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/dokumenty/skolni/diplomka/conclusion.tex
1,13 → 1,13
\chap Conclusion
Special design of scalable data-acquisition system was proposed. This system has unique parameters compared to state of the art radioastronomy signal processing hardware. Offered 16bit resolution and related dynamical range is more than other similar constructions could offer. We demonstrated system working on the most basic interferometric station. Other validation of reached parameters should be needed. After that, the final design will eventually become a part of MLAB Advanced Radio Astronomy System\cite[mlab-aras].
A special design of scalable data-acquisition system was proposed. This system has unique parameters compared to the state of the art radioastronomy signal processing hardware. Offering a 16bit resolution and comparable dynamical range is more than other similar constructions could offer. We demonstrated system functionality on the most basic interferometric station. Further validation of reached parameters would be necessary. Following that, the final design will eventually become a part of MLAB Advanced Radio Astronomy System\cite[mlab-aras].
All requirements demanding by specification have been reached or exceed. The required minimal sampling frequency 1 MHz has been exceeded fifth times at least. Requested dynamical range specified by 12 bit have been exceeded at least by 8 dB in decibel scale. As by-pass product of digitalisation unit design the software defined GPS disciplined oscillator device has been developed. This device is currently in use in several radio meteor detection station in Czech Republic.
All requirements demanded by the thesis specification have been reached or exceed. The required minimal sampling frequency of 1 MHz has been exceeded five times at least. Requested dynamical range specified by 12 bit have been exceeded at least by 8 dB in decibel scale. As by-pass product of digitalisation unit design the software defined GPS disciplined oscillator device has been developed. This device is currently in use on several radio meteor detection stations in Czech Republic.
On other hand the proposed design is not still perfect and some minor imperfections should be corrected in future work.
\sec Possible hardware improvements
The PCB design of the used modules might need more precise high-speed optimization of differential pairs. Improvement in high-speed routing allows a possible use of the fastest ADC from the Linear Technology devices family. The use of the faster ADCs even improve a range of possible usages. Minor ADC module imperfections, such as the unnecessary separation of FRAME and DCO signal to two connectors, should be mitigated. These two signals should be merged together to one SATA connector. With this modification we are able to remove one redundant SATA cable between the analog to digital converter device and between computational unit section.
The PCB design of the used modules might need more precise high-speed optimization of differential pairs. Improvement in high-speed routing allows a possible use of the fastest ADC from the Linear Technology devices family. The use of the faster ADCs even improves a range of possible usages. Minor ADC module imperfections, such as the unnecessary separation of FRAME and DCO signal to two connectors, should be mitigated. These two signals should be merged together to one SATA connector. With this modification we will be able to remove one redundant SATA cable between the analog to digital converter device and computational unit section.
\sec Possible software improvements

/dokumenty/skolni/diplomka/description.tex
13,17 → 13,17
\sec Required parameters
We require following technical parameter, to supersede existing digitalization units solutions.
Primarily, we need wide dynamical range and high IP3. The receiver must accept wide dynamic signals because a typical radioastronomical signal has a form of a weak signal covered by a strong man-made noise or other undesired noises as lighting, Sun emissions etc.
We require the following technical parameters, to supersede existing digitalization units solutions.
Primarily, we need wide a dynamical range and high IP3. The receiver must accept wide dynamic signals because a typical radioastronomical signal has a form of a weak signal covered by a strong man-made noise or other undesired noises as lighting, Sun emissions etc.
Summary of other additional required parameters follows
\begitems
* Dynamical range better than 80 dB see section \ref[dynamic-range-theory] for explanation
* Dynamical range better than 80 dB, see section \ref[dynamic-range-theory] for explanation
* Phase stability between channels
* Low noise (all types)
* Sampling jitter better than 100 metres
* Support for any number of receivers in range 1 to 8
* Support for any number of receivers in the range of 1 to 8
\enditems
Now we analyze several of the parameters in detail.
30,49 → 30,49
\sec Sampling frequency
Sampling frequency is not limited by the technical constrains in the trial design. This parameter is especially limited by the sampling frequencies of analog-to-digital conversion chips available on the market and interface bandwidth. Combination of the required parameters -- dynamic range requiring at least 16bit and a minimum sampling frequency of 1$\ $MSPS leads to need of high end ADC chips which does not support such low sampling frequencies at all. Their minimum sampling frequency is 5$\ $MSPS.
