WO2011098982A1 - Method and system for free-space optical communication with reduced scintillations - Google Patents
Method and system for free-space optical communication with reduced scintillations Download PDFInfo
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- WO2011098982A1 WO2011098982A1 PCT/IB2011/050593 IB2011050593W WO2011098982A1 WO 2011098982 A1 WO2011098982 A1 WO 2011098982A1 IB 2011050593 W IB2011050593 W IB 2011050593W WO 2011098982 A1 WO2011098982 A1 WO 2011098982A1
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- H—ELECTRICITY
- H04—ELECTRIC COMMUNICATION TECHNIQUE
- H04B—TRANSMISSION
- H04B10/00—Transmission systems employing electromagnetic waves other than radio-waves, e.g. infrared, visible or ultraviolet light, or employing corpuscular radiation, e.g. quantum communication
- H04B10/11—Arrangements specific to free-space transmission, i.e. transmission through air or vacuum
- H04B10/112—Line-of-sight transmission over an extended range
- H04B10/1121—One-way transmission
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- the present invention pertains to free-space optical communication through turbulent medium, such as atmosphere, and in particular to methods and approaches for reducing scintillations and minimizing signal fades.
- the optical beam arrives at the receiver's input aperture highly spatially deteriorated. This is because the random fluctuations in the refractive index of air ever so slightly bend and scatter the optical beam or its portions, the effect being accumulated over the distance of propagation.
- the received optical beam typically becomes fragmented, consisting of a pattern of bright and dark spots, called speckles. Moreover, these spots are constantly moving and fluctuating on the time scale of the atmospheric turbulence of about one millisecond.
- the signal received by the detector coupled to the optical receiver at the receiving end of the FSO communication link may strongly fluctuate in time, which decreases the performance of the link.
- Such fluctuations are called scintillations and are characterized by a scintillation index. Stronger fluctuations are characterized by a larger value of the scintillation index, e.g. 1 or more.
- Deep signal dropouts, called fades occur more frequently and last longer when the scintillation index is large. For example these fades may occur many times per second and last for a millisecond or longer. Under such conditions a typical FSO communication link shows large error rates, low reliability or complete loss of signal.
- the methods and the systems designed to reduce the scintillations and minimize signal fades as much as possible are of great importance for FSO communication. Good methods and systems must also be simple, reliable and inexpensive.
- Direct averaging of the scintillating signal over time cannot be used for high data rate FSO communication because of the slow rate of atmospheric fluctuations. For example, taking into account the fact that the characteristic time scale of the atmospheric turbulence is about one millisecond the effective averaging time of ten milliseconds or more is required. Ten-millisecond or longer averaging for each bit of the data stream will require the data rate of one hundred bits per second or less. Clearly, the required method and system should not only reduce scintillations, but do so in the manner applicable to the high bit-rate communication.
- MIMO multiple-input, multiple-output
- RF radiofrequency
- scintillation reduction can be achieved by using rough-surface phase masks or optical diffusers placed in the pathway of a temporally coherent light beam carrying the communication signal before it is send through atmosphere.
- phase masks or diffusers allegedly scramble the laser beam's spatial phase distribution to create a 'partially-coherent' optical beam.
- this approach indeed provides a complicated transverse phase and intensity profile of the beam that appears random, this profile remains stationary in time.
- the temporal coherence of the optical radiation remains unchanged after passing through the phase mask or diffuser, and is equal to the temporal coherence of the laser.
- the optical beam at the output of the phase mask or diffuser in this case can be considered as a set of multiple randomly distributed mutually coherent sources with stationary amplitudes and phases and can be called 'partially coherent' only to some extent.
- true partial coherence is understood to imply ensemble average. This means taking multiple independent realizations of the optical beam's transverse phase and amplitude and averaging over these realizations to obtain the final result.
- advantages of a true partially coherent beam can be realized only by applying the ergodicity conjecture, i.e. is the equivalence of ensemble average and the average over time.
- a true partially coherent beam in both space and time with short temporal coherence.
- the crossection of such true partially coherent beam comprises multiple randomly distributed and mutually incoherent sources.
- the characteristic coherence time of such true partially coherent beam also needs to be much shorter than the duration of the averaging.
- the true partially coherent beam would need to cycle through many independent realizations of its phase and amplitude during the time of one bit.
- the characteristic temporal coherence time of the true partially coherent beam should be much shorter than the duration of the bit in order to take advantage of the averaging discussed above.
- Transmitted optical signal should reach the detector via a number of substantially independent (uncorrelated) paths through atmosphere so that the probability of fade on all of those paths is minimized
- STPCB spatio-temporally partially coherent optical beam
- speckle structure of the light i.e. the position of bright and dark spots on the receiver's aperture, after propagation through turbulent atmosphere depends on both the state of the atmosphere and the spatio-temporal properties of the optical beam eradiated by the transmitter.
- these spatio-temporal properties include the transverse distribution of phase and amplitude of the light, as well as their variation in time. For one particular moment of time t 0 the transmitted optical beam with certain transverse phase and intensity distribution results in a certain speckle structure on the receiver aperture.
- t 1 t 0 +Delta_t, separated from the first by a delay Delta_t, another transverse phase and intensity distribution of the transmitted beam results in a substantially different speckle structure on the receiver aperture, Fig. 1A.
- the time delay Delta_t is chosen to be much shorter than the duration of each bit in the communication data stream.
- the speckle structures discussed above are different even for 'frozen' atmosphere, which it is on the time scales of the data bit duration.
- the speckle structure changes with the rate of change of the transmitted beam phase and intensity distribution and not with the rate of the atmosphere.
- STPCB spatio-temporally partially coherent optical beam
- the latter fluctuations can be averaged with a detector having finite radiofrequency (RF) bandwidth during each bit of the data stream.
- the STPCB's rate is substantially faster than the communication data rate, or equivalently the STPCB's coherence time is substantially shorter than the duration of the bit, effective averaging is possible with the benefit of suppressing signal scintillations and deep signal fades typical for standard FSO systems.
- the update rate of STPCB needs to be 10 GHz or higher to bring forth the advantages of averaging described above.
- the present invention teaches a very simple way of generating and using STPCBs with virtually unlimited update rates (short coherence times) suitable for high bit-rate FSO communication systems.
- the STPCB may be modulated with communication data in a number of standard ways known in the art, e.g. with amplitude modulation.
- the STPCB may be generated by coupling a broadband optical radiation into an optical system including a number of different optical paths (modes) with different delays, such as, for example, a volume diffraction element, another example being a multimode optical fiber or waveguide (MMF).
- a volume diffraction element such as, for example, a volume diffraction element, another example being a multimode optical fiber or waveguide (MMF).
- MMF multimode optical fiber or waveguide
- Gradient-index MMFs typically have small amount of intermodal dispersion and thus are not preferred to be used for, although not excluded from the use in the STPCB generation.
- step-index MMFs typically have large amount of intermodal dispersion and are thus preferred for the STPCB generation. Step-index MMFs will be assumed in the following arguments.
- a multi-frequency laser such as Fabri-Perot laser
- Fabri-Perot laser the schematic spectrum of which is shown in Fig. 2C.
- Such laser emits a number of distinct optical frequencies f 1 , f 2 ,...f n oscillating with random uncorrelated phases.
- each frequency excites essentially the same set of transverse spatial modes of the MMF. These modes propagate at different velocities towards the output end of the MMF.
- the interference of these modes at each individual optical frequency creates a distinct transverse phase and intensity pattern at the output of the MMF.
- Two examples of such intensity patterns are shown in Fig. 3B and Fig. 3C corresponding to a small and a large number of modes excited in the MMF respectively.
- each spatial pattern corresponding to each individual frequency of the laser may be considered to be an independent optical emitter with complicated transverse phase and amplitude distributions.
- the resulting overall distribution of phase and amplitude will fluctuate rapidly and essentially randomly thus forming an STPCB.
- the subset of optical frequencies After propagation through the communication medium, such as turbulent atmosphere, the subset of optical frequencies will reach the detector. The beat note between adjacent laser frequencies will not be effectively detected by the detector due to the limited RF bandwidth of the latter. Only the data modulation signal being within the RF bandwidth of the detector will be effectively received.
