High (?) Frequency Receivers. High (?) Frequency Rxs.

Slides:



Advertisements
Similar presentations
Noise Lecture 6.
Advertisements

Receiver Systems Alex Dunning.
WP-M3 Superconducting Materials PArametric COnverter Detector INFN_Genoa Renzo Parodi.
Optical sources Lecture 5.
Principles & Applications Communications Receivers
Second Sound in Superfluid Helium. Superfluids “Superfluid” describes a phase of matter. In this phase, a liquid has no viscosity and may exhibit several.
Spectrum analyser basics Spectrum analyser basics 1.
Heat Section 1 © Houghton Mifflin Harcourt Publishing Company Preview Section 1 Temperature and Thermal EquilibriumTemperature and Thermal Equilibrium.
Fiber-Optic Communications
Fiber-Optic Communications
Microwave Spectroscopy I
Radio Telescopes. Jansky’s Telescope Karl Jansky built a radio antenna in –Polarized array –Study lightning noise Detected noise that shifted 4.
Heat and Energy Energy is the ability to do work. Work is done when a force causes an object to move in the direction of the force. Work is a transfer.
COMMUNICATION SYSTEM EECB353 Chapter 2 Part IV AMPLITUDE MODULATION Dept of Electrical Engineering Universiti Tenaga Nasional.
Receiver Systems Suzy Jackson – based on previous talks by Alex Dunning & Graeme Carrad.
Fiber Optic Receiver A fiber optic receiver is an electro-optic device that accepts optical signals from an optical fiber and converts them into electrical.
ELCT564 Spring /17/20151ELCT564 Diodes, Transistors and Mixers.
Phase noise measurements in TRIUMF ISAC 2 cryomodule K. Fong, M. Laverty TRIUMF.
Microwave Engineering/Active Microwave Devices 9-13 September Semiconductor Microwave Devices Major Applications Substrate Material Frequency Limitation.
ENERGY.
4/11/2006BAE Application of photodiodes A brief overview.
Energy, Heat and Heat Transfer
Current and Direct Current Circuits
18/7/2002Ivan Hruska EP/ATE1 LV brick for TILECAL  How to power the electronics of TILECAL ? Power supply as close as possible to electronics ?  Positives.
1 1 Temperature and Thermal Energy Temperature and energy Glencoe: Chapter 9 – Section 1: pages
Thermal Energy and Matter Chapter 16. Heat Heat is the transfer of thermal energy from one object to another due to a temperature difference – Flows from.
Electro-Magnetic Radiation
What ARE all those little things anyway?
3/26/2003BAE of 10 Application of photodiodes A brief overview.
temperature heat conduction radiation Particles in Motion convection vaporization thermal conductor thermal insulator.
Heat and States of Matter
THERMAL Energy Chapter 5.
Amplitude Modulation 2.2 AM RECEIVERS
Proposed Versatile 1.2 to 14 GHz Radio Telescope Receiver S. Weinreb, JPL/Caltech, Draft July 5, 2005 Contents 1.Introduction and intended applications.
< BackNext >PreviewMain Section 1 Temperature What Is Temperature? Temperature is a measure of the average kinetic energy of the particles in an object.
HEAT & THERMAL ENERGY CH. 16. State indicator 17. Demonstrate that thermal energy can be transferred by conduction, convection or radiation (e.g., through.
CHAPTER 2 Amplitude Modulation 2-3 AM RECEIVERS. Introduction AM demodulation – reverse process of AM modulation. Demodulator: converts a received modulated-
AST 443: Submm & Radio Astronomy November 18, 2003.