Sampling frequency is not limited by the technical constrains in the trial version. This parameter is especially limited by the sampling frequencies of analog-to-digital conversion chips available on the market and interface bandwidth. Combination of the required parameters -- dynamic range requiring at least 16bit and a minimum sampling frequency of 1$\ $MSPS leads to the need of high end ADC chips which does not support such low sampling frequencies at all. Their minimum sampling frequency is 5$\ $MSPS.
We calculate minimum data bandwidth data rate for eight receivers, 2 bytes per sample and 5$\ $MSPS as $8 \cdot 2 \cdot 5\cdot 10^6 = 80\ $MB/s. Such data rate is at the limit of real writing speed o classical HDD and it is almost double of real bandwidth of USB 2.0 interface. As result of this facts we must use faster interface. Faster interface is especially needed in case where we need faster sampling rates than ADC minimal 5$\ $MSPS sample rate.
Most perspective interfaces for use in our type of application is USB 3.0 or PCI Express interface. Although USB 3.0 is new technology without availability of good development tools. We used PCI Express interface as simplest and most reliable solution.
We calculated a minimum data bandwidth data rate for eight receivers, 2 bytes per sample and 5$\ $MSPS as $8 \cdot 2 \cdot 5\cdot 10^6 = 80\ $MB/s. Such data rate is at the limit of the actual writing speed of classical HDD and it is almost double the real bandwidth of USB 2.0 interface. As a result of these facts we must use faster interface. Faster interface is especially needed in cases where we require faster sampling rates than ADC's minimal 5$\ $MSPS sample rate.
The most perspective interface for use in our type of application is USB 3.0 or PCI Express interface. However, USB 3.0 is a relatively new technology without good development tools currently available. We have used PCI Express interface as the simplest and the most reliable solution.
\sec System scalability
For analogue channels scalability, special parameters of ADC modules are required. Ideally, there should be a separate output for each analogue channel in ADC module. ADC module must also have separate outputs for frames and data output clocks. These parameters allow for conduction at relatively low digital data rates. As a result, the digital signal can be conducted even through long wires. Modular concept allows separation from central logic which support optimization of number analogue channels.
For analogue channels' scalability, special parameters of ADC modules are required. Ideally, there should be a separate output for each analogue channel in ADC module. ADC module must also have separate outputs for frames and data output clocks. These parameters allow for conduction at relatively low digital data rates. As a result, the digital signal can be conducted even through long wires. Modular concept allows a separation from central logical unit which supports optimization of number analogue channels.
Clock and data signals will be then handled distinctively in our modular scalable design. Selected ADC chip are guaranteed to have defined clock skew between sampling and data output clock. This allows taking data and frame clocks from the first ADC module only. The rest of the data and frame clocks from other ADC modules can be measured for diagnostic purposes (failure detection, jitter measurement etc.) but these redundant signals are not used for data sampling. If more robustness is required in final application, DCO and FR signal may be collected from other modules and routed through an voting logic which will correct possible signal defects.
Clock and data signals will be then handled distinctively in our modular scalable design. Selected ADC chips are guaranteed to have defined clock skew between the sampling and data output clocks. This allows taking data and frame clocks from the first ADC module only. The rest of the data and frame clocks from other ADC modules can be measured for diagnostic purposes (failure detection, jitter measurement etc.), but these redundant signals are not used for data sampling. If more robustness is required in the final application, DCO and FR signals may be collected from other modules and routed through an voting logic which will correct possible signal defects.
This system concept allows for scalability, that is technically limited by a number of differential signals on host side and its computational power. There is another advantage of scalable data acquisition system -- an economic one. Observatories or end users can make a choice of how much money are they willing to spent on radioastronomy receiver system. This freedom of choice is especially useful for science sites without previous experience in radioastronomy observations.