- a continuous-spectrum broadband optical source such as the one shown in Fig. 2A can be viewed as a limiting case of the example considered above with the separation between neighboring frequencies reduced to zero and a corresponding increase in the number of individual frequencies - to infinity.
- One difference from the previous case is that the beat note between the two adjacent frequencies now falls within the RF bandwidth of the detector.
- the beat notes between multiple pairs of adjacent frequencies oscillate with random phases and effectively produce a negligible noise and continuous DC background, which is usually filtered out by the detector or otherwise do not substantially affect the ability of the detector to receive the desired communication signal.
- FIG. 3D An example of transverse spatial intensity profile of an STPCB as measured by a slow detector, for example a CCD camera, is shown in Fig. 3D.
- the STPCB intensity profile has very low contrast. This is because the slow CCD camera cannot temporally resolve all the rapid fluctuations of the light and thus produces an averaged picture.
- the measurement of contrast just described may, in fact, serve as an indication of the quality of the STPCB: Lower observed contrast indicates a better quality STPCB for the purpose of scintillation reduction in an FSO communication link.
- Fig. 3A shows the intensity profile at the output of a single-mode optical fiber. This profile is a familiar bell-shaped 2-dimentional distribution, which essentially does not depend on the spectral width of the optical source and the length of the fiber.
- L is the physical length of the MMF
- n is its average refractive index
- NA is its numerical aperture
- c is the speed of light
- Delta_f is the frequency difference between the two adjacent optical frequencies of the optical source.
- Delta_F is the full spectral width of the optical source and M is the desired number of effective independent sources in the context of the above discussion. Larger values of M, say 100, generally results in a better-quality STPCB.
- the length L of the MMF cannot be too large, however. This is because the dispersion in the MMF aside from helping to generate STPCB also temporally stretches the data bits comprising the communication signal stream.
- the condition expressing the requirement that this temporal stretch is small reads:
- T is the duration of the bit.
- the quality of STPCB and with it the effectiveness of temporal averaging discussed above dependson the number of paths ormodes excited in theSTPCB creating system such as MMF.It is therefore desired tohave a substantially uniform excitation of the modesof the MMF, i.e.excite as large number of modes as possible with preferably equal intensities.
- an offset splice or connection between the input fiber and the MMF may be applied.
- the objective of the present invention to teach the method and to describe the apparatus for FSO communication with reduced scintillations using simple and effective methods for generating, modulating transmitting and receiving spatio-temporally partially coherent optical beams (STPCBs).
- STPCBs spatio-temporally partially coherent optical beams
- the method and the apparatus of the present invention may be applied with benefit to one-way and two-way communication for point-to-point and point-to multipoint FSO applications between stationary and moving platforms.
- a further advantage is the ease with which the existing FSO communication systems can be upgraded to incorporate the method and the system of the present invention thus yielding immediate performance improvements described. Still further objectives and advantages will become apparent from the consideration of ensuing description and drawings.
- a method for free-space optical communication with reduced scintillations includes:
- an apparatus for free-space optical communication with reduced scintillations includes:
- an optical collimation system adapted for collimating said spatio-temporally partially coherent optical beam to produce substantially collimated spatio-temporally partially coherent optical beam of large aperture and adapted for eradiating said substantially collimated spatio-temporally partially coherent optical beam of large aperture into a communication medium, such as atmosphere;
- an optical receiver adapted for receiving at least a portion of said substantially collimated spatio-temporally partially coherent optical beam of large aperture after propagation of said substantially collimated spatio-temporally partially coherent optical beam of large aperture through said communication medium;
- the source of broadband optical radiation is a low-coherence light source.
- the source of broadband optical radiation is an ultrashort-pulse laser.
- the source of broadband optical radiation is a multiple-frequency optical source.
- the source of broadband optical radiation is a plurality of single-frequency optical sources with distinct central optical frequencies.
- system for modulating said broadband optical radiation with said communication signal is adapted for direct modulation of the output of said source of broadband optical radiation.
- the system for modulating said broadband optical radiation with said communication signal comprises an external optical modulator.
- the apparatus further comprises an optical amplifier.
- the apparatus further comprises a system for a substantially uniform excitation of transverse modes of said multimode optical fiber or waveguide.
- the system for achieving substantial collimation of said spatio-temporally partially coherent optical beam to obtain substantially collimated spatio-temporally partially coherent optical beam of large aperture and eradiating said substantially collimated spatio-temporally partially coherent optical beam of large aperture into said communication medium comprises at least one optical element with positive optical power.
- the system for achieving substantial collimation of said spatio-temporally partially coherent optical beam to obtain substantially collimated spatio-temporally partially coherent optical beam of large aperture and eradiating said substantially collimated spatio-temporally partially coherent optical beam of large aperture into said communication medium is adapted for performing optical magnification of an optical core of said multimode optical fiber or waveguide to the transverse dimension of said large aperture.
- the said optical receiver further comprises a system for intercepting at least a portion of said substantially collimated spatio-temporally partially coherent optical beam of large aperture after propagation through said communication medium and concentrating the received potion of said substantially collimated spatio-temporally partially coherent optical beam of large aperture on an optical detector, the system for intercepting comprising at least one optical element with positive optical power.
- the optical detector is a fiber-coupled optical detector.
- Fig. 1A illustrates an example of the sequence of momentary beam intensity distributions of spatio-temporally partially coherent optical beam.
- Fig. 1B illustrates an example of spatio-temporally partially coherent beam's intensity distribution averaged during a one bit-long time interval.
- Fig. 2A illustrates an example of the spectrum of a continuous-spectrum broadband light source.
- Fig. 2B illustrates an example of the spectrum of a source consisting of a number of narrowband spectra
- Fig. 2C illustrates an example of the spectrum of a source consisting of a number of sharp lines.
- Fig. 3A illustrates spatially coherent light intensity distribution at the output of a single-mode optical fiber which is essentially independent on the spectral properties of the optical source and the length of the fiber.
- Fig. 3B illustrates spatially coherent multimode light intensity distribution formed by a small number of transverse modes of a multimode optical fiber excited with a narrowband optical source.
- Fig. 3C illustrates spatially coherent multimode light intensity distribution formed by a large number of transverse modes of a multimode optical fiber excited with a narrowband optical source.
- Fig. 3D illustrates a low-contrast intensity distribution of a spatio-temporally partially coherent optical beam formed at the output of a multimode optical fiber excited with a broadband optical source
- Fig. 4A is a schematic diagram of one embodiment of the system.
- Fig. 4B is a schematic diagram of one embodiment of the system utilizing an optical amplifier.
- Fig. 4C is a schematic diagram of one embodiment of the system utilizing an optical amplifier and a mode scrambler.
- the system for FSO communication with reduced scintillations comprises a transmitter and a receiver separated by the communication medium, such as atmosphere, preferably at the line of sight.
- the source of optical radiation allocated in the transmitter emits a substantially broad optical spectrum preferably in a single transverse mode.
- the optical spectrum of the source may be continuous, quasi-continuous or discrete within a finite bandwidth with the requirement being that the inverse width of the spectrum is substantially smaller than the duration of one bit of the digital communication signal.
- the broadband optical source may be a low-coherence superluminescent diode, an ultrashort-pulse laser, an optical supercontinuum source, a Fabri-Perot type multi-frequency laser, a number of single-frequency lasers with separate central frequencies, or a combination of such sources.
- Relatively inexpensive semiconductor optical sources of the above type are currently available and may be used in the system described herein.
- Fig. 2A is schematically shown a spectrum of a continuous-spectrum optical source with the overall spectral width Delta_F. Equation (5) above may be applied to estimate the required spectral width Delta_F for the most optimal STPCB generation.
- the minimum spectral width Delta_F should be about 1 THz, which for a telecommunication-region source near 1.55 micrometer central wavelength corresponds to less than 10 nanometers on the wavelength scale.
- superluminescent diodes with such or larger bandwidths are inexpensively available off the shelf.
- Fig. 2B shows a spectrum of quasi-continuous broadband optical source with several separated relatively broad lines. Similar analysis as outlined above can be applied to such source.
