Deck 14: Optical Fiber Measurements

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Optical spectrum analyzers directly measure the wavelength of light in an air environment. However, most wavelength measurements are quoted in terms of wavelengths or optical frequencies in a vacuum. This can lead to errors, particularly in DWDM systems, since the index of refraction of air is a function of wavelength, temperature, pressure, and gas composition. The wavelength dependence of the index of refraction n air of standard dry air at 760 torr and 15°C is 64 Optical spectrum analyzers directly measure the wavelength of light in an air environment. However, most wavelength measurements are quoted in terms of wavelengths or optical frequencies in a vacuum. This can lead to errors, particularly in DWDM systems, since the index of refraction of air is a function of wavelength, temperature, pressure, and gas composition. The wavelength dependence of the index of refraction n air of standard dry air at 760 torr and 15°C is 64   where is measured in micrometers. ( a ) Given that vacuum = air n air , what is the error in wavelength measurement at 1550 nm if the effect of the index of refraction of air is ignored What impact would this have on 0.8-nm-spaced WDM channels in the 1550-nm window ( b ) To compensate for temperature and pressure effects on the value of n air , one can use the relationship   where P is measured in torr and T is in Celsius. How much does n (T, P) vary from n air when the pressure is 640 torr and the temperature is 0°C (which would be at a higher elevation and a lower temperature)<div style=padding-top: 35px>
where is measured in micrometers.
( a ) Given that vacuum = air n air , what is the error in wavelength measurement at 1550 nm if the effect of the index of refraction of air is ignored What impact would this have on 0.8-nm-spaced WDM channels in the 1550-nm window
( b ) To compensate for temperature and pressure effects on the value of n air , one can use the relationship Optical spectrum analyzers directly measure the wavelength of light in an air environment. However, most wavelength measurements are quoted in terms of wavelengths or optical frequencies in a vacuum. This can lead to errors, particularly in DWDM systems, since the index of refraction of air is a function of wavelength, temperature, pressure, and gas composition. The wavelength dependence of the index of refraction n air of standard dry air at 760 torr and 15°C is 64   where is measured in micrometers. ( a ) Given that vacuum = air n air , what is the error in wavelength measurement at 1550 nm if the effect of the index of refraction of air is ignored What impact would this have on 0.8-nm-spaced WDM channels in the 1550-nm window ( b ) To compensate for temperature and pressure effects on the value of n air , one can use the relationship   where P is measured in torr and T is in Celsius. How much does n (T, P) vary from n air when the pressure is 640 torr and the temperature is 0°C (which would be at a higher elevation and a lower temperature)<div style=padding-top: 35px>
where P is measured in torr and T is in Celsius. How much does n (T, P) vary from n air when the pressure is 640 torr and the temperature is 0°C (which would be at a higher elevation and a lower temperature)
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Question
An engineer wants to find the attenuation at 1310 nm of an 1895-m long fiber. The only available instrument is a photodetector, which gives an output reading in volts. Using this device in a cutback-attenuation setup, the engineer measures an output of 3.31 V from the photodiode at the far end of the fiber. After cutting the fiber 2 m from the source, the output voltage from the photodetector now reads 3.78 V What is the attenuation of the fiber in dB/km
Question
Consider the cutback attenuation measurement technique described by Eq. (14.2) using a photodetector, the power measurements are proportional to the detector output voltage. If the uncertainty in the voltage readings for the two power measurements are ±0.1 percent each, what is the uncertainty in the attenuation accuracy How long must the fiber be to get a sensitivity better than ±0.05 dB/km
Question
Verify that the full-width at half-maximum of a gaussian pulse is given by t FWHM = 2(2 ln 2) 1/2.
( b ) Derive Eq. (14.11), which describes the 3-dB bandwidth of a fiber based on a gaussian output response.
Question
A gaussian approximation of | H ( f )| in the form A gaussian approximation of | H ( f )| in the form   has been found to be accurate to at least the 0.75-amplitude point in the frequency domain. Using this relationship, plot P( f)/P(t) as a function of frequency from 0 to 1000 MHz for fibers that have impulse responses of full rms pulse widths 2 equal to 2.0, 1.0, and 0.5 ns. What are the 3-dB bandwidths of these fibers<div style=padding-top: 35px>
has been found to be accurate to at least the 0.75-amplitude point in the frequency domain. Using this relationship, plot P( f)/P(t) as a function of frequency from 0 to 1000 MHz for fibers that have impulse responses of full rms pulse widths 2 equal to 2.0, 1.0, and 0.5 ns. What are the 3-dB bandwidths of these fibers
Question
Consider the data shown in Fig. 14.37 of the group delay versus wavelength for a 10-km long fiber. From this data, plot the chromatic dispersion D as a function of wavelength. What is the value of the zero-dispersion slope S 0 in the relationship D() = S 0 ( 0 ) Consider the data shown in Fig. 14.37 of the group delay versus wavelength for a 10-km long fiber. From this data, plot the chromatic dispersion D as a function of wavelength. What is the value of the zero-dispersion slope S 0 in the relationship D() = S 0 ( 0 )   Fig. 14.37 Chromatic-dispersion measurement of a 10-km fiber<div style=padding-top: 35px>
Fig. 14.37 Chromatic-dispersion measurement of a 10-km fiber
Question
Determine the value of the expected differential group delay from the polarization-mode- dispersion measurement response shown in Fig. 14.38 for a non-mode-coupled fiber. Determine the value of the expected differential group delay from the polarization-mode- dispersion measurement response shown in Fig. 14.38 for a non-mode-coupled fiber.   Fig. 14.38 PMD-inducedpowerexcursions about the mean power level (dashed line)<div style=padding-top: 35px>
Fig. 14.38 PMD-inducedpowerexcursions about the mean power level (dashed line)
Question
The influence of polarization-mode dispersion can be neglected for data rates up to a few Gb/s for intensity-modulated direct-detection systems. However, for higher rates, PMD can cause intersymbol interference (ISI) in long- span links. The ISI power penalty in decibels for PMD is approximately 65 The influence of polarization-mode dispersion can be neglected for data rates up to a few Gb/s for intensity-modulated direct-detection systems. However, for higher rates, PMD can cause intersymbol interference (ISI) in long- span links. The ISI power penalty in decibels for PMD is approximately 65   where T is a bit period (1/bit rate) and is the power-splitting ratio between principal polarization states. The maximum power penalty occurs when =   . If typical values of the expected value of the differential group delay are 1 ps over a 100-km link and 10 ps over a 1000-km link, find the maximum PMD power penalty for data rates of 10 and 100 Gb/s over these two link distances.<div style=padding-top: 35px>
where T is a bit period (1/bit rate) and is the power-splitting ratio between principal polarization states. The maximum power penalty occurs when = The influence of polarization-mode dispersion can be neglected for data rates up to a few Gb/s for intensity-modulated direct-detection systems. However, for higher rates, PMD can cause intersymbol interference (ISI) in long- span links. The ISI power penalty in decibels for PMD is approximately 65   where T is a bit period (1/bit rate) and is the power-splitting ratio between principal polarization states. The maximum power penalty occurs when =   . If typical values of the expected value of the differential group delay are 1 ps over a 100-km link and 10 ps over a 1000-km link, find the maximum PMD power penalty for data rates of 10 and 100 Gb/s over these two link distances.<div style=padding-top: 35px> . If typical values of the expected value of the differential group delay are 1 ps over a 100-km link and 10 ps over a 1000-km link, find the maximum PMD power penalty for data rates of 10 and 100 Gb/s over these two link distances.