\secc Differential signaling
\secc Differential signalling
The above mentioned concept of scalable design requires relatively long circuit traces between ADC and digital unit which captures the data and performs the computations. The long distance between the digital processing unit and the analog-to-digital conversion unit has an advantage in noise retention typically produced by digital circuits. Those digital circuits, such as FPGA, Ethernet or other flip-flops blocks and circuit traces, usually work at high frequencies and emit wide-band noise with relatively low power. In such cases any increase in a distance between the noise source and analog signal source increase S/N significantly. However, at the same time a long distance brings problems with the digital signal transmission between ADC and computational unit. But this obstacle should be resolved more easily in free-space than on board routing. The high-quality differential signalling shielded cables should be used such as massively produced and cheap SATA cables. This technology has two advantages over PCB signal routing. First, it can use twisted pair of wires for leak inductance suppression in signal path and second, the twisted pair may additionally be shielded by uninterrupted metal foil.
The above mentioned concept of scalable design requires relatively long circuit traces between ADC and digital unit which captures the data and performs the computations. The long distance between the digital processing unit and the analog-to-digital conversion unit has an advantage in noise retention typically produced by digital circuits. Those digital circuits, such as FPGA, Ethernet or other flip-flops blocks and circuit traces, usually work at high frequencies and emit wide-band noise with relatively low power. In such cases any increase in a distance between the noise source and analog signal source increase S/N significantly. However, at the same time, a long distance brings problems with the digital signal transmission between ADC and computational unit. But this obstacle should be resolved more easily in free-space than on board routing. The high-quality differential signalling shielded cables should be used, such as massively produced and cheap SATA cables. This technology has two advantages over PCB signal routing. First, it can use twisted pair of wires for leak inductance suppression in signal path and second, the twisted pair may additionally be shielded by uninterrupted metal foil.
\secc Phase matching
For multiple antenna radioastronomy projects, system phase stability is a mandatory condition. It allows precise high resolution imaging of objects, increases signal to noise ratios in several observation methods and allows use of advanced algorithms for signal processing.
For multiple antenna radioastronomy projects, system phase stability is a mandatory condition. It allows a precise, high resolution imaging of objects, increases signal to noise ratios in several observation methods and allows the use of advanced algorithms for signal processing.
High phase stability in our scalable design is achieved through centralized frequency generation and distribution with multi-output LVPECL hubs (CLKHUB02A), that have equiphased outputs for multiple devices. LVPECL logic is used on every system critical clock signal distribution hub. LVPECL logic has advantage over LVDS in signal integrity robustness. LVPECL uses higher logical levels and higher signalling currents. Power consumption of LVPECL logic are near constant over operating frequency range due to use of bipolar transistors this minimizes voltage glitches which are typical for CMOS logic. One drawbacks of that parameters is high power consumption of LVPECL logic which easily reach tens of milliamperes per device.
High phase stability in our scalable design is achieved through centralized frequency generation and distribution with multi-output LVPECL hubs (CLKHUB02A), that have equiphased outputs for multiple devices. LVPECL logic is used on every system critical clock signal distribution hub. LVPECL logic has an advantage over LVDS in signal integrity robustness. LVPECL uses higher logical levels and higher signalling currents. Power consumption of LVPECL logic is nearly constant over the operating frequency range due to the use of bipolar transistors. This minimizes voltage glitches which are typical for CMOS logic. One drawback of its parameters is a high power consumption of LVPECL logic which easily reaches tens of milliamperes per device.
This design ensures that all system devices have access to the defined phase and known frequency.
\sec System description
In this section testing system based on Xilinx ML605 development board \ref[ML605-development-board] will be described. This board was used in previous finished project and was unused until now, but FPGA parrameters are more than enough we need in fast data aquisition system.
This section deals with the description of the trial version based on Xilinx ML605 development board \ref[ML605-development-board]. The board had been used in a previous project and has not been used since then, but the FPGA parameters are more than sufficient of what we need for fast data acquisition system.
\secc Frequency synthesis
We have used a centralized topology as a basis for frequency synthesis. One precise high-frequency and low-jitter digital oscillator has been used \cite[MLAB-GPSDO], while other working frequencies have been derived from it by the division of its signal. This central oscillator has a software defined GPS disciplined control loop for frequency stabilization.\fnote{SDGPSDO design has been developed in parallel to this diploma thesis as a related project, but it is not explicitly required by the diploma thesis. Thus is described in separate document}
We have used new methods of software frequency monitoring and compensation in order to meet modern requirements on radioastronomy equipment which needs precise frequency and phase stability over a wide baseline scales for effective radioastronomy imaging.