- Fig. 2C schematically shows the spectrum of a multi-frequency laser, such as Fabri-Perot laser.
- the analysis for such laser is preferably performed using Eq. (4) above and was demonstrated above.
- the communication data stream may be modulated onto the optical radiation produced by the broadband optical source discussed above by either a direct modulation of the optical source itself via its drive current modulation or by using an external optical modulator.
- an external optical modulator may be a Lithium Niobate intensity modulator, an electroabsorption modulator or a similar device that offers the modulation speeds and modulation formats desired for the FSO communication link.
- the current invention does not specify and is not limited to any particular modulation format.
- direct detection formats such as OOK
- PPM will be preferred over the coherent detection formats, such as DPSK, BPSK.
- the broadband optical radiation may be optionally amplified in an optical amplifier to increase the transmitted power.
- an optical amplifier may be achieved using an Erbium-doped fiber amplifier (EDFA) or a semiconductor optical amplifier having sufficient optical bandwidth to not cause severe spectrum narrowing of the input broadband optical radiation.
- EDFA Erbium-doped fiber amplifier
- Optically broadband radiation modulated and optionally amplified as described above is further coupled into (specifically, but not exclusively) a multimode optical fiber or waveguide (MMF) of the length L satisfying Eq. (4) or Eq. (5).
- MMF multimode optical fiber or waveguide
- An offset splice or connection is used to uniformly excite a large number of fiber modes with approximately equal intensities.
- a mode scrambler may be used for the purpose of uniform excitation of a large number of modes.
- STPCB desired spatio-temporally partially coherent optical beam
- Propagation of the broadband optical radiation through a relatively short length L of MMF is usually not associated with substantial losses, making the generation of STPCB essentially penalty-free in terms of the optical power.
- the STPCB produced at the output of the MMF and carrying the communication data signal is subsequently prepared for transmission through the communication medium, such as atmosphere, by enlarging its aperture to the dimension desired, for example 10 centimeters in diameter, and by properly collimating.
- the STPCB may be enlarged and substantially collimated using a lens, a mirror or a more complex telescope assembly known in the art.
- the same assembly may be used for the receiving of the optical signal propagating in the opposite direction in a full duplex FSO communication link, for which a means to separate the incoming beam from the outcoming beam, such as a beamsplitter, is used.
- the enlargement of the SPCB produced at the output of the MMF may also be done by imaging the optical core of the MMF with magnification to the desired dimension by using a double-lens telecentric system.
- the enlarged and substantially collimated STPCB modulated with the communication data signal and optionally optically amplified as described above is further eradiated into the communication medium, such as atmosphere, towards the receiver.
- the communication medium such as atmosphere
- techniques for pointing and tracking known in the art may be used to facilitate the directing of the transmitted STPCB.
- the receiver operates in a manner typical for the art by intercepting at least a portion of the incoming optical beam.
- a lens or a mirror or a more complex optical telescope assembly similar or optionally the same as the one used for transmission (in case of a full-duplex FSO communication system sharing the same optical head for transmitting and receiving optical signals), concentrates the intercepted portion of the incoming optical beam to the dimension suitable for high-speed detection.
- the concentrated received light is projected on the active surface of an optical detector suitable for detecting the communication data stream chosen for the FSO communication link.
- the detector may comprise any of a number of intensity detectors known in the art, such PIN, avalanche, or photon-counting detectors.
- the detector may also be optical fiber-coupled.
- Fig. 4A schematically illustrates a system with directly or externally modulated broadband optical source 10 coupled to MMF 11, the output of which is an STPCB, which is further substantially collimated with an optical system 12, such as a lens, spherical or parabolic mirror, an array of lenses or mirrors, a telescope, or similar system, for sending STPCB into the transmission medium 13, such as atmosphere, toward the receiving end of the communication link 14.
- Fig. 4B schematically illustrates a system with an optical amplifier 15 used to increase the power of the transmitted optical signal.
- Fig. 4C further illustrates a system in which a mode scrambler 16 or a similar device is used to enhance the excitation of a large number of modes in the MMF.
- the system offered herein possess the optional advantage of optical-only fiber-coupling the transmitter and receiver heads to the rest of the system. There is no need for any electronic components within the optical heads, which are usually located outside the protected space on the roof tops, towers and moving platforms. This feature improves the electromagnetic immunity of the overall system as previously discussed.
- the simplicity of the method and the system disclosed herein allows for easy and inexpensive upgrade of existing FSO systems to include a broadband light source and a multimode optical fiber or waveguide of a certain moderate length to readily take advantage of the scintillation reduction and thus substantially improve the quality of the FSO communication link.
- the SLD incorporates an optical isolator, a polarization-maintaining single-mode fiber pigtail terminated with an FC/PC fiberoptic connector.
- the SLD is preferably housed in a standard 14-pin butterfly housing commonly used in the art.
- the SLD preferably further incorporates a thermoelectric (TE) cooler for temperature stabilization.
- the SLD is driven using standard techniques known in the art by supplying required electrical voltages and currents to the pins of the SLD.
- a standard Lithium Niobate external optical intensity modulator is employed for imprinting the communication data stream on the broadband light produced by the SLD.
- the modulator has an input single-mode fiberoptic pigtail and an output single-mode fiberoptic pigtail, both terminated with FC/PC connectors.
- the output of the SLD is connected to the input of the modulator using a bulkhead optical FC-FC adapter.
- the modulator is driven by a RF communication data signal with standard means known in the art at the bit rate chosen by the user, for example 2.5 Gbps.
- the Erbium-doped fiber amplifier can be used.
- the maximum output power of the EDFA can be, for example, 23dBm, or 200 milliwatts.
- the EDFA has an input single-mode fiberoptic pigtail and an output single-mode fiberoptic pigtail, both terminated with FC/PC connectors.
- the output of the modulator is connected to the input of the EDFA using a bulkhead optical FC-FC adapter.
- the output of the system (output fiber pigtail of the EDFA) so far described comprises a high-power broadband single spatial mode optical light intensity modulated with the communication data stream at 2.5 Gbps.
- a length of multimode optical fiber is connected to the output of the EDFA.
- the MMF used is a standard and inexpensive step-index optical fiber with optical core diameter of 100 micrometers and a length of approximately 2 meters.
- the MMF can be prepared or purchased in the form of a jacketed patch cord with FC/PC connectors on both ends.
- the output of the EDFA is connected to the input of the MMF using a bulkhead optical FC-FC adapter.
- the visual image of the MMF output as obtained, for example by shining the light on the surface of an infrared-sensitive card, should be of low-contrast, as in Fig. 3D.
- the output of the system (output of the MMF) so far described comprises a high-power broadband STPCB intensity modulated with the communication data stream at 2.5 Gbps.
- the STPCB emanating from the output of the MMF is coupled into a collimation system which also enlarges its aperture.
- a standard double-mirror reflective telescope for example a Newtonian telescope
- the telescope is fitted with a FC/PC fiber receptacle in such a way that the output plane of the FC connector ferrule, when attached to the receptacle, approximately coincides with the focal plane of the telescope.
- Said receptacle can preferably have a mechanism for small adjustment of the position of the ferrule output plane with respect to the telescope's focal plane for the purpose of allowing minor tuning of the beam collimation.
- the output end of the MMF is connected to the telescope via said receptacle.
- the output of the system (output of the telescope) so far described comprises a STPCB of large aperture, substantially collimated and intensity modulated with the communication data stream at 2.5 Gbps.
- the telescope being the optical transmitter within the present discussion is further attached to a mounting system and to a steering system, which is used to steer the beam being output by the telescope in the direction of the receiver.
- the receiver is intended to intercept at least a portion of the STPCB eradiated by the transmitter.
- the best mode receiver comprises a double-mirror Newtonian telescope very similar or identical to the one used in optical transmitter described above.
- the telescope is fitted with a FC/PC fiber receptacle in such a way that the tip of the FC connector ferrule, when attached to the receptacle, approximately coincides with the focal plane of the telescope.
- Said receptacle can preferably have a mechanism for small adjustments of the position of the ferrule plane with respect to the telescope's focal plane for the purpose of allowing minor tuning of the coupling of the intercepted and concentrated beam into the receiving fiber.