Question
The optical power in a fiber at a distance x from the input end is given by Eq. (14.18). By assuming that the loss coefficient is uniform along the fiber, use this equation to derive Eq. (14.2).
Question
Assuming that Rayleight scattering is approxi­mately isotropic (uniform in all directions), show that the fraction S of scattered light trapped in a multimode fiber in the backward direction is given by Assuming that Rayleight scattering is approxi­mately isotropic (uniform in all directions), show that the fraction S of scattered light trapped in a multimode fiber in the backward direction is given by   where NA is the fiber numerical aperture, n is the core refractive index, and NA/ n represents the half-angle of the cone of captured rays. If NA = 0.20 and n = 1.50, what fraction of the scattered light is recaptured by the fiber in the reverse direction.<div style=padding-top: 35px>
where NA is the fiber numerical aperture, n is the core refractive index, and NA/ n represents the half-angle of the cone of captured rays. If NA = 0.20 and n = 1.50, what fraction of the scattered light is recaptured by the fiber in the reverse direction.
Question
Three 5-km-long fibers have been spliced together in series and an OTDR is used to measure the attenuation of the resultant fiber. The reduced data of the OTDR display is shown in Fig. 14.39. What are the attenuations in decibels per kilometer of the three individual fibers What are the splice losses in decibels What are some possible reasons for the large splice loss occurring between the second and third fibers
Question
Let be the attenuation of the forward propagating light, s the attenuation of the backscattered light, and S the fraction of the total output power scattered in the backward direction, as described in Eq. (14.20). Show that the backscatter response of a rectangular pulse of width W from a point a distance L down the fiber is Let be the attenuation of the forward propagating light, s the attenuation of the backscattered light, and S the fraction of the total output power scattered in the backward direction, as described in Eq. (14.20). Show that the backscatter response of a rectangular pulse of width W from a point a distance L down the fiber is   when L W /2, and   for 0 L W/2   Fig. 14.39 An OTDR trace of three 5-km spilced fibers<div style=padding-top: 35px>
when L W /2, and Let be the attenuation of the forward propagating light, s the attenuation of the backscattered light, and S the fraction of the total output power scattered in the backward direction, as described in Eq. (14.20). Show that the backscatter response of a rectangular pulse of width W from a point a distance L down the fiber is   when L W /2, and   for 0 L W/2   Fig. 14.39 An OTDR trace of three 5-km spilced fibers<div style=padding-top: 35px>
for 0 L W/2 Let be the attenuation of the forward propagating light, s the attenuation of the backscattered light, and S the fraction of the total output power scattered in the backward direction, as described in Eq. (14.20). Show that the backscatter response of a rectangular pulse of width W from a point a distance L down the fiber is   when L W /2, and   for 0 L W/2   Fig. 14.39 An OTDR trace of three 5-km spilced fibers<div style=padding-top: 35px>
Fig. 14.39 An OTDR trace of three 5-km spilced fibers
Question
Using the expression given in Prob. 14.12 for the backscattered power P S (L) from a rectangular pulse of width W, show that for very short pulse widths the backscattered power is proportional to the pulse duration. Note: This is the basis of operation of an OTDR.
Question
The uncertainty U of OTDR loss measure­ments as a function of the signal-to-noise ratio SNR can be approximated by 36
log| U |= 0.2SNR + 0.6
Here, U and SNR are given in decibels. If a 0.5-dB splice is located near the far end of a 50-km fiber, what dynamic range must the OTDR have to measure the insertion loss of this splice event with a ±0.05-dB accuracy. Assume the fiber attenuation is 0.33 dB/km.
Question
Show that, when using an OTDR, an optical pulse width of 5 ns or less is required to locate a fiber fault to within ±0.5 m of its true position.
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Deck 14: Optical Fiber Measurements
1
Optical spectrum analyzers directly measure the wavelength of light in an air environment. However, most wavelength measurements are quoted in terms of wavelengths or optical frequencies in a vacuum. This can lead to errors, particularly in DWDM systems, since the index of refraction of air is a function of wavelength, temperature, pressure, and gas composition. The wavelength dependence of the index of refraction n air of standard dry air at 760 torr and 15°C is 64 Optical spectrum analyzers directly measure the wavelength of light in an air environment. However, most wavelength measurements are quoted in terms of wavelengths or optical frequencies in a vacuum. This can lead to errors, particularly in DWDM systems, since the index of refraction of air is a function of wavelength, temperature, pressure, and gas composition. The wavelength dependence of the index of refraction n air of standard dry air at 760 torr and 15°C is 64   where is measured in micrometers. ( a ) Given that vacuum = air n air , what is the error in wavelength measurement at 1550 nm if the effect of the index of refraction of air is ignored What impact would this have on 0.8-nm-spaced WDM channels in the 1550-nm window ( b ) To compensate for temperature and pressure effects on the value of n air , one can use the relationship   where P is measured in torr and T is in Celsius. How much does n (T, P) vary from n air when the pressure is 640 torr and the temperature is 0°C (which would be at a higher elevation and a lower temperature)
where is measured in micrometers.