We have used a centralized topology as a basis for frequency synthesis. One precise high-frequency and low-jitter digital oscillator has been used \cite[MLAB-GPSDO], while other working frequencies have been derived from it by the division of its signal. This central oscillator has a software defined GPS disciplined control loop for frequency stabilization.\fnote{SDGPSDO design has been developed in parallel to this diploma thesis as a related project, but it is not explicitly required by the thesis itself and thus it is described in a separate document}
We have used new methods of software frequency monitoring and compensation in order to meet modern requirements on radioastronomy equipment which need precise frequency and phase stability over a wide baseline scales for effective radioastronomy imaging.
GPSDO device consists the Si570 chip with LVPECL output. Phase jitter of GPSDO is determined mainly by Si570 phase noise. Parameters of used Si570 from source \cite[si570-chip] are summarized in table \ref[LO-noise].
The GPSDO device consists of Si570 chip with LVPECL output. Phase jitter of GPSDO is determined mainly by Si570 phase noise. Parameters of the Si570 are summarized in the following table \ref[LO-noise] (source \cite[si570-chip] ).
GPSDO design included in data acquisition system has special feature -- generates time marks for precise time-stamping of received signal. Timestamps are created by disabling of local oscillator outputs connected to SDRX01B receivers for 100 us. As result rectangle click in ADC input signal is created which appears as horizontal line in spectrogram.
Timestamps should be seen in image \ref[meteor-reflection] (above and below meteor reflection).
The GPSDO design, that is included in data acquisition system, has special feature -- it generates time marks for a precise time-stamping of the received signal. Timestamps are created by disabling the local oscillator's outputs, connected to SDRX01B receivers, for 100 us. As result, a rectangular click in the ADC input signal is created which appears as a horizontal line in spectrogram.
Timestamps should be seen in image \ref[meteor-reflection] (above and below the meteor reflection).
Time-marking should be improved in future by digitalization of GPS signal received by antenna on observational station. GPS signal can be then directly sampled by dedicated receiver and one separate ADC module. Datafile then consists samples from channels of radio-astronomy receivers along with GPS signal containing precise time information.
Time-marking should be improved in future by digitalization of GPS signal received by antenna on observational station. Following that, the GPS signal can be directly sampled by a dedicated receiver and one separate ADC module. Datafile then consists of samples from channels of radio-astronomy receivers along with the GPS signal containing precise time information.
\midinsert \clabel[LO-noise]{Phase noise of used local oscillator}
\midinsert \clabel[LO-noise]{Phase noise of the local oscillator}
\ctable{lcc}{
& \multispan2 \hfil Phase Noise [dBc/Hz] \hfil \cr
Offset Frequency & $F_{out}$ 156.25 MHz & $F_{out}$ 622.08 MHz \cr
84,10 → 84,10
10 [MHz] & –147 & –146 \cr
100 [MHz] & n/a & –148 \cr
}
\caption/t Phase noise of used Silicon Laboratories Si570 chip. Offset frequency is measured from carrier frequency. Values are tabled for two district carrier frequencies.
\caption/t Phase noise of the used Silicon Laboratories Si570 chip. Offset frequency is measured from carrier frequency. Values shown in the table are given for two different carrier frequencies.
\endinsert
Every ADC module will be directly connected to CLKHUB02A module which takes sampling clock signal delivered by FPGA from main local oscillator. This signal should use high quality differential signaling cable -- we should use SATA cable for this purpose. FPGA may slightly affect clock signal quality by additive noise, but has negligible effect in application where developed system will be used.
Every ADC module will be directly connected to CLKHUB02A module which takes sampling clock signal delivered by FPGA from the main local oscillator. This signal should use high quality differential signalling cable -- we should use SATA cable for this purpose. FPGA may slightly affect the clock signal quality by adding a noise, but it has a negligible effect on the application where developed system will be used.
\secc Signal cable connectors
103,8 → 103,8
* SAS/miniSAS
\enditems
At the end, MiniSAS connector was chosen as the best option to be used in connecting together multiple ADC modules. A transition between SATA and miniSAS is achieved by SAS to SATA adapter cable which is commonly used in servers to connect SAS controller to multiple SATA hard disc in RAID systems and thus is commercially easily available. It is compatible with existing SATA cabling systems and aggregates multiple SATA cables to a single connector, it has SPI configuration lines which can be seen on the following picture \ref[img-miniSAS-cable] as standard pinheader connector.