- the detector used to detect the incoming light carrying the communication data is chosen to have a fiber pigtail with a standard FC/PC connector at the end of the pigtail. This connector is attached to the receiving telescope's FC/PC fiber receptacle.
- the detector's pigtail fiber is preferably a multimode fiber with 50 micrometer diameter core or more preferably with 100 micrometer diameter core. Large-core pigtails are preferred for better coupling of the incoming light and relaxed pointing requirements of the receiving telescope.
- the length of the multimode pigtail should not be excessive as to not substantially stretch the individual data carrying bits of the communication signal due to fiber dispersion.
- One-meter long pigtail is preferred and is standard in the art.
- the data received by the detector in the form of the electrical signal is amplified, conditioned and processed and the data signal extracted with the standard means known in the art.
- the decoding scheme employed at the receiving end of the FSO link should match the encoding scheme employed at the transmitting end of the FSO link, with data modulation formats and forward error correction codes, if any properly handled.
Abstract
The apparatus and the method are offered for substantial reduction in scintillations, signal fade depth, duration and probability of occurrence in a free-space optical communication system through a turbulent medium, such as atmosphere. A spatio-temporally partially coherent optical beam (STPCB) is produced by coupling a sufficiently broadband optical light into a sufficiently long multimode optical fiber or waveguide and is used for communication. The length of the fiber and the spectral width of the light are such that intermodal delay of the majority of the modes exceeds the inverse spectral width of the broadband optical source, but is smaller than the duration of the bit in the communication data stream.
Description
The present invention pertains to
free-space optical communication through turbulent
medium, such as atmosphere, and in particular to
methods and approaches for reducing scintillations and
minimizing signal fades.
In long-range free-space optical (FSO)
communication links, such as those exceeding a few
kilometers and operating under turbulent conditions in
the communication medium, such as atmosphere, the
optical beam arrives at the receiver's input
aperture highly spatially deteriorated. This is
because the random fluctuations in the refractive index
of air ever so slightly bend and scatter the optical
beam or its portions, the effect being accumulated
over the distance of propagation. Thus, the received
optical beam typically becomes fragmented, consisting
of a pattern of bright and dark spots, called
speckles. Moreover, these spots are constantly moving
and fluctuating on the time scale of the atmospheric
turbulence of about one millisecond.
As a result, the signal received by the
detector coupled to the optical receiver at the
receiving end of the FSO communication link may
strongly fluctuate in time, which decreases the
performance of the link. Such fluctuations are called
scintillations and are characterized by a
scintillation index. Stronger fluctuations are
characterized by a larger value of the scintillation
index, e.g. 1 or more. Deep signal dropouts, called
fades, occur more frequently and last longer when the
scintillation index is large. For example these fades
may occur many times per second and last for a
millisecond or longer. Under such conditions a typical
FSO communication link shows large error rates, low
reliability or complete loss of signal. Thus, the
methods and the systems designed to reduce the
scintillations and minimize signal fades as much as
possible are of great importance for FSO communication.
Good methods and systems must also be simple, reliable
and inexpensive.
Direct averaging of the scintillating
signal over time cannot be used for high data rate FSO
communication because of the slow rate of atmospheric
fluctuations. For example, taking into account the fact
that the characteristic time scale of the atmospheric
turbulence is about one millisecond the effective
averaging time of ten milliseconds or more is
required. Ten-millisecond or longer averaging for each
bit of the data stream will require the data rate of
one hundred bits per second or less. Clearly, the
required method and system should not only reduce
scintillations, but do so in the manner applicable to
the high bit-rate communication.
A number of methods to reduce
scintillations in view of the above arguments were
offered in the past. One of these methods is based on
using adaptive optical systems. However, such systems
are of limited use due to high complexity and cost, as
well as the need for a feedback signal (with
associated latency due to finite speed of light) to
operate properly. Furthermore, such systems involve
sensitive electronic components inside optical
transmitter and/or receiver heads. This increases the
sensitivity of the system to atmospheric electricity,
such as lightning, and requires uninterrupted supply
of electrical power to the optical transmitter and/or
receiver head, which is often located outside the
protected space, on the roof tops, towers and moving
platforms. For military applications, such system would
also be susceptible to electromagnetic interference
(EMI) or electromagnetic pulse (EMP) attack.
Another method for scintillation
reduction in FSO communication systems utilizes the
MIMO (multiple-input, multiple-output) paradigm known
in radiofrequency (RF) communication systems. Such
approach involves the use of several independent
transmitters separated in space and communicating the
same data signal. Essentially the multiple transmitters
used in this approach send mutually incoherent light
beams through somewhat different optical paths the
assumption being that the probability of a fade on all
of these paths occurring simultaneously is small. This
approach, however, is still rather complex, involving
a large number of independent lasers and corresponding
collimating optical systems, which need to be precisely
aligned with each other. If the optical transmitter
head is operated remotely from its electronics
counterpart a large number of equal-length optical
fibers connecting the transmitting lasers to their
respective transmitting apertures would be required.
Still in other methods it is claimed
that scintillation reduction can be achieved by using
rough-surface phase masks or optical diffusers placed
in the pathway of a temporally coherent light beam
carrying the communication signal before it is send
through atmosphere. Such phase masks or diffusers
allegedly scramble the laser beam's spatial phase
distribution to create a 'partially-coherent'
optical beam. Though this approach indeed provides a
complicated transverse phase and intensity profile of
the beam that appears random, this profile remains
stationary in time. In other words, the temporal
coherence of the optical radiation remains unchanged
after passing through the phase mask or diffuser, and is
equal to the temporal coherence of the laser. The
optical beam at the output of the phase mask or
diffuser in this case can be considered as a set of
multiple randomly distributed mutually coherent
sources with stationary amplitudes and phases and can
be called 'partially coherent' only to some extent.
In theoretical treatments true partial
coherence is understood to imply ensemble average.
This means taking multiple independent realizations of
the optical beam's transverse phase and amplitude
and averaging over these realizations to obtain the
final result. In reality, the advantages of a true
partially coherent beam can be realized only by applying
the ergodicity conjecture, i.e. is the equivalence of
ensemble average and the average over time. To take
advantage of averaging over time what is needed then
is a true partially coherent beam in both space and time
with short temporal coherence. The crossection of such
true partially coherent beam comprises multiple
randomly distributed and mutually incoherent sources.
The characteristic coherence time of such true
partially coherent beam also needs to be much shorter
than the duration of the averaging. For example, if it
is desired to average the received signal over the
duration of one bit in the communication data stream,
as is done in all RF bandwidth-limited detection
systems, the true partially coherent beam would need to
cycle through many independent realizations of its
phase and amplitude during the time of one bit. In
other words, the characteristic temporal coherence time
of the true partially coherent beam should be much
shorter than the duration of the bit in order to take
advantage of the averaging discussed above.
In accordance with the present invention,
there are provided improved method and system for
free-space optical communication with reduced scintillations.
There exist at least two important
conditions for high bit-rate FSO communication with
reduced-scintillation between an optical transmitter and
an optical receiver through turbulent medium, such as atmosphere:
1) Transmitted optical signal should
reach the detector via a number of substantially
independent (uncorrelated) paths through atmosphere so
that the probability of fade on all of those paths is
minimized, and
2) Optical signals reaching the detector
via different paths should not produce detectable optical interference.
In the present invention the above
conditions are satisfied by employing a spatio-temporally
partially coherent optical beam (STPCB) transmitted from
the optical transmitter to the optical receiver having
substantially large apertures.