( a ) Given that vacuum = air n air , what is the error in wavelength measurement at 1550 nm if the effect of the index of refraction of air is ignored What impact would this have on 0.8-nm-spaced WDM channels in the 1550-nm window
( b ) To compensate for temperature and pressure effects on the value of n air , one can use the relationship Optical spectrum analyzers directly measure the wavelength of light in an air environment. However, most wavelength measurements are quoted in terms of wavelengths or optical frequencies in a vacuum. This can lead to errors, particularly in DWDM systems, since the index of refraction of air is a function of wavelength, temperature, pressure, and gas composition. The wavelength dependence of the index of refraction n air of standard dry air at 760 torr and 15°C is 64   where is measured in micrometers. ( a ) Given that vacuum = air n air , what is the error in wavelength measurement at 1550 nm if the effect of the index of refraction of air is ignored What impact would this have on 0.8-nm-spaced WDM channels in the 1550-nm window ( b ) To compensate for temperature and pressure effects on the value of n air , one can use the relationship   where P is measured in torr and T is in Celsius. How much does n (T, P) vary from n air when the pressure is 640 torr and the temperature is 0°C (which would be at a higher elevation and a lower temperature)
where P is measured in torr and T is in Celsius. How much does n (T, P) vary from n air when the pressure is 640 torr and the temperature is 0°C (which would be at a higher elevation and a lower temperature)
Consider the given equation Consider the given equation   of standard dry air at   and   is,   Since, the wave length of the light in air is   or   . Thus, after substitution of the   value, we get   . (a) To calculate the error in wavelength at 1550 nm as follows:   In DWDM systems, the channel spacing is   , it depends on total value of signal bandwidth. Consider channel spacing is most commercial WDM system is   . So, the error in wavelength at   spaced WDM channels in the 1550 nm window is   . (b) Consider the given equation   variation at   and   is,   Substitute the   value in the given expression as,   Then calculate   as follows:   So, the   variation from   at   and   is   . Thus, the error in wavelength at   spaced WDM channels in the 1550 nm window and variation from   at   and   is calculated. of standard dry air at Consider the given equation   of standard dry air at   and   is,   Since, the wave length of the light in air is   or   . Thus, after substitution of the   value, we get   . (a) To calculate the error in wavelength at 1550 nm as follows:   In DWDM systems, the channel spacing is   , it depends on total value of signal bandwidth. Consider channel spacing is most commercial WDM system is   . So, the error in wavelength at   spaced WDM channels in the 1550 nm window is   . (b) Consider the given equation   variation at   and   is,   Substitute the   value in the given expression as,   Then calculate   as follows:   So, the   variation from   at   and   is   . Thus, the error in wavelength at   spaced WDM channels in the 1550 nm window and variation from   at   and   is calculated. and Consider the given equation   of standard dry air at   and   is,   Since, the wave length of the light in air is   or   . Thus, after substitution of the   value, we get   . (a) To calculate the error in wavelength at 1550 nm as follows:   In DWDM systems, the channel spacing is   , it depends on total value of signal bandwidth. Consider channel spacing is most commercial WDM system is   . So, the error in wavelength at   spaced WDM channels in the 1550 nm window is   . (b) Consider the given equation   variation at   and   is,   Substitute the   value in the given expression as,   Then calculate   as follows:   So, the   variation from   at   and   is   . Thus, the error in wavelength at   spaced WDM channels in the 1550 nm window and variation from   at   and   is calculated. is, Consider the given equation   of standard dry air at   and   is,   Since, the wave length of the light in air is   or   . Thus, after substitution of the   value, we get   . (a) To calculate the error in wavelength at 1550 nm as follows:   In DWDM systems, the channel spacing is   , it depends on total value of signal bandwidth. Consider channel spacing is most commercial WDM system is   . So, the error in wavelength at   spaced WDM channels in the 1550 nm window is   . (b) Consider the given equation   variation at   and   is,   Substitute the   value in the given expression as,   Then calculate   as follows:   So, the   variation from   at   and   is   . Thus, the error in wavelength at   spaced WDM channels in the 1550 nm window and variation from   at   and   is calculated. Since, the wave length of the light in air is Consider the given equation   of standard dry air at   and   is,   Since, the wave length of the light in air is   or   . Thus, after substitution of the   value, we get   . (a) To calculate the error in wavelength at 1550 nm as follows:   In DWDM systems, the channel spacing is   , it depends on total value of signal bandwidth. Consider channel spacing is most commercial WDM system is   . So, the error in wavelength at   spaced WDM channels in the 1550 nm window is   . (b) Consider the given equation   variation at   and   is,   Substitute the   value in the given expression as,   Then calculate   as follows:   So, the   variation from   at   and   is   . Thus, the error in wavelength at   spaced WDM channels in the 1550 nm window and variation from   at   and   is calculated. or Consider the given equation   of standard dry air at   and   is,   Since, the wave length of the light in air is   or   . Thus, after substitution of the   value, we get   . (a) To calculate the error in wavelength at 1550 nm as follows:   In DWDM systems, the channel spacing is   , it depends on total value of signal bandwidth. Consider channel spacing is most commercial WDM system is   . So, the error in wavelength at   spaced WDM channels in the 1550 nm window is   . (b) Consider the given equation   variation at   and   is,   Substitute the   value in the given expression as,   Then calculate   as follows:   So, the   variation from   at   and   is   . Thus, the error in wavelength at   spaced WDM channels in the 1550 nm window and variation from   at   and   is calculated. . Thus, after substitution of the Consider the given equation   of standard dry air at   and   is,   Since, the wave length of the light in air is   or   . Thus, after substitution of the   value, we get   . (a) To calculate the error in wavelength at 1550 nm as follows:   In DWDM systems, the channel spacing is   , it depends on total value of signal bandwidth. Consider channel spacing is most commercial WDM system is   . So, the error in wavelength at   spaced WDM channels in the 1550 nm window is   . (b) Consider the given equation   variation at   and   is,   Substitute the   value in the given expression as,   Then calculate   as follows:   So, the   variation from   at   and   is   . Thus, the error in wavelength at   spaced WDM channels in the 1550 nm window and variation from   at   and   is calculated. value, we get Consider the given equation   of standard dry air at   and   is,   Since, the wave length of the light in air is   or   . Thus, after substitution of the   value, we get   . (a) To calculate the error in wavelength at 1550 nm as follows:   In DWDM systems, the channel spacing is   , it depends on total value of signal bandwidth. Consider channel spacing is most commercial WDM system is   . So, the error in wavelength at   spaced WDM channels in the 1550 nm window is   . (b) Consider the given equation   variation at   and   is,   Substitute the   value in the given expression as,   Then calculate   as follows:   So, the   variation from   at   and   is   . Thus, the error in wavelength at   spaced WDM channels in the 1550 nm window and variation from   at   and   is calculated. .
(a)
To calculate the error in wavelength at 1550 nm as follows: Consider the given equation   of standard dry air at   and   is,   Since, the wave length of the light in air is   or   . Thus, after substitution of the   value, we get   . (a) To calculate the error in wavelength at 1550 nm as follows:   In DWDM systems, the channel spacing is   , it depends on total value of signal bandwidth. Consider channel spacing is most commercial WDM system is   . So, the error in wavelength at   spaced WDM channels in the 1550 nm window is   . (b) Consider the given equation   variation at   and   is,   Substitute the   value in the given expression as,   Then calculate   as follows:   So, the   variation from   at   and   is   . Thus, the error in wavelength at   spaced WDM channels in the 1550 nm window and variation from   at   and   is calculated. In DWDM systems, the channel spacing is Consider the given equation   of standard dry air at   and   is,   Since, the wave length of the light in air is   or   . Thus, after substitution of the   value, we get   . (a) To calculate the error in wavelength at 1550 nm as follows:   In DWDM systems, the channel spacing is   , it depends on total value of signal bandwidth. Consider channel spacing is most commercial WDM system is   . So, the error in wavelength at   spaced WDM channels in the 1550 nm window is   . (b) Consider the given equation   variation at   and   is,   Substitute the   value in the given expression as,   Then calculate   as follows:   So, the   variation from   at   and   is   . Thus, the error in wavelength at   spaced WDM channels in the 1550 nm window and variation from   at   and   is calculated. , it depends on total value of signal bandwidth. Consider channel spacing is most commercial WDM system is Consider the given equation   of standard dry air at   and   is,   Since, the wave length of the light in air is   or   . Thus, after substitution of the   value, we get   . (a) To calculate the error in wavelength at 1550 nm as follows:   In DWDM systems, the channel spacing is   , it depends on total value of signal bandwidth. Consider channel spacing is most commercial WDM system is   . So, the error in wavelength at   spaced WDM channels in the 1550 nm window is   . (b) Consider the given equation   variation at   and   is,   Substitute the   value in the given expression as,   Then calculate   as follows:   So, the   variation from   at   and   is   . Thus, the error in wavelength at   spaced WDM channels in the 1550 nm window and variation from   at   and   is calculated. . So, the error in wavelength at Consider the given equation   of standard dry air at   and   is,   Since, the wave length of the light in air is   or   . Thus, after substitution of the   value, we get   . (a) To calculate the error in wavelength at 1550 nm as follows:   In DWDM systems, the channel spacing is   , it depends on total value of signal bandwidth. Consider channel spacing is most commercial WDM system is   . So, the error in wavelength at   spaced WDM channels in the 1550 nm window is   . (b) Consider the given equation   variation at   and   is,   Substitute the   value in the given expression as,   Then calculate   as follows:   So, the   variation from   at   and   is   . Thus, the error in wavelength at   spaced WDM channels in the 1550 nm window and variation from   at   and   is calculated. spaced WDM channels in the 1550 nm window is Consider the given equation   of standard dry air at   and   is,   Since, the wave length of the light in air is   or   . Thus, after substitution of the   value, we get   . (a) To calculate the error in wavelength at 1550 nm as follows:   In DWDM systems, the channel spacing is   , it depends on total value of signal bandwidth. Consider channel spacing is most commercial WDM system is   . So, the error in wavelength at   spaced WDM channels in the 1550 nm window is   . (b) Consider the given equation   variation at   and   is,   Substitute the   value in the given expression as,   Then calculate   as follows:   So, the   variation from   at   and   is   . Thus, the error in wavelength at   spaced WDM channels in the 1550 nm window and variation from   at   and   is calculated. .