The main drawback of miniSAS PCB connectors lies in the fact, that they are manufactured in SMT versions only, SMT design may eventually decrease the durability of the connector even if outer metal housing of connector is designed to be mounted using a standard through-hole mounting method.
At the end, MiniSAS connector was chosen as the best option to be used in connecting together multiple ADC modules. A transition between SATA and miniSAS is achieved by SAS to SATA adapter cable which is commonly used in servers to connect SAS controller to multiple SATA hard disc in RAID systems and thus is commercially easily available. It is compatible with existing SATA cabling systems and aggregates multiple SATA cables to a single connector. It also has SPI configuration lines which can be seen in the following picture \ref[img-miniSAS-cable] as standard pinheader connector.
The main drawback of miniSAS PCB connectors lies in the fact, that they are manufactured in SMT versions only. SMT design may eventually decrease the durability of the connector even if outer metal housing of connector is designed to be mounted using a standard through-hole mounting method.
\midinsert
\clabel[img-miniSAS-cable]{Used miniSAS cable}
116,7 → 116,7
\label[diff-signaling]
We use ADC devices that have DATA clock frequency eight times higher than sampling frequency in single line output mode, implying a 40 MHz output bit rate. This imply $ 1/4 \cdot 10^7 = 25\ $ns time length of data bit, which is equivalent to 7.5m light path in free space. If we use copper PCB with FR4 substrate layer or coaxial/twinax cable, we could obtain velocity factor of 0.66 at worst condition. Then the light path for the same bit rate $t_s$ will be 4.95 m. Although we do not have any cables in system with comparable lengths, worst data bit skew described by data sheets of used components is $0.3 \cdot t_s$, which is 1.485 m. Therefore length matching is not critical in our current design operated on lowest sampling speed. Length matching becomes critical in future version with higher sampling rates, then cable length must be matched. However SATA cabling technology is prepared for that case and matched SATA cables are standard merchandise.
We use ADC devices that have DATA clock frequency eight times higher than sampling frequency in a single line output mode, implying a 40 MHz output bit rate. This implies a $ 1/4 \cdot 10^7 = 25\ $ns time length of data bit, which is equivalent to 7.5m light path in free space. If we use copper PCB with FR4 substrate layer or coaxial/twinax cable, we could obtain velocity factor of 0.66 at worst condition. Then the light path for the same bit rate $t_s$ will be 4.95 m. Although we do not have any cables in the system with comparable lengths, the worst data bit skew described by data sheets of the used components is $0.3 \cdot t_s$, which is 1.485 m. Therefore the length matching is not critical in our current design operating on lowest sampling speed. Length matching may become critical in future versions with higher sampling rates, where the cable length must be matched. However SATA cabling technology is already prepared for that case and matched SATA cables are a standard merchandise.
\secc ADC modules design
124,12 → 124,12
\clabel[adcdual-preview]{Preview of designed ADCdual PCB}
\picw=10cm \cinspic ./img/ADCdual01A_Top_Big.JPG
\picw=10cm \cinspic ./img/ADCdual01A_Bottom_Big.JPG
\caption/f Realised PCB of ADCdual01A modules. Differential pairs routing are clearly visible.
\caption/f Realised PCB of ADCdual01A modules. Differential pairs routings are clearly visible.
\endinsert
\secc ADC selection
There exist several standard ADC signaling formats currently used in communication with FPGA.
There exist several standard ADC signalling formats currently used in communication with FPGA.
\begitems
* DDR LVDS
140,9 → 140,9
* serial LVDS
\enditems
Because we need to use the smallest number of cables, the choice fell on the serial LVDS format. Small number of differential pairs is an important parameter determining the construction complexity and reliability\cite[serial-lvds]. No much many currently existing ADC devices have this kind of digital interface. An ultrasound AFE device chips seems to be ideal for this purpose -- the chip has integrated both front-end amplifiers and filters. It has a drawback though - it is incapable of handling differential input signal and has a relatively low dynamic range (as it consists only of 12bit ADC) and has many single ended ADC channels. Consequently scaling is possible only by a factor of 4 receivers (making 8 analogue single ended channels).
