+ All Categories
Home > Documents > DBBC - EVN CDR Meeting, Bologna May 2005 DBBC Project G. Tuccari, S. Buttaccio, G. Nicotra -...

DBBC - EVN CDR Meeting, Bologna May 2005 DBBC Project G. Tuccari, S. Buttaccio, G. Nicotra -...

Date post: 31-Dec-2015
Category:
Upload: michael-cook
View: 215 times
Download: 1 times
Share this document with a friend
Popular Tags:
23
DBBC - EVN CDR Meeting, Bologn a May 2005 DBBC Project G. Tuccari, S. Buttaccio, G. Nicotra - Istituto di Radioastronomia CNR, Sezione di Noto - Italy M. Wunderlich - Max Planck Institute fuer Radioastronomie, Bonn - Germany Y. Xiang - Shanghai Astronomical Observatory, CAS – China G. Balodis - Faculty of Electronics and Telecommunications, University of Riga - Latvia
Transcript
Page 1: DBBC - EVN CDR Meeting, Bologna May 2005 DBBC Project G. Tuccari, S. Buttaccio, G. Nicotra - Istituto di Radioastronomia CNR, Sezione di Noto - Italy M.

DBBC - EVN CDR Meeting, Bologna May 2005

DBBC Project

G. Tuccari, S. Buttaccio, G. Nicotra - Istituto di Radioastronomia CNR, Sezione di Noto - Italy

M. Wunderlich - Max Planck Institute fuer Radioastronomie, Bonn - Germany

Y. Xiang - Shanghai Astronomical Observatory, CAS – China

G. Balodis - Faculty of Electronics and Telecommunications, University of Riga - Latvia

Page 2: DBBC - EVN CDR Meeting, Bologna May 2005 DBBC Project G. Tuccari, S. Buttaccio, G. Nicotra - Istituto di Radioastronomia CNR, Sezione di Noto - Italy M.

DBBC - EVN CDR Meeting, Bologna May 2005

DBBC Project overview

• The main goal is to replace the existing terminal with a complete compact system to be used with any VSI compliant recorder or data transport

• Hardware programmability is the main feature in order to optimize the architecture to the needed performance having the possibility to arrange different architecture in the same hardware support

• Maximum Input and Output data rates are the limitation and are set so to satisfy the present and near future necessities

• The new development is compatible with the existing terminals and correlators

Page 3: DBBC - EVN CDR Meeting, Bologna May 2005 DBBC Project G. Tuccari, S. Buttaccio, G. Nicotra - Istituto di Radioastronomia CNR, Sezione di Noto - Italy M.

DBBC - EVN CDR Meeting, Bologna May 2005

DBBC Project overview (cont.)

•The new set of BBCs is fully up-gradable and ready to process in a future larger bandwidth with modified correlators

•Upgrade or improvements will be mostly only software

• Upgrade is also possible in hardware replacing compatible ‘pin-to-pin’ processing modules

• Data out as VSI interface and modified MK4 formatter

Page 4: DBBC - EVN CDR Meeting, Bologna May 2005 DBBC Project G. Tuccari, S. Buttaccio, G. Nicotra - Istituto di Radioastronomia CNR, Sezione di Noto - Italy M.

DBBC - EVN CDR Meeting, Bologna May 2005

DBBC General Features

• Four IF Input in the range 1-512 , 512-1024, 1024-1536, 1536-2048 MHz

• Four polarizations or bands available for a single group of output data channel selection

• 230=1.073.741.824 Hz frequency sampling clock

• Channel bandwidth ranging between 250KHz to 32 MHz

• Tuning step 1 Hz or less if required

• Station based fringe counter-rotation possible

• Multiple architecture using fully re-configurable FPGA Core Modules

• Modular realization for cascaded processing

Page 5: DBBC - EVN CDR Meeting, Bologna May 2005 DBBC Project G. Tuccari, S. Buttaccio, G. Nicotra - Istituto di Radioastronomia CNR, Sezione di Noto - Italy M.