Prior to offering the detailed
description of STPCB, its action and benefit is better
illustrated by example. The exact speckle structure of the
light, i.e. the position of bright and dark spots on the
receiver's aperture, after propagation through
turbulent atmosphere depends on both the state of the
atmosphere and the spatio-temporal properties of the
optical beam eradiated by the transmitter. In particular,
these spatio-temporal properties include the transverse
distribution of phase and amplitude of the light, as well
as their variation in time. For one particular moment of
time t0 the transmitted optical beam with
certain transverse phase and intensity distribution
results in a certain speckle structure on the receiver
aperture. For the next moment of time
t1=t0+Delta_t, separated from the
first by a delay Delta_t, another transverse phase and
intensity distribution of the transmitted beam results in a
substantially different speckle structure on the receiver
aperture, Fig. 1A. The time delay Delta_t is chosen to be
much shorter than the duration of each bit in the
communication data stream. At a further delayed moment of
time t3=t2+Delta_t the speckle
structure changes yet again and so on. Because the
characteristic time of speckle pattern change Delta_t is
much shorter than the bit duration, the optical detector
coupled to the optical receiver effectively averages
multiple speckle structure realizations during each bit of
the data stream, Fig. 1B. Importantly, the speckle
structures discussed above are different even for
'frozen' atmosphere, which it is on the time
scales of the data bit duration. The speckle structure
changes with the rate of change of the transmitted beam
phase and intensity distribution and not with the rate of
the atmosphere. Thus, the slow signal fluctuations due to
atmospheric turbulence are now replaced with fast
fluctuations due to such spatio-temporally partially
coherent optical beam (STPCB) action. The latter
fluctuations can be averaged with a detector having finite
radiofrequency (RF) bandwidth during each bit of the data
stream. Provided the STPCB's rate is substantially
faster than the communication data rate, or equivalently the
STPCB's coherence time is substantially shorter than
the duration of the bit, effective averaging is possible
with the benefit of suppressing signal scintillations and
deep signal fades typical for standard FSO systems.
By way of a further example, for a
communication signal data rate of 1 Gbps the update rate
of STPCB needs to be 10 GHz or higher to bring forth the
advantages of averaging described above. The present
invention teaches a very simple way of generating and using
STPCBs with virtually unlimited update rates (short
coherence times) suitable for high bit-rate FSO
communication systems. Still, the STPCB may be modulated
with communication data in a number of standard ways known
in the art, e.g. with amplitude modulation.
The STPCB may be generated by coupling a
broadband optical radiation into an optical system
including a number of different optical paths (modes) with
different delays, such as, for example, a volume
diffraction element, another example being a multimode
optical fiber or waveguide (MMF). There exist a certain
mathematical expression relating the spectral width of the
broadband optical radiation and the parameters of the MMF,
most importantly its length, the fulfillment of which is
required for the generation of proper STPCB, suitable for
scintillation reduction in a high-rate FSO communication
system. The MMF must also preferably possess an appreciable
amount of intermodal dispersion, which is the difference in
propagation speeds of various modes. Gradient-index MMFs
typically have small amount of intermodal dispersion and
thus are not preferred to be used for, although not excluded
from the use in the STPCB generation. On the other hand,
step-index MMFs typically have large amount of intermodal
dispersion and are thus preferred for the STPCB
generation. Step-index MMFs will be assumed in the following arguments.
By way of example consider the source of
broadband optical radiation mentioned above to be a
multi-frequency laser, such as Fabri-Perot laser, the
schematic spectrum of which is shown in Fig. 2C. Such
laser emits a number of distinct optical frequencies
f1, f2,...fn oscillating
with random uncorrelated phases. When coupled into the MMF
each frequency excites essentially the same set of
transverse spatial modes of the MMF. These modes propagate
at different velocities towards the output end of the MMF.
The interference of these modes at each individual optical
frequency creates a distinct transverse phase and
intensity pattern at the output of the MMF. Two examples of
such intensity patterns are shown in Fig. 3B and Fig. 3C
corresponding to a small and a large number of modes
excited in the MMF respectively.
Importantly, the optical phase
accumulated by each mode at different frequencies of the
laser will be different. Thus, the intermodal interference
patterns produced by different frequencies of the laser
after propagation through MMF will be substantially
different. Each spatial pattern corresponding to each
individual frequency of the laser may be considered to be
an independent optical emitter with complicated transverse
phase and amplitude distributions. For a large number of
overlapping independent emitters operating at many
different frequenciesand unrelated phases the resulting
overall distribution of phase and amplitude will fluctuate
rapidly and essentially randomly thus forming an STPCB.
After propagation through the communication medium, such
as turbulent atmosphere, the subset of optical frequencies
will reach the detector. The beat note between adjacent
laser frequencies will not be effectively detected by the
detector due to the limited RF bandwidth of the latter.
Only the data modulation signal being within the RF
bandwidth of the detector will be effectively received.
A continuous-spectrum broadband optical
source, such as the one shown in Fig. 2A can be viewed as
a limiting case of the example considered above with the
separation between neighboring frequencies reduced to zero
and a corresponding increase in the number of individual
frequencies - to infinity. One difference from the
previous case is that the beat note between the two
adjacent frequencies now falls within the RF bandwidth of
the detector. However, the beat notes between multiple
pairs of adjacent frequencies oscillate with random phases
and effectively produce a negligible noise and continuous
DC background, which is usually filtered out by the detector
or otherwise do not substantially affect the ability of
the detector to receive the desired communication signal.
An example of transverse spatial
intensity profile of an STPCB as measured by a slow
detector, for example a CCD camera, is shown in Fig. 3D.
Unlike the profiles shown in Fig. 3B and Fig. 3C
corresponding to a narrowband optical source or a very
short length of the MMF, the STPCB intensity profile has
very low contrast. This is because the slow CCD camera
cannot temporally resolve all the rapid fluctuations of the
light and thus produces an averaged picture. The
measurement of contrast just described may, in fact, serve
as an indication of the quality of the STPCB: Lower observed
contrast indicates a better quality STPCB for the purpose of
scintillation reduction in an FSO communication link. For
completeness Fig. 3A shows the intensity profile at the
output of a single-mode optical fiber. This profile is a
familiar bell-shaped 2-dimentional distribution, which
essentially does not depend on the spectral width of the
optical source and the length of the fiber.
As was mentioned above the desired STPCB
can be obtained only under certain, although easily
fulfilled conditions. Specifically, detailed
considerations yield the following simple relation for the
case of discrete-frequency optical source:
where L is the physical length of the
MMF, n is its average refractive index, NA is its
numerical aperture, c is the speed of light and Delta_f is
the frequency difference between the two adjacent optical
frequencies of the optical source. For the case of
continuous-spectrum broadband optical source an equivalent
relation can be written as:
where Delta_F is the full spectral width
of the optical source and M is the desired number of
effective independent sources in the context of the above
discussion. Larger values of M, say 100, generally results
in a better-quality STPCB.
The length L of the MMF cannot be too
large, however. This is because the dispersion in the MMF
aside from helping to generate STPCB also temporally
stretches the data bits comprising the communication
signal stream. The condition expressing the requirement that
this temporal stretch is small reads:
where T is the duration of the bit.
Combining the two conditions above one
can write: , for discrete-frequency
optical source (4) , for continuous-spectrum
broadband optical source (5)
By way of example, for a
discrete-frequency optical source with Delta_f=100GHz and
a MMF with n=1.5 and NA=0.22, and for a 1Gbps data rate of
the communication link from the first equation above one can
obtain approximately:
which can be readily satisfied with a MMF
length of about one meter.
The quality of STPCB and with it the
effectiveness of temporal averaging discussed above
dependson the number of paths ormodes excited in theSTPCB
creating system such as MMF.It is therefore desired tohave
a substantially uniform excitation of the modesof the MMF,
i.e.excite as large number of modes as possible with
preferably equal intensities. As known in the art, to
excite a large number of modes with approximately equal
intensitiesan offset splice or connection between the
input fiber and the MMF may be applied.Similar result can
be reached by using a mode scrambler.Further optimization
of STPCB generation may be obtained by connecting several
different or similarpieces of multimode fibers or
waveguides. In the case of another intensity distribution
is desired, such as predominantly higher number modes
excitation or other distribution, an appropriate method
could be applied.
It is, therefore, the objective of the
present invention to teach the method and to describe the
apparatus for FSO communication with reduced
scintillations using simple and effective methods for
generating, modulating transmitting and receiving
spatio-temporally partially coherent optical beams
(STPCBs). The method and the apparatus of the present
invention may be applied with benefit to one-way and two-way
communication for point-to-point and point-to multipoint FSO
applications between stationary and moving platforms.