As a result of our need to use the smallest number of cables possible, the choice fell on the serial LVDS format. Small number of differential pairs is an important parameter determining the construction complexity and reliability\cite[serial-lvds]. No many currently existing ADC devices have this kind of digital interface. An ultrasound AFE device chips seem to be ideal for this purpose -- the chip has integrated both front-end amplifiers and filters. It has a drawback though - it is incapable of handling differential input signal and has a relatively low dynamic range (as it consists only of 12bit ADC) and has many single ended ADC channels. Consequently, the scaling is possible only by a factor of 4 receivers (making 8 analogue single ended channels).
If we add a requirement of separate output for every analogue channel and a 16bit depth we find that there are only a few 2-Channel simultaneous sampling ADCs currently existing which meet these requirements. We have summarized those ADCs in the following table \ref[ADC-types]
If we add a requirement of separate output for every analogue channel and a 16bit depth we find that there are only a few 2-Channel simultaneous sampling ADCs currently existing which meet these criteria. We have summarized those ADCs in the following table \ref[ADC-types]
\midinsert
\typosize[9/11] \def\tabiteml{ }\let\tabitemr=\tabiteml
156,17 → 156,17
Configuration & \multispan7 SPI \strut \cr
Package & \multispan7 \hfil 52-Lead (7mm $\times$ 8mm) QFN \hfil \strut \cr
}
\caption/t The summary of available ADC types and theirs characteristics.
\caption/t The summary of the currently available ADC types and theirs characteristics.
\endinsert
All parts in this category are compatible with one board layout. Main differences lay in the sampling frequency and signal to noise ratio, with the slowest having a maximum sampling frequency of 20 MHz. However all of them have a minimal sampling frequency of 5 MSPS and all are configurable over a serial interface (SPI). SPI seems to be a standard interface used in high-end ADC chips made by the largest manufacturers (Analog Devices, Linear technology, Texas instruments, Maxim integrated..). We selected two slowest types for our evaluation design. Then PCB for this part have been designed.
We decided that ADCdual01A modules have a standard MLAB construction layout with four mounting holes in corners aligned in defined raster of 400 mils.
All parts in this category are compatible with one board layout. The main differences lay in the sampling frequency and signal to noise ratio, with the slowest having a maximum sampling frequency of 20 MHz. However, all of them have a minimal sampling frequency of 5 MSPS and all are configurable over a serial interface (SPI). SPI seems to be a standard interface used in high-end ADC chips made by the largest manufacturers (Analog Devices, Linear technology, Texas instruments, Maxim integrated..). We have selected two slowest types for our evaluation design. Following that, a PCB for this part have been designed.
We have decided that ADCdual01A modules will have a standard MLAB construction layout with four mounting holes in corners aligned in defined raster of 400 mils.
Data serial data outputs of ADC modules should be connected directly by LVDS signalling levels conducted by SATA cables to FPGAs for the basic primary signal processing. The ADC chips used in the modules has a selectable bit width of data output bus and thus the output SATA connectors have signals arranged to contain a single bit from every ADC channel. This creates a signal concept enabling a selection of a proper bus bit-width according to the sampling rate (higher bus bit-width downgrades signalling speed and vice versa.)
Data serial data outputs of ADC modules should be connected directly by LVDS signalling levels conducted by SATA cables to FPGAs for the basic primary signal processing. The ADC chips used in the modules have a selectable bit width of data output bus and thus the output SATA connectors have signals arranged to contain a single bit from every ADC channel. This creates a signal concept enabling a selection of proper bus bit-width according to the sampling rate (higher bus bit-width downgrades signalling speed and vice versa.)
In order to connect the above mentioned signalling layout, miniSAS to multiple SATA cable should be used as described in section \ref[signal-cables].
A KiCAD design suite had been chosen for PCB layout. However, the version is, despite having integrated CERN Push \& Shove routing capability, slightly unstable as it sometimes crushes due to an exception during routing. On the basis of these stability issues, the design had to be saved quite often. On the other hand, compared to commercially available solutions, such as MentorGraphics PADS or Cadence Orcad, the Open-source KiCAD provides an acceptable option and it easily surpasses a widely used Eagle software.
A KiCAD design suite had been chosen for PCB layout. However, the version, despite having integrated CERN Push \& Shove routing capability, is slightly unstable as it sometimes crushes due to an exception during routing. On the basis of these stability issues, the design had to be saved quite often. On the other hand, compared to commercially available solutions, such as MentorGraphics PADS or Cadence Orcad, the Open-source KiCAD provides an acceptable option and it easily surpasses a widely used Eagle software.