(b)
Consider the given equation Consider the given equation   of standard dry air at   and   is,   Since, the wave length of the light in air is   or   . Thus, after substitution of the   value, we get   . (a) To calculate the error in wavelength at 1550 nm as follows:   In DWDM systems, the channel spacing is   , it depends on total value of signal bandwidth. Consider channel spacing is most commercial WDM system is   . So, the error in wavelength at   spaced WDM channels in the 1550 nm window is   . (b) Consider the given equation   variation at   and   is,   Substitute the   value in the given expression as,   Then calculate   as follows:   So, the   variation from   at   and   is   . Thus, the error in wavelength at   spaced WDM channels in the 1550 nm window and variation from   at   and   is calculated. variation at Consider the given equation   of standard dry air at   and   is,   Since, the wave length of the light in air is   or   . Thus, after substitution of the   value, we get   . (a) To calculate the error in wavelength at 1550 nm as follows:   In DWDM systems, the channel spacing is   , it depends on total value of signal bandwidth. Consider channel spacing is most commercial WDM system is   . So, the error in wavelength at   spaced WDM channels in the 1550 nm window is   . (b) Consider the given equation   variation at   and   is,   Substitute the   value in the given expression as,   Then calculate   as follows:   So, the   variation from   at   and   is   . Thus, the error in wavelength at   spaced WDM channels in the 1550 nm window and variation from   at   and   is calculated. and Consider the given equation   of standard dry air at   and   is,   Since, the wave length of the light in air is   or   . Thus, after substitution of the   value, we get   . (a) To calculate the error in wavelength at 1550 nm as follows:   In DWDM systems, the channel spacing is   , it depends on total value of signal bandwidth. Consider channel spacing is most commercial WDM system is   . So, the error in wavelength at   spaced WDM channels in the 1550 nm window is   . (b) Consider the given equation   variation at   and   is,   Substitute the   value in the given expression as,   Then calculate   as follows:   So, the   variation from   at   and   is   . Thus, the error in wavelength at   spaced WDM channels in the 1550 nm window and variation from   at   and   is calculated. is, Consider the given equation   of standard dry air at   and   is,   Since, the wave length of the light in air is   or   . Thus, after substitution of the   value, we get   . (a) To calculate the error in wavelength at 1550 nm as follows:   In DWDM systems, the channel spacing is   , it depends on total value of signal bandwidth. Consider channel spacing is most commercial WDM system is   . So, the error in wavelength at   spaced WDM channels in the 1550 nm window is   . (b) Consider the given equation   variation at   and   is,   Substitute the   value in the given expression as,   Then calculate   as follows:   So, the   variation from   at   and   is   . Thus, the error in wavelength at   spaced WDM channels in the 1550 nm window and variation from   at   and   is calculated. Substitute the Consider the given equation   of standard dry air at   and   is,   Since, the wave length of the light in air is   or   . Thus, after substitution of the   value, we get   . (a) To calculate the error in wavelength at 1550 nm as follows:   In DWDM systems, the channel spacing is   , it depends on total value of signal bandwidth. Consider channel spacing is most commercial WDM system is   . So, the error in wavelength at   spaced WDM channels in the 1550 nm window is   . (b) Consider the given equation   variation at   and   is,   Substitute the   value in the given expression as,   Then calculate   as follows:   So, the   variation from   at   and   is   . Thus, the error in wavelength at   spaced WDM channels in the 1550 nm window and variation from   at   and   is calculated. value in the given expression as, Consider the given equation   of standard dry air at   and   is,   Since, the wave length of the light in air is   or   . Thus, after substitution of the   value, we get   . (a) To calculate the error in wavelength at 1550 nm as follows:   In DWDM systems, the channel spacing is   , it depends on total value of signal bandwidth. Consider channel spacing is most commercial WDM system is   . So, the error in wavelength at   spaced WDM channels in the 1550 nm window is   . (b) Consider the given equation   variation at   and   is,   Substitute the   value in the given expression as,   Then calculate   as follows:   So, the   variation from   at   and   is   . Thus, the error in wavelength at   spaced WDM channels in the 1550 nm window and variation from   at   and   is calculated. Then calculate Consider the given equation   of standard dry air at   and   is,   Since, the wave length of the light in air is   or   . Thus, after substitution of the   value, we get   . (a) To calculate the error in wavelength at 1550 nm as follows:   In DWDM systems, the channel spacing is   , it depends on total value of signal bandwidth. Consider channel spacing is most commercial WDM system is   . So, the error in wavelength at   spaced WDM channels in the 1550 nm window is   . (b) Consider the given equation   variation at   and   is,   Substitute the   value in the given expression as,   Then calculate   as follows:   So, the   variation from   at   and   is   . Thus, the error in wavelength at   spaced WDM channels in the 1550 nm window and variation from   at   and   is calculated. as follows: Consider the given equation   of standard dry air at   and   is,   Since, the wave length of the light in air is   or   . Thus, after substitution of the   value, we get   . (a) To calculate the error in wavelength at 1550 nm as follows:   In DWDM systems, the channel spacing is   , it depends on total value of signal bandwidth. Consider channel spacing is most commercial WDM system is   . So, the error in wavelength at   spaced WDM channels in the 1550 nm window is   . (b) Consider the given equation   variation at   and   is,   Substitute the   value in the given expression as,   Then calculate   as follows:   So, the   variation from   at   and   is   . Thus, the error in wavelength at   spaced WDM channels in the 1550 nm window and variation from   at   and   is calculated. So, the Consider the given equation   of standard dry air at   and   is,   Since, the wave length of the light in air is   or   . Thus, after substitution of the   value, we get   . (a) To calculate the error in wavelength at 1550 nm as follows:   In DWDM systems, the channel spacing is   , it depends on total value of signal bandwidth. Consider channel spacing is most commercial WDM system is   . So, the