FRBs), each works at a different frequency and has a different detection criteria. Using simulations, we have combined the constraints from all four telescopes to identify an allowed range of model parameters $(\alpha , \overline{E}_{33})$ for the FRB source population. Here, α is the spectral index and $\overline{E}_{33}$ is the mean FRB energy in units of $10^{33} \, {\rm J}$ across a 2128–2848 MHz band in the FRB rest frame. We have considered several different FRB energy distributions, and also different scenarios for the scattering pulse broadening, the event rate density variation with z and the host dispersion measure (DM). We find that in all cases, the common allowed region includes the range −3.9 ≤ α ≤ −1.3 and $0.42\le \overline{E}_{33}\le 1$. In all case, large values α > 4 and $\overline{E}_{33} \gt 60$ are ruled out. Considering the allowed $(\alpha , \overline{E}_{33})$ parameter range, we predict that CHIME is unlikely to detect an FRB with extragalactic dispersion measure (DMEx) exceeding $3700\, {\rm pc\, cm}^{-3}$. A substantially larger DMEx in the large FRB sample anticipated from CHIME would falsify the assumptions of the present analysis. Our analysis is expected to yield tighter parameter constraints with the advent of more FRB data.

A population analysis of pulse broadening in ASKAP fast radio bursts

ABSTRACT The pulse morphology of fast radio bursts (FRBs) provides key information in both understanding progenitor physics and the plasma medium through which the burst propagates. We present a study of the profiles of 33 bright FRBs detected by the Australian Square Kilometre Array Pathfinder. We identify seven FRBs with measureable intrinsic pulse widths, including two FRBs that have been seen to repeat. In our modest sample, we see no evidence for bimodality in the pulse width distribution. We also identify five FRBs with evidence of millisecond time-scale pulse broadening caused by scattering in inhomogeneous plasma. We find no evidence for a relationship between pulse broadening and extragalactic dispersion measure. The scattering could be either caused by extreme turbulence in the host galaxy or chance propagation through foreground galaxies. With future high time resolution observations and detailed study of host galaxy properties, we may be able to probe line-of-sight turbulence on gigaparsec scales.

Enhancement of Signals Characteristics with Least Effect of Optical Communication Losses for Dense Optical Communication Systems

In this paper, the major aim is to enhance the bandwidth and therefore increase the capacity of the optical fibre communication system by reducing the dispersion in the fibre. Dispersion compensation is necessary to reduce losses and cost of the system. In this paper, we are basically focusing on reducing or decreasing chromatic dispersion. Chromatic dispersion is a type of dispersion in which pulse broadening occurs due to delay in different spectral components. We here make use of dispersion compensated fibre (DCF) for reducing the dispersion in the WDM system. Here, we basically use three dispersion compensated techniques (pre-compensation, post-compensation and mix compensation). The comparison in the three models of dispersion compensated technique is made in terms of transmission power vs. Q factor and also transmission power vs. Bit Error Rate.