DBBC - EVN CDR Meeting, Bologna May 2005

DBBC General Schematic View

A/D 1

cPCILinux PC

FS PC

1074 MHz Synthesizer Distributor

H-Maser

MK4/VSImax64 ch

CORE

HSI

HSO

cPCIInterfaces

IFn (MHz)1~512, 512~1024,1024~1536, 1536~2048

AGC/Filter

IF 4IF 3IF 2IF 1

A/D 2 A/D 1 A/D 2 HSIR

HSOR

CORE

HSI

HSO

HSIR

HSOR

AGC/Filter

AGC/Filter

AGC/Filter

CORE

HSI

HSO

HSIR

HSOR Collector

D/AMonitor

Page 6: DBBC - EVN CDR Meeting, Bologna May 2005 DBBC Project G. Tuccari, S. Buttaccio, G. Nicotra - Istituto di Radioastronomia CNR, Sezione di Noto - Italy M.

DBBC - EVN CDR Meeting, Bologna May 2005

Schematic Top View6U x 84 TE x 360 mm

A/D

min 1- max 4

(4 for a VLBA equivalent system)

CoreModule

min 1 – max 16

(8 for a VLBA equivalent system)

VSI

MK4

Analog

IF1 IF2 IF3 IF410 MHz 1 PPS

FsIF1 IF2 IF3 IF4

cPCI

Linux PC and Interfaces

FiLa FiLa

Ethernet

D

I

S

K

1 PPS

Fs/2

Fs/4

JTAG

1.5VVcore

3.3VDig

3.3VVAux

3.3VAn

1.5VVcore

5V 12V

Page 7: DBBC - EVN CDR Meeting, Bologna May 2005 DBBC Project G. Tuccari, S. Buttaccio, G. Nicotra - Istituto di Radioastronomia CNR, Sezione di Noto - Italy M.

DBBC - EVN CDR Meeting, Bologna May 2005

System Components

• Analog to digital converter ‘environment’• 1074 MHz Synthesizer (commercial)• CoreModule boards• FPGAs Core Firmware Configurations• DA monitor• FiLa board (data insertion and collector)• VSI interface• PCI interfaces (commercial)• Linux PC Board (commercial)• System Management Software + Field System

Integration

Page 8: DBBC - EVN CDR Meeting, Bologna May 2005 DBBC Project G. Tuccari, S. Buttaccio, G. Nicotra - Istituto di Radioastronomia CNR, Sezione di Noto - Italy M.

DBBC - EVN CDR Meeting, Bologna May 2005

Analog to digital converter ‘environment’

• Conversion Clock Fs=1.073.741.824 Hz or Fs/2, Fs/4, Fs/8

• MAX108 AD converter (under evaluation ATMEL AT84AS003)

• Front-end power level control

• Bandwidth 1-512 / 512-1024 / 1024-1536 / 1536-2048 MHz selection/filtering

• Total power measurement

• LVPECL differential data bus (ATMEL: LVDS)

Page 9: DBBC - EVN CDR Meeting, Bologna May 2005 DBBC Project G. Tuccari, S. Buttaccio, G. Nicotra - Istituto di Radioastronomia CNR, Sezione di Noto - Italy M.

DBBC - EVN CDR Meeting, Bologna May 2005

A/D Board Schematic View

ADCONVERTER

RX IF2X8bit Data

LVPECL differential

Power Level

ControlAnti-image

AnalogFilter

TotalPower

Interface

1PPS

H-Maser1074 MHz Synthesizer

Band Reduction

Page 10: DBBC - EVN CDR Meeting, Bologna May 2005 DBBC Project G. Tuccari, S. Buttaccio, G. Nicotra - Istituto di Radioastronomia CNR, Sezione di Noto - Italy M.

DBBC - EVN CDR Meeting, Bologna May 2005

AD Board Layout

Page 11: DBBC - EVN CDR Meeting, Bologna May 2005 DBBC Project G. Tuccari, S. Buttaccio, G. Nicotra - Istituto di Radioastronomia CNR, Sezione di Noto - Italy M.