error in wavelength at   spaced WDM channels in the 1550 nm window is   . (b) Consider the given equation   variation at   and   is,   Substitute the   value in the given expression as,   Then calculate   as follows:   So, the   variation from   at   and   is   . Thus, the error in wavelength at   spaced WDM channels in the 1550 nm window and variation from   at   and   is calculated. variation from Consider the given equation   of standard dry air at   and   is,   Since, the wave length of the light in air is   or   . Thus, after substitution of the   value, we get   . (a) To calculate the error in wavelength at 1550 nm as follows:   In DWDM systems, the channel spacing is   , it depends on total value of signal bandwidth. Consider channel spacing is most commercial WDM system is   . So, the error in wavelength at   spaced WDM channels in the 1550 nm window is   . (b) Consider the given equation   variation at   and   is,   Substitute the   value in the given expression as,   Then calculate   as follows:   So, the   variation from   at   and   is   . Thus, the error in wavelength at   spaced WDM channels in the 1550 nm window and variation from   at   and   is calculated. at Consider the given equation   of standard dry air at   and   is,   Since, the wave length of the light in air is   or   . Thus, after substitution of the   value, we get   . (a) To calculate the error in wavelength at 1550 nm as follows:   In DWDM systems, the channel spacing is   , it depends on total value of signal bandwidth. Consider channel spacing is most commercial WDM system is   . So, the error in wavelength at   spaced WDM channels in the 1550 nm window is   . (b) Consider the given equation   variation at   and   is,   Substitute the   value in the given expression as,   Then calculate   as follows:   So, the   variation from   at   and   is   . Thus, the error in wavelength at   spaced WDM channels in the 1550 nm window and variation from   at   and   is calculated. and Consider the given equation   of standard dry air at   and   is,   Since, the wave length of the light in air is   or   . Thus, after substitution of the   value, we get   . (a) To calculate the error in wavelength at 1550 nm as follows:   In DWDM systems, the channel spacing is   , it depends on total value of signal bandwidth. Consider channel spacing is most commercial WDM system is   . So, the error in wavelength at   spaced WDM channels in the 1550 nm window is   . (b) Consider the given equation   variation at   and   is,   Substitute the   value in the given expression as,   Then calculate   as follows:   So, the   variation from   at   and   is   . Thus, the error in wavelength at   spaced WDM channels in the 1550 nm window and variation from   at   and   is calculated. is Consider the given equation   of standard dry air at   and   is,   Since, the wave length of the light in air is   or   . Thus, after substitution of the   value, we get   . (a) To calculate the error in wavelength at 1550 nm as follows:   In DWDM systems, the channel spacing is   , it depends on total value of signal bandwidth. Consider channel spacing is most commercial WDM system is   . So, the error in wavelength at   spaced WDM channels in the 1550 nm window is   . (b) Consider the given equation   variation at   and   is,   Substitute the   value in the given expression as,   Then calculate   as follows:   So, the   variation from   at   and   is   . Thus, the error in wavelength at   spaced WDM channels in the 1550 nm window and variation from   at   and   is calculated. .
Thus, the error in wavelength at Consider the given equation   of standard dry air at   and   is,   Since, the wave length of the light in air is   or   . Thus, after substitution of the   value, we get   . (a) To calculate the error in wavelength at 1550 nm as follows:   In DWDM systems, the channel spacing is   , it depends on total value of signal bandwidth. Consider channel spacing is most commercial WDM system is   . So, the error in wavelength at   spaced WDM channels in the 1550 nm window is   . (b) Consider the given equation   variation at   and   is,   Substitute the   value in the given expression as,   Then calculate   as follows:   So, the   variation from   at   and   is   . Thus, the error in wavelength at   spaced WDM channels in the 1550 nm window and variation from   at   and   is calculated. spaced WDM channels in the 1550 nm window and variation from Consider the given equation   of standard dry air at   and   is,   Since, the wave length of the light in air is   or   . Thus, after substitution of the   value, we get   . (a) To calculate the error in wavelength at 1550 nm as follows:   In DWDM systems, the channel spacing is   , it depends on total value of signal bandwidth. Consider channel spacing is most commercial WDM system is   . So, the error in wavelength at   spaced WDM channels in the 1550 nm window is   . (b) Consider the given equation   variation at   and   is,   Substitute the   value in the given expression as,   Then calculate   as follows:   So, the   variation from   at   and   is   . Thus, the error in wavelength at   spaced WDM channels in the 1550 nm window and variation from   at   and   is calculated. at Consider the given equation   of standard dry air at   and   is,   Since, the wave length of the light in air is   or   . Thus, after substitution of the   value, we get   . (a) To calculate the error in wavelength at 1550 nm as follows:   In DWDM systems, the channel spacing is   , it depends on total value of signal bandwidth. Consider channel spacing is most commercial WDM system is   . So, the error in wavelength at   spaced WDM channels in the 1550 nm window is   . (b) Consider the given equation   variation at   and   is,   Substitute the   value in the given expression as,   Then calculate   as follows:   So, the   variation from   at   and   is   . Thus, the error in wavelength at   spaced WDM channels in the 1550 nm window and variation from   at   and   is calculated. and Consider the given equation   of standard dry air at   and   is,   Since, the wave length of the light in air is   or   . Thus, after substitution of the   value, we get   . (a) To calculate the error in wavelength at 1550 nm as follows:   In DWDM systems, the channel spacing is   , it depends on total value of signal bandwidth. Consider channel spacing is most commercial WDM system is   . So, the error in wavelength at   spaced WDM channels in the 1550 nm window is   . (b) Consider the given equation   variation at   and   is,   Substitute the   value in the given expression as,   Then calculate   as follows:   So, the   variation from   at   and   is   . Thus, the error in wavelength at   spaced WDM channels in the 1550 nm window and variation from   at   and   is calculated. is calculated.