Other advantages of the method and the
system offered herein include:
a) improved performance and reliability
as compared to existing FSO communication systems;
b) increased simplicity and reduced cost
of manufacturing using standard off the shelf components;
c) electric power-free operation of the
optical transmitter's head;
d) insensitivity of the optical
transmitter's head to natural or man-made atmospheric electricity;
e) single-fiber connectivity of the
optical transmitter head
A further advantage is the ease with
which the existing FSO communication systems can be
upgraded to incorporate the method and the system of the
present invention thus yielding immediate performance
improvements described. Still further objectives and
advantages will become apparent from the consideration of
ensuing description and drawings.
According to one aspect of the present
invention, a method for free-space optical communication
with reduced scintillations is provided that includes:
(a) generating a broadband optical
radiation using at least one light source;
(b) modulating said broadband optical
radiation by a communication signal;
(c) generating a spatio-temporally
partially coherent optical beam by propagating said
broadband optical radiation through a multimode optical
fiber or waveguide;
(d) collimating said spatio-temporally
partially coherent optical beam to form a substantially
collimated spatio-temporally partially coherent optical
beam of large aperture;
(e) eradiating said substantially
collimated spatio-temporally partially coherent optical
beam of large aperture into a communication medium, such
as atmosphere;
(f) receiving at least a portion of said
substantially collimated spatio-temporally partially
coherent optical beam of large aperture after propagation
of said substantially collimated spatio-temporally
partially coherent optical beam of large aperture through
said communication medium;
(g) detecting said communication signal.
According to another aspect of the
present invention, an apparatus for free-space optical
communication with reduced scintillations is provided that includes:
(a) at least one source of broadband
optical radiation;
(b) a system for modulating said
broadband optical radiation with a communication signal;
(c) a multimode optical fiber or
waveguide adapted for generating a spatio-temporally
partially coherent optical beam;
(d) an optical collimation system adapted
for collimating said spatio-temporally partially coherent
optical beam to produce substantially collimated
spatio-temporally partially coherent optical beam of large
aperture and adapted for eradiating said substantially
collimated spatio-temporally partially coherent optical
beam of large aperture into a communication medium, such
as atmosphere;
(e) an optical receiver adapted for
receiving at least a portion of said substantially
collimated spatio-temporally partially coherent optical
beam of large aperture after propagation of said
substantially collimated spatio-temporally partially
coherent optical beam of large aperture through said
communication medium;
In one embodiment, the source of
broadband optical radiation is a low-coherence light source.
In another embodiment, the source of
broadband optical radiation is an ultrashort-pulse laser.
In a further embodiment, the source of
broadband optical radiation is a multiple-frequency
optical source.
In a further embodiment, the source of
broadband optical radiation is a plurality of
single-frequency optical sources with distinct central
optical frequencies.
In another embodiment, the system for
modulating said broadband optical radiation with said
communication signal is adapted for direct modulation of
the output of said source of broadband optical radiation.
In still another embodiment, the system
for modulating said broadband optical radiation with said
communication signal comprises an external optical modulator.
In another embodiment, the apparatus
further comprises an optical amplifier.
In another embodiment, the apparatus
further comprises a system for a substantially uniform
excitation of transverse modes of said multimode optical
fiber or waveguide.
In a further embodiment, the system for
achieving substantial collimation of said
spatio-temporally partially coherent optical beam to
obtain substantially collimated spatio-temporally partially
coherent optical beam of large aperture and eradiating
said substantially collimated spatio-temporally partially
coherent optical beam of large aperture into said
communication medium comprises at least one optical element
with positive optical power.
In still another embodiment, the system
for achieving substantial collimation of said
spatio-temporally partially coherent optical beam to
obtain substantially collimated spatio-temporally partially
coherent optical beam of large aperture and eradiating said
substantially collimated spatio-temporally partially
coherent optical beam of large aperture into said
communication medium is adapted for performing optical
magnification of an optical core of said multimode optical
fiber or waveguide to the transverse dimension of said
large aperture.
In another embodiment, the said optical
receiver further comprises a system for intercepting at
least a portion of said substantially collimated
spatio-temporally partially coherent optical beam of large
aperture after propagation through said communication medium
and concentrating the received potion of said
substantially collimated spatio-temporally partially
coherent optical beam of large aperture on an optical
detector, the system for intercepting comprising at least
one optical element with positive optical power.
In still another embodiment, the optical
detector is a fiber-coupled optical detector.
Still other objects and aspects of the
present invention will become readily apparent to those
skilled in this art from the following description wherein
there are shown and described preferred embodiments of
this invention, simply by way of illustration of the best
modes suited for to carry out the invention. As it will be
realized by those skilled in the art, the invention is
capable of other different embodiments and its several
details are capable of modifications in various obvious
aspects all without departing from the scope of the
invention. Accordingly, the drawings and description will
be regarded as illustrative in nature and not as restrictive.
For a more complete understanding of
the present invention and the advantages thereof,
reference is now made to the following description
taken in conjunction with the accompanying drawings, in which:
Fig. 1A illustrates an example of the
sequence of momentary beam intensity distributions of
spatio-temporally partially coherent optical beam.
Fig. 1B illustrates an example of
spatio-temporally partially coherent beam's
intensity distribution averaged during a one bit-long
time interval.
Fig. 2A illustrates an example of the
spectrum of a continuous-spectrum broadband light source.
Fig. 2B illustrates an example of the
spectrum of a source consisting of a number of
narrowband spectra
Fig. 2C illustrates an example of the
spectrum of a source consisting of a number of sharp lines.
Fig. 3A illustrates spatially
coherent light intensity distribution at the output of
a single-mode optical fiber which is essentially
independent on the spectral properties of the optical
source and the length of the fiber.
Fig. 3B illustrates spatially
coherent multimode light intensity distribution formed
by a small number of transverse modes of a multimode
optical fiber excited with a narrowband optical source.
Fig. 3C illustrates spatially
coherent multimode light intensity distribution formed
by a large number of transverse modes of a multimode
optical fiber excited with a narrowband optical source.
Fig. 3D illustrates a low-contrast
intensity distribution of a spatio-temporally
partially coherent optical beam formed at the output
of a multimode optical fiber excited with a broadband
optical source;
Fig. 4A is a schematic diagram of one
embodiment of the system.
Fig. 4B is a schematic diagram of one
embodiment of the system utilizing an optical amplifier.
Fig. 4C is a schematic diagram of one
embodiment of the system utilizing an optical
amplifier and a mode scrambler.
In light of the preceding discussion
the system for FSO communication with reduced
scintillations according to the present invention
comprises a transmitter and a receiver separated by the
communication medium, such as atmosphere, preferably
at the line of sight. The source of optical radiation
allocated in the transmitter emits a substantially broad
optical spectrum preferably in a single transverse mode.
The optical spectrum of the source may be continuous,
quasi-continuous or discrete within a finite bandwidth
with the requirement being that the inverse width of the
spectrum is substantially smaller than the duration of
one bit of the digital communication signal.
Specifically, but not exclusively, the broadband optical
source may be a low-coherence superluminescent diode,
an ultrashort-pulse laser, an optical supercontinuum
source, a Fabri-Perot type multi-frequency laser, a
number of single-frequency lasers with separate
central frequencies, or a combination of such sources.
Relatively inexpensive semiconductor optical sources of
the above type are currently available and may be used
in the system described herein. Several examples of
optical spectra of such sources are shown in Fig. 2. In
Fig. 2A is schematically shown a spectrum of a
continuous-spectrum optical source with the overall
spectral width Delta_F. Equation (5) above may be
applied to estimate the required spectral width Delta_F
for the most optimal STPCB generation. For example,
for M=100 effective independent sources and MMF length
not exceeding 100 cm the minimum spectral width Delta_F
should be about 1 THz, which for a
telecommunication-region source near 1.55 micrometer
central wavelength corresponds to less than 10
nanometers on the wavelength scale. Notably,
superluminescent diodes with such or larger bandwidths
are inexpensively available off the shelf.
Fig. 2B shows a spectrum of
quasi-continuous broadband optical source with several
separated relatively broad lines. Similar analysis as
outlined above can be applied to such source.