DBBC - EVN CDR Meeting, Bologna May 2005

DBBC CoreModule

• A single module able to process more channels

• More modules can be arranged in cascade

• External buses: HIS/HSIR, HSO/HSOR, CCM/CCMR

• HSI Input data bus, is propagated with HSIR

• HSO Output data bus, is shared for multiple IF access

• CCM/R Control/Configuration/Monitor bus

Page 12: DBBC - EVN CDR Meeting, Bologna May 2005 DBBC Project G. Tuccari, S. Buttaccio, G. Nicotra - Istituto di Radioastronomia CNR, Sezione di Noto - Italy M.

DBBC - EVN CDR Meeting, Bologna May 2005

DBBC Core Modules Cascade Architecture

HSI | HSIR

CORE CORE

HSO

CORE

HSORHSO HSOR HSO HSOR

CORE

HSO HSOR

Stream IF 1-2-3-4

To Collector and VSI interface

HSI | HSIR HSI | HSIR HSI | HSIR

Page 13: DBBC - EVN CDR Meeting, Bologna May 2005 DBBC Project G. Tuccari, S. Buttaccio, G. Nicotra - Istituto di Radioastronomia CNR, Sezione di Noto - Italy M.

DBBC - EVN CDR Meeting, Bologna May 2005

DBBC CORE Module Features

• Different configuration can be supported:

SSB down converter

Wide band parallel FIR

Polyphase FIR + FFT

• A module able to handle:

Maximum Input bandwidth 8.192 Gbit/s

Maximum Output bandwidth 4.096 Gbit/s

Control/Configuration bus through a common PCI interface

Page 14: DBBC - EVN CDR Meeting, Bologna May 2005 DBBC Project G. Tuccari, S. Buttaccio, G. Nicotra - Istituto di Radioastronomia CNR, Sezione di Noto - Italy M.

DBBC - EVN CDR Meeting, Bologna May 2005

Core Module Board

• HIS/HSIR Cascade-able Input Bus 4x2x8bit @512 MHz equivalent

• HSO Shared Output bus 2x32bit @32, 64MHz

• CCM Control / Configuration bus 32bit

• CCM Monitor bus to DA converter 12 bit @32,64 MHz

• 1 FPGA VirII-1152pin, 3000 - 4000 - 6000 – 8000

(to be evaluated Xilinx V4 device)

• ‘Sandwich’ cascade method

Page 15: DBBC - EVN CDR Meeting, Bologna May 2005 DBBC Project G. Tuccari, S. Buttaccio, G. Nicotra - Istituto di Radioastronomia CNR, Sezione di Noto - Italy M.

DBBC - EVN CDR Meeting, Bologna May 2005

CoreModule Layout

Page 16: DBBC - EVN CDR Meeting, Bologna May 2005 DBBC Project G. Tuccari, S. Buttaccio, G. Nicotra - Istituto di Radioastronomia CNR, Sezione di Noto - Italy M.

DBBC - EVN CDR Meeting, Bologna May 2005

Digital Down Converter Configuration

• SSB conversion between high data rate sampled IF band and lower data rate base band

• LO as a Numerically Controlled Oscillator

• Mixer as Complex as Look Up Table multiplier

• Low-pass band filter Finite Impulse Response (FIR) filters cascade

• Decimation because of the high ratio between IF and output data rate performed with CIC or multirate/multistage FIR

• Bandwidth: 16, 8, 4, 2, 1, 0.5, 0.25 MHz

Page 17: DBBC - EVN CDR Meeting, Bologna May 2005 DBBC Project G. Tuccari, S. Buttaccio, G. Nicotra - Istituto di Radioastronomia CNR, Sezione di Noto - Italy M.

DBBC - EVN CDR Meeting, Bologna May 2005

Linux PC Board: System Management Software

• Standard commercial PC board including HD

• Configuration files for each FPGA stored on HD

• Software interface for FPGA configuration

• Software interface for servicing FPGAs (I/O registers access)

• Software interface for A/D level control

Page 18: DBBC - EVN CDR Meeting, Bologna May 2005 DBBC Project G. Tuccari, S. Buttaccio, G. Nicotra - Istituto di Radioastronomia CNR, Sezione di Noto - Italy M.