2
An engineer wants to find the attenuation at 1310 nm of an 1895-m long fiber. The only available instrument is a photodetector, which gives an output reading in volts. Using this device in a cutback-attenuation setup, the engineer measures an output of 3.31 V from the photodiode at the far end of the fiber. After cutting the fiber 2 m from the source, the output voltage from the photodetector now reads 3.78 V What is the attenuation of the fiber in dB/km
Since the output voltage from the photodetector is proportional to the optical power, we can write Eq. (14.1) as Since the output voltage from the photodetector is proportional to the optical power, we can write Eq. (14.1) as   where L1 is the length of the current fiber, L2 is the length cut off, and V1 and V2 are the voltage output readings from the long and short lengths, respectively. Then the attenuation in decibels is  where L1 is the length of the current fiber, L2 is the length cut off, and V1 and V2 are the voltage output readings from the long and short lengths, respectively. Then the attenuation in decibels is Since the output voltage from the photodetector is proportional to the optical power, we can write Eq. (14.1) as   where L1 is the length of the current fiber, L2 is the length cut off, and V1 and V2 are the voltage output readings from the long and short lengths, respectively. Then the attenuation in decibels is
3
Consider the cutback attenuation measurement technique described by Eq. (14.2) using a photodetector, the power measurements are proportional to the detector output voltage. If the uncertainty in the voltage readings for the two power measurements are ±0.1 percent each, what is the uncertainty in the attenuation accuracy How long must the fiber be to get a sensitivity better than ±0.05 dB/km
Refer to equation 14.2 from the text book to calculate uncertainty in the attenuation accuracy. The average loss Refer to equation 14.2 from the text book to calculate uncertainty in the attenuation accuracy. The average loss   is given by   Here   and   are output powers of the near and far ends of the fiber, respectively and L is the separation of the two measurement points. Rearrange the equation with near and far end length of the fiber   .   Since the output voltage from the photo detector is proportional to the optical power, we can write the equation 14.2 as follows.   Now, calculate the uncertainty in the attenuation accuracy is,   Since,   , refer to equation 14.19 from the text book and then substitute two power measurements are   in the expression as follows:   So, the uncertainty in the attenuation accuracy is   . For determine better sensitivity than   as follows; Consider   , then   So, the fiber is to get a better sensitivity than   is   . Hence, the uncertainty in the attenuation accuracy and better sensitivity of the fiber is calculated. is given by Refer to equation 14.2 from the text book to calculate uncertainty in the attenuation accuracy. The average loss   is given by   Here   and   are output powers of the near and far ends of the fiber, respectively and L is the separation of the two measurement points. Rearrange the equation with near and far end length of the fiber   .   Since the output voltage from the photo detector is proportional to the optical power, we can write the equation 14.2 as follows.   Now, calculate the uncertainty in the attenuation accuracy is,   Since,   , refer to equation 14.19 from the text book and then substitute two power measurements are   in the expression as follows:   So, the uncertainty in the attenuation accuracy is   . For determine better sensitivity than   as follows; Consider   , then   So, the fiber is to get a better sensitivity than   is   . Hence, the uncertainty in the attenuation accuracy and better sensitivity of the fiber is calculated. Here Refer to equation 14.2 from the text book to calculate uncertainty in the attenuation accuracy. The average loss   is given by   Here   and   are output powers of the near and far ends of the fiber, respectively and L is the separation of the two measurement points. Rearrange the equation with near and far end length of the fiber   .   Since the output voltage from the photo detector is proportional to the optical power, we can write the equation 14.2 as follows.   Now, calculate the uncertainty in the attenuation accuracy is,   Since,   , refer to equation 14.19 from the text book and then substitute two power measurements are   in the expression as follows:   So, the uncertainty in the attenuation accuracy is   . For determine better sensitivity than   as follows; Consider   , then   So, the fiber is to get a better sensitivity than   is   . Hence, the uncertainty in the attenuation accuracy and better sensitivity of the fiber is calculated. and Refer to equation 14.2 from the text book to calculate uncertainty in the attenuation accuracy. The average loss   is given by   Here   and   are output powers of the near and far ends of the fiber, respectively and L is the separation of the two measurement points. Rearrange the equation with near and far end length of the fiber   .   Since the output voltage from the photo detector is proportional to the optical power, we can write the equation 14.2 as follows.   Now, calculate the uncertainty in the attenuation accuracy is,   Since,   , refer to equation 14.19 from the text book and then substitute two power measurements are   in the expression as follows:   So, the uncertainty in the attenuation accuracy is   . For determine better sensitivity than   as follows; Consider   , then   So, the fiber is to get a better sensitivity than   is   . Hence, the uncertainty in the attenuation accuracy and better sensitivity of the fiber is calculated. are output powers of the near and far ends of the fiber, respectively and L is the separation of the two measurement points.
Rearrange the equation with near and far end length of the fiber Refer to equation 14.2 from the text book to calculate uncertainty in the attenuation accuracy. The average loss   is given by   Here   and   are output powers of the near and far ends of the fiber, respectively and L is the separation of the two measurement points. Rearrange the equation with near and far end length of the fiber   .   Since the output voltage from the photo detector is proportional to the optical power, we can write the equation 14.2 as follows.   Now, calculate the uncertainty in the attenuation accuracy is,   Since,   , refer to equation 14.19 from the text book and then substitute two power measurements are   in the expression as follows:   So, the uncertainty in the attenuation accuracy is   . For determine better sensitivity than   as follows; Consider   , then   So, the fiber is to get a better sensitivity than   is   . Hence, the uncertainty in the attenuation accuracy and better sensitivity of the fiber is calculated. . Refer to equation 14.2 from the text book to calculate uncertainty in the attenuation accuracy. The average loss   is given by   Here   and   are output powers of the near and far ends of the fiber, respectively and L is the separation of the two measurement points. Rearrange the equation with near and far end length of the fiber   .   Since the output voltage from the photo detector is proportional to the optical power, we can write the equation 14.2 as follows.   Now, calculate the uncertainty in the attenuation accuracy is,   Since,   , refer to equation 14.19 from the text book and then substitute two power measurements are   in the expression as follows:   So, the uncertainty in the attenuation accuracy is   . For determine better sensitivity than   as follows; Consider   , then   So, the fiber is to get a better sensitivity than   is   . Hence, the uncertainty in the attenuation accuracy and better sensitivity of the fiber is calculated. Since the output voltage from the photo detector is proportional to the optical power, we can write the equation 14.2 as follows. Refer to equation 14.2 from the text book to calculate uncertainty in the attenuation accuracy. The average loss   is given by   Here   and   are output powers of the near and far ends of the fiber, respectively and L is the separation of the two measurement points. Rearrange the equation with near and far end length of the fiber   .   Since the output voltage from the photo detector is proportional to the optical power, we can write the equation 14.2 as follows.   Now, calculate the uncertainty in the attenuation accuracy is,   Since,   , refer to equation 14.19 from the text book and then substitute two power measurements are   in the expression as follows:   So, the uncertainty in the attenuation accuracy is   . For determine better sensitivity than   as follows; Consider   , then   So, the fiber is to get a better sensitivity than   is   . Hence, the uncertainty in the attenuation accuracy and better sensitivity of the fiber is calculated. Now, calculate the uncertainty in the attenuation accuracy is, Refer to equation 14.2 from the text book to calculate uncertainty in the attenuation accuracy. The average loss   is given by   Here   and   are output powers of the near and far ends of the fiber, respectively and L is the separation of the two measurement points. Rearrange the equation with near and far end length of the fiber   .   Since the output voltage from the photo detector is proportional to the optical power, we can write the equation 14.2 as follows.   