Fig. 2C schematically shows the
spectrum of a multi-frequency laser, such as
Fabri-Perot laser. The analysis for such laser is
preferably performed using Eq. (4) above and was
demonstrated above.
The communication data stream may be
modulated onto the optical radiation produced by the
broadband optical source discussed above by either a
direct modulation of the optical source itself via its
drive current modulation or by using an external
optical modulator. Specifically, but not exclusively
such external light modulator may be a Lithium Niobate
intensity modulator, an electroabsorption modulator or a
similar device that offers the modulation speeds and
modulation formats desired for the FSO communication
link. The current invention does not specify and is not
limited to any particular modulation format. However,
due to the nature of the optical beam used in the
present invention direct detection formats, such as OOK,
PPM will be preferred over the coherent detection
formats, such as DPSK, BPSK.
Before or after modulation of the
broadband optical signal with communication data the
broadband optical radiation may be optionally
amplified in an optical amplifier to increase the
transmitted power. Specifically, but not exclusively,
such amplification may be achieved using an
Erbium-doped fiber amplifier (EDFA) or a semiconductor
optical amplifier having sufficient optical bandwidth
to not cause severe spectrum narrowing of the input
broadband optical radiation.
Optically broadband radiation
modulated and optionally amplified as described above
is further coupled into (specifically, but not
exclusively) a multimode optical fiber or waveguide
(MMF) of the length L satisfying Eq. (4) or Eq. (5).
An offset splice or connection is used to uniformly
excite a large number of fiber modes with approximately
equal intensities. Alternatively, a mode scrambler may
be used for the purpose of uniform excitation of a
large number of modes. At the output of the MMF the
desired spatio-temporally partially coherent optical
beam (STPCB) is formed. Propagation of the broadband
optical radiation through a relatively short length L
of MMF is usually not associated with substantial
losses, making the generation of STPCB essentially
penalty-free in terms of the optical power.
The STPCB produced at the output of
the MMF and carrying the communication data signal is
subsequently prepared for transmission through the
communication medium, such as atmosphere, by enlarging
its aperture to the dimension desired, for example 10
centimeters in diameter, and by properly collimating.
Specifically, but not exclusively, the STPCB may be
enlarged and substantially collimated using a lens, a
mirror or a more complex telescope assembly known in
the art. The same assembly may be used for the
receiving of the optical signal propagating in the
opposite direction in a full duplex FSO communication
link, for which a means to separate the incoming beam
from the outcoming beam, such as a beamsplitter, is
used. The enlargement of the SPCB produced at the
output of the MMF may also be done by imaging the
optical core of the MMF with magnification to the
desired dimension by using a double-lens telecentric system.
The enlarged and substantially
collimated STPCB modulated with the communication data
signal and optionally optically amplified as described
above is further eradiated into the communication
medium, such as atmosphere, towards the receiver.
Optionally, techniques for pointing and tracking known
in the art may be used to facilitate the directing of
the transmitted STPCB.
The receiver operates in a manner
typical for the art by intercepting at least a portion
of the incoming optical beam. A lens or a mirror or a
more complex optical telescope assembly, similar or
optionally the same as the one used for transmission
(in case of a full-duplex FSO communication system
sharing the same optical head for transmitting and
receiving optical signals), concentrates the intercepted
portion of the incoming optical beam to the dimension
suitable for high-speed detection. Specifically, but
not exclusively, the concentrated received light is
projected on the active surface of an optical detector
suitable for detecting the communication data stream
chosen for the FSO communication link. For example, if
OOK modulation format is chosen the detector may
comprise any of a number of intensity detectors known
in the art, such PIN, avalanche, or photon-counting
detectors. The detector may also be optical fiber-coupled.
Several embodiments of an apparatus
employing the method disclosed herein are
schematically shown in Fig. 4. Fig. 4A schematically
illustrates a system with directly or externally
modulated broadband optical source 10 coupled to MMF
11, the output of which is an STPCB, which is further
substantially collimated with an optical system 12, such
as a lens, spherical or parabolic mirror, an array of
lenses or mirrors, a telescope, or similar system, for
sending STPCB into the transmission medium 13, such as
atmosphere, toward the receiving end of the
communication link 14. Fig. 4B schematically
illustrates a system with an optical amplifier 15 used
to increase the power of the transmitted optical
signal. Fig. 4C further illustrates a system in which
a mode scrambler 16 or a similar device is used to
enhance the excitation of a large number of modes in the MMF.
It may be reiterated again that the
system offered herein possess the optional advantage
of optical-only fiber-coupling the transmitter and
receiver heads to the rest of the system. There is no
need for any electronic components within the optical
heads, which are usually located outside the protected
space on the roof tops, towers and moving platforms.
This feature improves the electromagnetic immunity of
the overall system as previously discussed.
Furthermore, it may be observed that
the simplicity of the method and the system disclosed
herein allows for easy and inexpensive upgrade of
existing FSO systems to include a broadband light source
and a multimode optical fiber or waveguide of a certain
moderate length to readily take advantage of the
scintillation reduction and thus substantially improve
the quality of the FSO communication link.
For the purpose of demonstrating by
example a mode of practicing the invention presented
herein the following steps may be taken to assemble
and operate the apparatus and apply the method of the
present invention:
A relatively inexpensive broadband
semiconductor source of low-coherence light with
central wavelength being approximately 1550 nanometers
and average output power approximately 10 milliwatts,
specifically a Superluminescent Diode (SLD), is
chosen. Preferably the SLD incorporates an optical
isolator, a polarization-maintaining single-mode fiber
pigtail terminated with an FC/PC fiberoptic connector.
The SLD is preferably housed in a standard 14-pin
butterfly housing commonly used in the art. The SLD
preferably further incorporates a thermoelectric (TE)
cooler for temperature stabilization. The SLD is
driven using standard techniques known in the art by
supplying required electrical voltages and currents to
the pins of the SLD.
For imprinting the communication data
stream on the broadband light produced by the SLD a
standard Lithium Niobate external optical intensity
modulator is employed. The modulator has an input
single-mode fiberoptic pigtail and an output
single-mode fiberoptic pigtail, both terminated with
FC/PC connectors. The output of the SLD is connected to
the input of the modulator using a bulkhead optical
FC-FC adapter. The modulator is driven by a RF
communication data signal with standard means known in
the art at the bit rate chosen by the user, for
example 2.5 Gbps.
If larger optical power is desired a
standard optical amplifier, the Erbium-doped fiber
amplifier (EDFA) can be used. The maximum output power
of the EDFA can be, for example, 23dBm, or 200
milliwatts. The EDFA has an input single-mode
fiberoptic pigtail and an output single-mode
fiberoptic pigtail, both terminated with FC/PC
connectors. The output of the modulator is connected
to the input of the EDFA using a bulkhead optical FC-FC adapter.
The output of the system (output
fiber pigtail of the EDFA) so far described comprises
a high-power broadband single spatial mode optical
light intensity modulated with the communication data
stream at 2.5 Gbps.
Further, for the purpose of
generating STPCB a length of multimode optical fiber
(MMF) is connected to the output of the EDFA. The MMF
used is a standard and inexpensive step-index optical
fiber with optical core diameter of 100 micrometers
and a length of approximately 2 meters. The MMF can be
prepared or purchased in the form of a jacketed patch
cord with FC/PC connectors on both ends. The output of
the EDFA is connected to the input of the MMF using a
bulkhead optical FC-FC adapter. The visual image of
the MMF output as obtained, for example by shining the
light on the surface of an infrared-sensitive card,
should be of low-contrast, as in Fig. 3D.
The output of the system (output of
the MMF) so far described comprises a high-power
broadband STPCB intensity modulated with the
communication data stream at 2.5 Gbps.
For the purpose of transmitting the
STPCB thus obtained through the communication medium,
such as atmosphere, the STPCB emanating from the
output of the MMF is coupled into a collimation system
which also enlarges its aperture. To this end a
standard double-mirror reflective telescope, for
example a Newtonian telescope, can be used. The
telescope is fitted with a FC/PC fiber receptacle in
such a way that the output plane of the FC connector
ferrule, when attached to the receptacle, approximately
coincides with the focal plane of the telescope. Said
receptacle can preferably have a mechanism for small
adjustment of the position of the ferrule output plane
with respect to the telescope's focal plane for
the purpose of allowing minor tuning of the beam
collimation. The output end of the MMF is connected to
the telescope via said receptacle.