DBBC - EVN CDR Meeting, Bologna May 2005

Software Management Structure

FieldSystem

PC

cPCIPC+

INT

FPGAModule FPGA

Module

FPGAModule

HD

Ethernet

AD

AD

Page 19: DBBC - EVN CDR Meeting, Bologna May 2005 DBBC Project G. Tuccari, S. Buttaccio, G. Nicotra - Istituto di Radioastronomia CNR, Sezione di Noto - Italy M.

DBBC - EVN CDR Meeting, Bologna May 2005

DBBC Prototype Status at April 2005

• AD Environment:- Conditioning modules developed (IRA)

- AD Board developed, to be realized (MPI)• CoreModule:

- Board developed, to be realized (IRA)- FPGA firmware configurations (IRA+SHAO):

– 0.5, 1, 2, 4 MHz bwd, completed, – 0.25, 8, 16 MHz bwd, near to completion, to be tested – 0.125, 0.0625, 0.03125, 32 MHz ready in simulation– tunable base band with 1 Hz resolution– tuning range in Nyquist blocks of 64 and 128 MHz ready– tuning range in Nyquist blocks of 256, 512 MHz ready in

simulation, under development

Page 20: DBBC - EVN CDR Meeting, Bologna May 2005 DBBC Project G. Tuccari, S. Buttaccio, G. Nicotra - Istituto di Radioastronomia CNR, Sezione di Noto - Italy M.

DBBC - EVN CDR Meeting, Bologna May 2005

DBBC Prototype Status at April 2005 (cont)

• Insertion/Collector board: developed, to be realized (IRA)• Monitor: to be realized (IRA)• Synthesizer: commercial + ad hoc: developed, to be realized• 1.5V high current power supply ready (IRA)• cPCI under Linux PC: commercial• cPCI interfaces: commercial• Communication software: partially done (SHAO)

Page 21: DBBC - EVN CDR Meeting, Bologna May 2005 DBBC Project G. Tuccari, S. Buttaccio, G. Nicotra - Istituto di Radioastronomia CNR, Sezione di Noto - Italy M.

DBBC - EVN CDR Meeting, Bologna May 2005

DBBC Prototype Performance (Apr 2005)

• Preliminary testing has been done in laboratory for the developed configurations

• Good performance in conversion and tuning have been measured from 0 up to 2.5 GHz

• Today with appropriate Nyquist zone pre-selection, L and S band can be directly down-converted and recorded with modified MK4 formatter (Noto and Seshan)

• Testing with real observation started with mDBBC (IRA-SHAO agreement): fringes detected in analog-digital and digital-digital baselines.

Page 22: DBBC - EVN CDR Meeting, Bologna May 2005 DBBC Project G. Tuccari, S. Buttaccio, G. Nicotra - Istituto di Radioastronomia CNR, Sezione di Noto - Italy M.

DBBC - EVN CDR Meeting, Bologna May 2005

First Results with the mDBBC prototype(collaboration Italy-China)

• First digital x analog fringes detected on Nov 23, 2004 in the Seshan-Urumuqi baseline

• First digital x digital fringes detected on Feb 2, 2005

in the Noto-Seshan baseline

Page 23: DBBC - EVN CDR Meeting, Bologna May 2005 DBBC Project G. Tuccari, S. Buttaccio, G. Nicotra - Istituto di Radioastronomia CNR, Sezione di Noto - Italy M.

DBBC - EVN CDR Meeting, Bologna May 2005

Conclusions• The DBBC system is an high flexible instrument because

is able to produce independent tunable channels for a full compatibility with the existing acquisition system and correlators. One CoreModule board is replacing a BBC module.

• The DBBC system is able to handle polyphase + FFT architectures for producing contiguous not tunable channels. One CoreModule board is able to produce multiple channels.

• Both solutions are possible within the same system adopting a variable number of AD and CoreModule units


Recommended