Now, calculate the uncertainty in the attenuation accuracy is,   Since,   , refer to equation 14.19 from the text book and then substitute two power measurements are   in the expression as follows:   So, the uncertainty in the attenuation accuracy is   . For determine better sensitivity than   as follows; Consider   , then   So, the fiber is to get a better sensitivity than   is   . Hence, the uncertainty in the attenuation accuracy and better sensitivity of the fiber is calculated. Since, Refer to equation 14.2 from the text book to calculate uncertainty in the attenuation accuracy. The average loss   is given by   Here   and   are output powers of the near and far ends of the fiber, respectively and L is the separation of the two measurement points. Rearrange the equation with near and far end length of the fiber   .   Since the output voltage from the photo detector is proportional to the optical power, we can write the equation 14.2 as follows.   Now, calculate the uncertainty in the attenuation accuracy is,   Since,   , refer to equation 14.19 from the text book and then substitute two power measurements are   in the expression as follows:   So, the uncertainty in the attenuation accuracy is   . For determine better sensitivity than   as follows; Consider   , then   So, the fiber is to get a better sensitivity than   is   . Hence, the uncertainty in the attenuation accuracy and better sensitivity of the fiber is calculated. , refer to equation 14.19 from the text book and then substitute two power measurements are Refer to equation 14.2 from the text book to calculate uncertainty in the attenuation accuracy. The average loss   is given by   Here   and   are output powers of the near and far ends of the fiber, respectively and L is the separation of the two measurement points. Rearrange the equation with near and far end length of the fiber   .   Since the output voltage from the photo detector is proportional to the optical power, we can write the equation 14.2 as follows.   Now, calculate the uncertainty in the attenuation accuracy is,   Since,   , refer to equation 14.19 from the text book and then substitute two power measurements are   in the expression as follows:   So, the uncertainty in the attenuation accuracy is   . For determine better sensitivity than   as follows; Consider   , then   So, the fiber is to get a better sensitivity than   is   . Hence, the uncertainty in the attenuation accuracy and better sensitivity of the fiber is calculated. in the expression as follows: Refer to equation 14.2 from the text book to calculate uncertainty in the attenuation accuracy. The average loss   is given by   Here   and   are output powers of the near and far ends of the fiber, respectively and L is the separation of the two measurement points. Rearrange the equation with near and far end length of the fiber   .   Since the output voltage from the photo detector is proportional to the optical power, we can write the equation 14.2 as follows.   Now, calculate the uncertainty in the attenuation accuracy is,   Since,   , refer to equation 14.19 from the text book and then substitute two power measurements are   in the expression as follows:   So, the uncertainty in the attenuation accuracy is   . For determine better sensitivity than   as follows; Consider   , then   So, the fiber is to get a better sensitivity than   is   . Hence, the uncertainty in the attenuation accuracy and better sensitivity of the fiber is calculated. So, the uncertainty in the attenuation accuracy is Refer to equation 14.2 from the text book to calculate uncertainty in the attenuation accuracy. The average loss   is given by   Here   and   are output powers of the near and far ends of the fiber, respectively and L is the separation of the two measurement points. Rearrange the equation with near and far end length of the fiber   .   Since the output voltage from the photo detector is proportional to the optical power, we can write the equation 14.2 as follows.   Now, calculate the uncertainty in the attenuation accuracy is,   Since,   , refer to equation 14.19 from the text book and then substitute two power measurements are   in the expression as follows:   So, the uncertainty in the attenuation accuracy is   . For determine better sensitivity than   as follows; Consider   , then   So, the fiber is to get a better sensitivity than   is   . Hence, the uncertainty in the attenuation accuracy and better sensitivity of the fiber is calculated. .
For determine better sensitivity than Refer to equation 14.2 from the text book to calculate uncertainty in the attenuation accuracy. The average loss   is given by   Here   and   are output powers of the near and far ends of the fiber, respectively and L is the separation of the two measurement points. Rearrange the equation with near and far end length of the fiber   .   Since the output voltage from the photo detector is proportional to the optical power, we can write the equation 14.2 as follows.   Now, calculate the uncertainty in the attenuation accuracy is,   Since,   , refer to equation 14.19 from the text book and then substitute two power measurements are   in the expression as follows:   So, the uncertainty in the attenuation accuracy is   . For determine better sensitivity than   as follows; Consider   , then   So, the fiber is to get a better sensitivity than   is   . Hence, the uncertainty in the attenuation accuracy and better sensitivity of the fiber is calculated. as follows;
Consider Refer to equation 14.2 from the text book to calculate uncertainty in the attenuation accuracy. The average loss   is given by   Here   and   are output powers of the near and far ends of the fiber, respectively and L is the separation of the two measurement points. Rearrange the equation with near and far end length of the fiber   .   Since the output voltage from the photo detector is proportional to the optical power, we can write the equation 14.2 as follows.   Now, calculate the uncertainty in the attenuation accuracy is,   Since,   , refer to equation 14.19 from the text book and then substitute two power measurements are   in the expression as follows:   So, the uncertainty in the attenuation accuracy is   . For determine better sensitivity than   as follows; Consider   , then   So, the fiber is to get a better sensitivity than   is   . Hence, the uncertainty in the attenuation accuracy and better sensitivity of the fiber is calculated. , then Refer to equation 14.2 from the text book to calculate uncertainty in the attenuation accuracy. The average loss   is given by   Here   and   are output powers of the near and far ends of the fiber, respectively and L is the separation of the two measurement points. Rearrange the equation with near and far end length of the fiber   .   Since the output voltage from the photo detector is proportional to the optical power, we can write the equation 14.2 as follows.   Now, calculate the uncertainty in the attenuation accuracy is,   Since,   , refer to equation 14.19 from the text book and then substitute two power measurements are   in the expression as follows:   So, the uncertainty in the attenuation accuracy is   . For determine better sensitivity than   as follows; Consider   , then   So, the fiber is to get a better sensitivity than   is   . Hence, the uncertainty in the attenuation accuracy and better sensitivity of the fiber is calculated. So, the fiber is to get a better sensitivity than Refer to equation 14.2 from the text book to calculate uncertainty in the attenuation accuracy. The average loss   is given by   Here   and   are output powers of the near and far ends of the fiber, respectively and L is the separation of the two measurement points. Rearrange the equation with near and far end length of the fiber   .   Since the output voltage from the photo detector is proportional to the optical power, we can write the equation 14.2 as follows.   Now, calculate the uncertainty in the attenuation accuracy is,   Since,   , refer to equation 14.19 from the text book and then substitute two power measurements are   in the expression as follows:   So, the uncertainty in the attenuation accuracy is   . For determine better sensitivity than   as follows; Consider   , then   So, the fiber is to get a better sensitivity than   is   . Hence, the uncertainty in the attenuation accuracy and better sensitivity of the fiber is calculated. is Refer to equation 14.2 from the text book to calculate uncertainty in the attenuation accuracy. The average loss   is given by   Here   and   are output powers of the near and far ends of the fiber, respectively and L is the separation of the two measurement points. Rearrange the equation with near and far end length of the fiber   .   Since the output voltage from the photo detector is proportional to the optical power, we can write the equation 14.2 as follows.   Now, calculate the uncertainty in the attenuation accuracy is,   Since,   , refer to equation 14.19 from the text book and then substitute two power measurements are   in the expression as follows:   So, the uncertainty in the attenuation accuracy is   . For determine better sensitivity than   as follows; Consider   , then   So, the fiber is to get a better sensitivity than   is   . Hence, the uncertainty in the attenuation accuracy and better sensitivity of the fiber is calculated. .
Hence, the uncertainty in the attenuation accuracy and better sensitivity of the fiber is calculated.
4
Verify that the full-width at half-maximum of a gaussian pulse is given by t FWHM = 2(2 ln 2) 1/2.
( b ) Derive Eq. (14.11), which describes the 3-dB bandwidth of a fiber based on a gaussian output response.