The output of the system (output of
the telescope) so far described comprises a STPCB of
large aperture, substantially collimated and intensity
modulated with the communication data stream at 2.5 Gbps.
The telescope being the optical
transmitter within the present discussion is further
attached to a mounting system and to a steering
system, which is used to steer the beam being output by
the telescope in the direction of the receiver. The
receiver is intended to intercept at least a portion
of the STPCB eradiated by the transmitter.
The best mode receiver comprises a
double-mirror Newtonian telescope very similar or
identical to the one used in optical transmitter
described above. Similarly, the telescope is fitted with
a FC/PC fiber receptacle in such a way that the tip of
the FC connector ferrule, when attached to the
receptacle, approximately coincides with the focal plane
of the telescope. Said receptacle can preferably have
a mechanism for small adjustments of the position of
the ferrule plane with respect to the telescope's
focal plane for the purpose of allowing minor tuning of
the coupling of the intercepted and concentrated beam
into the receiving fiber. For the purpose of the best
mode description the detector used to detect the
incoming light carrying the communication data is chosen
to have a fiber pigtail with a standard FC/PC
connector at the end of the pigtail. This connector is
attached to the receiving telescope's FC/PC fiber
receptacle. The detector's pigtail fiber is
preferably a multimode fiber with 50 micrometer
diameter core or more preferably with 100 micrometer
diameter core. Large-core pigtails are preferred for
better coupling of the incoming light and relaxed
pointing requirements of the receiving telescope.
However, the length of the multimode pigtail should
not be excessive as to not substantially stretch the
individual data carrying bits of the communication
signal due to fiber dispersion. One-meter long pigtail
is preferred and is standard in the art.
The data received by the detector in
the form of the electrical signal is amplified,
conditioned and processed and the data signal
extracted with the standard means known in the art. The
decoding scheme employed at the receiving end of the
FSO link should match the encoding scheme employed at
the transmitting end of the FSO link, with data
modulation formats and forward error correction codes,
if any properly handled.
The foregoing description of the
preferred embodiments of the subject application has
been presented for purposes of illustration and
description. It is not intended to be exhaustive or to
limit the subject application to the precise form
disclosed. Obvious modifications or variations are
possible in light of the above teachings. The
embodiments were chosen and described to provide the
best illustration of the principles of the subject
application and its practical application to thereby
enable one of ordinary skill in the art to use the
subject application in various embodiments and with
various modifications as are suited to the particular
use contemplated. All such modifications and
variations are within the scope of the subject
application as determined by the appended claims when
interpreted in accordance with the breadth to which
they are fairly, legally and equitably entitled.
Claims (26)
- A method for free-space optical communication with reduced scintillations, the method comprising:(a) generating a broadband optical radiation using at least one light source;(b) modulating said broadband optical radiation by a communication signal;(c) generating a spatio-temporally partially coherent optical beam by propagating said broadband optical radiation through a multimode optical fiber or waveguide;(d) collimating said spatio-temporally partially coherent optical beam to form a substantially collimated spatio-temporally partially coherent optical beam of large aperture;(e) eradiating said substantially collimated spatio-temporally partially coherent optical beam of large aperture into a communication medium, such as atmosphere;(f) receiving at least a portion of said substantially collimated spatio-temporally partially coherent optical beam of large aperture after propagation of said substantially collimated spatio-temporally partially coherent optical beam of large aperture through said communication medium;(g) detecting said communication signal.
- The method of claim 1 wherein said light source is a low-coherence optical source.
- The method of claim 1 wherein said light source is an ultrashort-pulse laser.
- The method of claim 1 wherein said light source is a multiple-frequency optical source.
- The method of claim 1 wherein said light source is a plurality of single-frequency optical sources with distinct central optical frequencies.
- The method of claim 1 wherein the modulation of said broadband optical radiation with said communication signal is performed by directly modulating said light source.
- The method of claim 1 wherein the modulation of said broadband optical radiation with said communication signal is performed by using an external modulator.
- The method of claim 1 wherein said broadband optical radiation is amplified by an optical amplifier.
- The method of claim 1 wherein the generation of said spatio-temporally partially coherent optical beam in said multimode optical fiber or waveguide is performed using substantially uniform excitation of transverse modes of said multimode optical fiber or waveguide.
- The method of claim 1 wherein at least one optical element with positive optical power is used for collimating said spatio-temporally partially coherent optical beam to form said substantially collimated spatio-temporally partially coherent optical beam of large aperture.
- The method of claim 1 wherein collimating said spatio-temporally partially coherent optical beam to form said substantially collimated spatio-temporally partially coherent optical beam of large aperture is performed by image transfer with magnification of the optical core of said multimode optical fiber or waveguide to the dimension of said large aperture.
- The method of claim 1 wherein receiving at least a portion of said substantially collimated spatio-temporally partially coherent optical beam of large aperture after propagation of said substantially collimated spatio-temporally partially coherent optical beam of large aperture through said communication medium is performed by concentrating the received optical beam on an optical detector using an optical system comprising at least one optical element with positive optical power.
- The method of claim 12 wherein said optical detector is a fiber-coupled optical detector.
- An apparatus for free-space optical communication with reduced scintillations, the apparatus comprising:(a) at least one source of broadband optical radiation;(b) a system for modulating said broadband optical radiation with a communication signal;(c) a multimode optical fiber or waveguide adapted for generating a spatio-temporally partially coherent optical beam;(d) an optical collimation system adapted for collimating said spatio-temporally partially coherent optical beam to produce substantially collimated spatio-temporally partially coherent optical beam of large aperture and adapted for eradiating said substantially collimated spatio-temporally partially coherent optical beam of large aperture into a communication medium, such as atmosphere;(e) an optical receiver adapted for receiving at least a portion of said substantially collimated spatio-temporally partially coherent optical beam of large aperture after propagation of said substantially collimated spatio-temporally partially coherent optical beam of large aperture through said communication medium.
- The apparatus of claim 14 wherein said source of broadband optical radiation is a low-coherence light source.
- The apparatus of claim 14 wherein said source of broadband optical radiation is an ultrashort-pulse laser.
- The apparatus of claim 14 wherein said source of broadband optical radiation is a multiple-frequency optical source.
- The apparatus of claim 14 wherein said source of broadband optical radiation is a plurality of single-frequency optical sources with distinct central optical frequencies.
- The apparatus of claim 14 wherein said system for modulating said broadband optical radiation with said communication signal is adapted for direct modulation of the output of said source of broadband optical radiation.
- The apparatus of claim 14 wherein said system for modulating said broadband optical radiation with said communication signal comprises an external optical modulator.
- The apparatus of claim 14 further comprising an optical amplifier.
- The apparatus of claim 14 further comprising a system for a substantially uniform excitation of transverse modes of said multimode optical fiber or waveguide.
- The apparatus of claim 14 wherein the system for achieving substantial collimation of said spatio-temporally partially coherent optical beam and eradiating said substantially collimated spatio-temporally partially coherent optical beam of large aperture into said communication medium comprises at least one optical element with positive optical power.
- The apparatus of claim 14 wherein the system for achieving substantial collimation of said spatio-temporally partially coherent optical beam and eradiating said substantially collimated spatio-temporally partially coherent optical beam of large aperture into said communication medium is adapted for performing optical magnification of an optical core of said multimode optical fiber or waveguide to the transverse dimension of said substantially collimated spatio-temporally partially coherent optical beam of large aperture.
- The apparatus of claim 14 wherein said optical receiver further comprises a system for intercepting at least a portion of said substantially collimated spatio-temporally partially coherent optical beam of large aperture after propagation through said communication medium and concentrating the received potion of said substantially collimated spatio-temporally partially coherent optical beam of large aperture on an optical detector, the system for intercepting comprising at least one optical element with positive optical power.
- The apparatus of claim 25 wherein said optical detector is a fiber-coupled optical detector.
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US30380510P | 2010-02-12 | 2010-02-12 | |
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