As a part of work on the thesis, new PCB footprints for FMC, SATA, ADCs a and miniSAS connectors have been designed and were committed to KiCAD github library repository. They are now publicly available on the official KiCAD repository at GitHub.
186,7 → 186,7
\caption/f Digital signalling schema for 1-line ADC digital output mode.
\endinsert
ADCdual01A parameters can be set either by jumper setup (referred to as a parallel programming in the device's data sheet) or by SPI interface. SPI interface has been selected for our system, because of the parallel programming lack of options (test pattern output setup for example).
ADCdual01A parameters can be set either by jumper setup (referred to as a parallel programming in the device's data sheet) or by SPI interface. SPI interface has been chosen for our system, because of the parallel programming's lack of options (test pattern output setup for example).
Complete schematic diagram of ADCdual01A module board is included in the appendix.
203,17 → 203,16
This industry standard guarantees the compatibility with other FPGA boards that have FMC LPC connectors for Mezzanine Card. Schematic diagram of designed adapter board is included in the appendix.
The primary purpose of the PCB is to enable the connection of ADC modules located outside the PC case with ML605 development board. (In PC box analog circuits cannot be realized without the use of massive RFI mitigation techniques).
Differential signaling connectors should be used for conducting digital signal over relatively long cables. The signal integrity sensitive links (clocks) are equipped with output driver and translator to LVPECL logic for better signal transmission quality.
Differential signalling connectors should be used for conducting digital signal over relatively long cables. The signal integrity sensitive links (clocks) are equipped with output driver and translator to LVPECL logic for better signal transmission quality.
LVPECL level signal connectors on FMC2DIFF01A board are dedicated for clock signals. We selected the SY55855V and SY55857L dual translators. Dual configuration in useful due to fact that SATA cable contains two differential pairs.
LVPECL level signal connectors on FMC2DIFF01A board are dedicated to transmit the clock signals. We have selected the SY55855V and SY55857L dual translators. Dual configuration in useful due to fact, that SATA cable contains two differential pairs.
The SY55855V is a fully differential, CML/PECL/LVPECL-to-LVDS translator. It achieves LVDS signaling up to 1.5Gbps, depending on the distance and the characteristics of the media and noise coupling sources.
LVDS is intended to drive 50 $\Omega$ impedance transmission
line media such as PCB traces, backplanes, or cables. SY55855V inputs can be terminated with a single resistor between the true and the complement pins of a given input \cite[SY55855V-chip].
The SY55855V is a fully differential, CML/PECL/LVPECL-to-LVDS translator. It achieves LVDS signalling up to 1.5Gbps, depending on the distance and the characteristics of the media and noise coupling sources.
LVDS is intended to drive 50 $\Omega$ impedance transmission line media such as PCB traces, backplanes, or cables. SY55855V inputs can be terminated with a single resistor between the true and the complement pins of a given input \cite[SY55855V-chip].
The SY55857L is a fully differential, high-speed dual translator optimized to accept any logic standard from single-ended TTL/CMOS to differential LVDS, HSTL, or CML and translate it to LVPECL. Translation is guaranteed for speeds up to 2.5Gbps (2.5GHz toggle frequency). The SY55857L does not internally terminate its inputs, as different interfacing standards have different termination requirements\cite[SY55857L-chip].
Inputs of both used chips are terminated accordingly to used logic. The LVDS input is terminated differentially by 100 $\Omega$ resistor between positive and negative inputs. PECL input is terminated by Thevenin resistor network. Thevenin termination method was selected as optimal due to absence of proper power voltage (1,3 V) for direct termination by 50 $\Omega$ resistors. Termination on FPGA side is realized directly by settings proper digital logic type on input pins.
Inputs of both used chips are terminated accordingly to used logic. The LVDS input is terminated differentially by 100 $\Omega$ resistor between positive and negative inputs. PECL input is terminated by Thevenin resistor network. Thevenin termination method was selected as optimal one, due to the absence of a proper power voltage (1,3 V) for direct termination by 50 $\Omega$ resistors. Termination on FPGA side is realized directly by settings the proper digital logic type on input pins.
\midinsert
\clabel[ML605-development-board]{ML605 development board}