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A gaussian approximation of | H ( f )| in the form A gaussian approximation of | H ( f )| in the form   has been found to be accurate to at least the 0.75-amplitude point in the frequency domain. Using this relationship, plot P( f)/P(t) as a function of frequency from 0 to 1000 MHz for fibers that have impulse responses of full rms pulse widths 2 equal to 2.0, 1.0, and 0.5 ns. What are the 3-dB bandwidths of these fibers
has been found to be accurate to at least the 0.75-amplitude point in the frequency domain. Using this relationship, plot P( f)/P(t) as a function of frequency from 0 to 1000 MHz for fibers that have impulse responses of full rms pulse widths 2 equal to 2.0, 1.0, and 0.5 ns. What are the 3-dB bandwidths of these fibers
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Consider the data shown in Fig. 14.37 of the group delay versus wavelength for a 10-km long fiber. From this data, plot the chromatic dispersion D as a function of wavelength. What is the value of the zero-dispersion slope S 0 in the relationship D() = S 0 ( 0 ) Consider the data shown in Fig. 14.37 of the group delay versus wavelength for a 10-km long fiber. From this data, plot the chromatic dispersion D as a function of wavelength. What is the value of the zero-dispersion slope S 0 in the relationship D() = S 0 ( 0 )   Fig. 14.37 Chromatic-dispersion measurement of a 10-km fiber
Fig. 14.37 Chromatic-dispersion measurement of a 10-km fiber
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7
Determine the value of the expected differential group delay from the polarization-mode- dispersion measurement response shown in Fig. 14.38 for a non-mode-coupled fiber. Determine the value of the expected differential group delay from the polarization-mode- dispersion measurement response shown in Fig. 14.38 for a non-mode-coupled fiber.   Fig. 14.38 PMD-inducedpowerexcursions about the mean power level (dashed line)
Fig. 14.38 PMD-inducedpowerexcursions about the mean power level (dashed line)
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The influence of polarization-mode dispersion can be neglected for data rates up to a few Gb/s for intensity-modulated direct-detection systems. However, for higher rates, PMD can cause intersymbol interference (ISI) in long- span links. The ISI power penalty in decibels for PMD is approximately 65 The influence of polarization-mode dispersion can be neglected for data rates up to a few Gb/s for intensity-modulated direct-detection systems. However, for higher rates, PMD can cause intersymbol interference (ISI) in long- span links. The ISI power penalty in decibels for PMD is approximately 65   where T is a bit period (1/bit rate) and is the power-splitting ratio between principal polarization states. The maximum power penalty occurs when =   . If typical values of the expected value of the differential group delay are 1 ps over a 100-km link and 10 ps over a 1000-km link, find the maximum PMD power penalty for data rates of 10 and 100 Gb/s over these two link distances.
where T is a bit period (1/bit rate) and is the power-splitting ratio between principal polarization states. The maximum power penalty occurs when = The influence of polarization-mode dispersion can be neglected for data rates up to a few Gb/s for intensity-modulated direct-detection systems. However, for higher rates, PMD can cause intersymbol interference (ISI) in long- span links. The ISI power penalty in decibels for PMD is approximately 65   where T is a bit period (1/bit rate) and is the power-splitting ratio between principal polarization states. The maximum power penalty occurs when =   . If typical values of the expected value of the differential group delay are 1 ps over a 100-km link and 10 ps over a 1000-km link, find the maximum PMD power penalty for data rates of 10 and 100 Gb/s over these two link distances. . If typical values of the expected value of the differential group delay are 1 ps over a 100-km link and 10 ps over a 1000-km link, find the maximum PMD power penalty for data rates of 10 and 100 Gb/s over these two link distances.
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The optical power in a fiber at a distance x from the input end is given by Eq. (14.18). By assuming that the loss coefficient is uniform along the fiber, use this equation to derive Eq. (14.2).
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10
Assuming that Rayleight scattering is approxi­mately isotropic (uniform in all directions), show that the fraction S of scattered light trapped in a multimode fiber in the backward direction is given by Assuming that Rayleight scattering is approxi­mately isotropic (uniform in all directions), show that the fraction S of scattered light trapped in a multimode fiber in the backward direction is given by   where NA is the fiber numerical aperture, n is the core refractive index, and NA/ n represents the half-angle of the cone of captured rays. If NA = 0.20 and n = 1.50, what fraction of the scattered light is recaptured by the fiber in the reverse direction.
where NA is the fiber numerical aperture, n is the core refractive index, and NA/ n represents the half-angle of the cone of captured rays. If NA = 0.20 and n = 1.50, what fraction of the scattered light is recaptured by the fiber in the reverse direction.
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11
Three 5-km-long fibers have been spliced together in series and an OTDR is used to measure the attenuation of the resultant fiber. The reduced data of the OTDR display is shown in Fig. 14.39. What are the attenuations in decibels per kilometer of the three individual fibers What are the splice losses in decibels What are some possible reasons for the large splice loss occurring between the second and third fibers
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12
Let be the attenuation of the forward propagating light, s the attenuation of the backscattered light, and S the fraction of the total output power scattered in the backward direction, as described in Eq. (14.20). Show that the backscatter response of a rectangular pulse of width W from a point a distance L down the fiber is Let be the attenuation of the forward propagating light, s the attenuation of the backscattered light, and S the fraction of the total output power scattered in the backward direction, as described in Eq. (14.20). Show that the backscatter response of a rectangular pulse of width W from a point a distance L down the fiber is   when L W /2, and   for 0 L W/2   Fig. 14.39 An OTDR trace of three 5-km spilced fibers
when L W /2, and Let be the attenuation of the forward propagating light, s the attenuation of the backscattered light, and S the fraction of the total output power scattered in the backward direction, as described in Eq. (14.20). Show that the backscatter response of a rectangular pulse of width W from a point a distance L down the fiber is   when L W /2, and   for 0 L W/2   Fig. 14.39 An OTDR trace of three 5-km spilced fibers
for 0 L W/2 Let be the attenuation of the forward propagating light, s the attenuation of the backscattered light, and S the fraction of the total output power scattered in the backward direction, as described in Eq. (14.20). Show that the backscatter response of a rectangular pulse of width W from a point a distance L down the fiber is   when L W /2, and   for 0 L W/2   Fig. 14.39 An OTDR trace of three 5-km spilced fibers
Fig. 14.39 An OTDR trace of three 5-km spilced fibers
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13
Using the expression given in Prob. 14.12 for the backscattered power P S (L) from a rectangular pulse of width W, show that for very short pulse widths the backscattered power is proportional to the pulse duration. Note: This is the basis of operation of an OTDR.
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14
The uncertainty U of OTDR loss measure­ments as a function of the signal-to-noise ratio SNR can be approximated by 36
log| U |= 0.2SNR + 0.6
Here, U and SNR are given in decibels. If a 0.5-dB splice is located near the far end of a 50-km fiber, what dynamic range must the OTDR have to measure the insertion loss of this splice event with a ±0.05-dB accuracy. Assume the fiber attenuation is 0.33 dB/km.
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15
Show that, when using an OTDR, an optical pulse width of 5 ns or less is required to locate a fiber fault to within ±0.5 m of its true position.
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