Travelling Wave Tube For Broadband amplifier helix TWTs (proposed by Pierce and others in 1946 ) are widely used For High average power purposes the.
Temperature and Heat 4.1 Temperature depends on particle movement. 4.2
Temperature and Heat CHAPTER the BIG idea CHAPTER OUTLINE Heat is a flow of energy due to temperature differences. Temperature depends on particle movement.
Section 1 Temperature. Describe how temperature relates to kinetic energy. Compare temperatures on different temperature scales. Give examples of thermal.
1 Microwave Semiconductor Devices Major Applications Substrate Material Frequency Limitation Device Transmitters AmplifiersSi, GaAs, InP< 300 GHzIMPATT.
CHAPTER 2 Amplitude Modulation 2-3 AM RECEIVERS. Introduction AM demodulation – reverse process of AM modulation. Demodulator: converts a received modulated-
Thoughts on the Design of a WVR for Alan Roy (MPIfR) the Twin Telescope at Wettzell.
Modulators and Semiconductors ERIC MITCHELL. Acousto-Optic Modulators Based on the diffraction of light though means of sound waves travelling though.
 What is temperature??  The degree of hotness or coldness of a body or environment.  A measure of the warmth or coldness of an object or substance.
AM RECEPTION Introduction
ECE 4710: Lecture #37 1 Link Budget Analysis  BER baseband performance determined by signal to noise ratio ( S / N ) at input to detector (product, envelope,
What is Heat?. Why did you put a jacket on this morning? What is cold? What is hot? Why are faucets labeled “H” and “C”? When you first turn on the “hot”
UCLA IEEE NATCAR 2004 SUMMER CLASS Magnetic Sensors & Power Regulation.
Heat Section 1 Preview Section 1 Temperature and Thermal EquilibriumTemperature and Thermal Equilibrium Section 2 Defining HeatDefining Heat Section 3.
Heat and Heat Technology Section 2 – What is Heat? pp
Thermal Energy. Warm Up: To shape metal into a horseshoe, the metal is heated in a fire. Why will a horseshoe bend when it’s very hot, but not after it.
@earthscience92. What is Energy? Energy – Is the ability to cause change – Many forms of energy – Two general forms of energy are Kinetic energy Potential.
Temperature and Heat CHAPTER the BIG idea CHAPTER OUTLINE Heat is a flow of energy due to temperature differences. Temperature depends on particle movement.
What is the kinetic molecular theory? In what three ways is thermal energy transferred? How are thermal conductors and insulators different? Particles.
Standards 3: Thermal Energy How Heat Moves  How heat energy transfers through solid.  By direct contact from HOT objects to COLD objects.
Energy in Earth Processes Unit 4. What is Energy? Energy is _____________________________ Everything that is done in the universe involves the _______________________________.
* Materials that allow heat, electricity, or sound waves to pass through them.
P RESENTATION ON MONOLITHIC MICROWAVE INTEGRATED CIRCUITS PASSIVE COMPONENTS SUBMITTED BY:- AJAY KAUSHIK(088/ECE/09 ) NAMAN KUMAR(082/ECE/09 )
Thermal Energy Transfer
Current and future ground-based gravitational-wave detectors
Receiver Systems Signal Processing.
Noise Figure Measurement using Natural Noise Sources
Thermal Energy and Heat
An X-band system for phase space linearisation on CLARA
PIN DIODE.
Transfer of Thermal Energy
Thermal energy Chapter 4.
Presentation transcript:

High (?) Frequency Receivers

High (?) Frequency Rxs

……covering What is high frequency? Receivers Why would you want one? What’s it look like? Where’s it go? Why are they like they are? Examples

20/13 cm Band 6/3 cm Band 12/3 mm Bands Australia Telescope Compact Array Receiver Bands Thanks to Russell Gough for the slide

Receiver : Do we really need one?

….because our senses can’t detect radio waves and the receiver system takes the unguided wave and transforms it into a guided wave that can be detected so as to provide data that can be studied.

What does a receiver look like? A quick primer to avoid confusion

Radiotelescope receiverReceiver of presents

Wide radiotelescope receiverWide receiver

Radiotelescope receiver Receiver in bankruptcy firm

Radiotelescope receiver Receiver of stolen goods

Where do these things go?

In a prime focus system like Parkes ……

It goes in here

In a Cassegrain system like Narrabri or Mopra……

It goes in here

Charged particles change their state of motion when they interact with energy What is the signal like? A change in state of motion gives rise to an EM wave Matter is made of huge numbers of charged particles receiving energy being jostled and the radiation consists of unrelated waves at all frequencies and by analogy with the acoustic case it is called NOISE. There is a general background and areas of enhanced radiation and energy

…….but it’s bloody weak If Parkes, for its 40 years of operation, had operated non-stop observing 100 Jy sources (that’s big) in a 1 GHz bandwidth (that’s big too) the total energy collected would light a 60 watt light globe for a mere 67 milliseconds

Is there a typical structure to them?

feed Signal in f signal

feed Signal in f signal Noise source Coupler to main signal path

OMT f signal To get both polarisation components (polariser) feed f signal Noise source Signal in

amplifier f signal OMT (polariser) feed f signal Noise source Signal in

amplifiermixer f signal f signal- f lo OMT (polariser) ….to get the signal to a lower frequency where more established (cheaper) backend components and processing electronics handle the signal feed f signal Noise source Signal in (LO) Local Oscillator Phase locked

D f (1.5 GHz) freq D f f lo f signal (100 GHz)(98.5 GHz) freq amplitude cosAcosB=1/2 {cos(A-B) + cos(A+B)}

D f (1.5 GHz) freq D f f lo f signal (97 GHz)(98.5 GHz) freq amplitude USBLSB

amplifiermixer LO OMT (polariser) feed f signal Noise source Signal in To other conversions Side band rejection

….so I am saying that this is a pretty typical structure of our receivers ………………….and the 3/12 mm systems reflect this

OMT amplifier Signal line to mixer Feed sits up top here Noise coupler 12mm components

oscillator mixers LO split Phase lock electronics 3mm LO system

………so what is all the other crap for? Some of these receiver components are pretty small……. …….we have seen the receivers are quite sizeable…..

Apart from the complex support and monitor electronics…. ……………………..we need to consider sensitivity to explain.

To measure the radiation we observe it for an interval long compared to most of the fluctuations and find the mean average power over the interval. Each observation will fluctuate about the true mean and this limits the sensitivity. A rough estimate of the size of the fluctuations: Random fluctuating quantity restricted to bandwidth D f is equivalent to a sequence of D f independent values in 1 sec. Averaging a sequence over t seconds means t * D f values Fluctuations in the mean of n independent readings ~ n -1/2 so our mean power fluctuations will be D P/P ~ ( t * D f) -1/2

D P ~ P ( t * D f) 1/2 …but the components in the signal path contribute to P because they are matter with thermal energy. So the components’ contribution masks the signal. It is like trying to measure the change in water level of a swimming pool when dropping a child in during free-for-all time at a swimming carnival To reduce their masking effect we reduce their thermal energy by cooling them! The following demonstration displays this. or P = Psig + Prec

Reduce noise by cooling Electronic device generates a signal Cold stuff (liquid nitrogen)

So we need way cool gear to get some cooling and keep things cold *Refrigerator and compressor (He as working fluid) *Keep heat transfer from the outside minimal *Watch out for the axis of evil in conduction, convection and radiation

compressor Fridge gas lines Rad shield Stainless steel dewar Insulating material

There is a good reason for the structure….. Nyquist came up with the theorem which relates noise power to the temperature (T) of a matched resistor which would produce the same effect through Pn = k T D f So a device or system is assigned a noise temperature by considering the device or system noise free and seeing what temperature resistor at its input would produce the same noise output For example we talk of our receivers having a noise temperature of 20 K which more correctly should be stated that the receiver behaves as a matched resistor at an absolute temperature of 20 Kelvin

Further for systems in cascade it can be shown Teq = T1 + T2 + T3 + ……. Gain1 Gain1*Gain2 This highlights the desire for cooling and for low loss, low noise, high gain components at the front of a system. amplifiermixer Local oscillator OMT feed f signal

The active components currently used in most millimetre, radioastronomy receivers are superconductor-insulator- superconductor (SIS) mixers and discrete Gallium Arsenide (GaAs) or Indium Phosphide (InP) transistors. The monolithic microwave integrated circuits (MMICs) we have developed can replace all the discrete components of an amplifier with a single chip which can be mass produced allowing cost savings and greater reproducibility and reliability. Indium Phosphide technology has become the first choice of our millimetre devices because of its lower noise, higher frequency response and superior cryogenic performance What’s special about these higher frequency receivers is………..

……….the Mopra mm receiver is different as are others…… After all I said before…….amplifiermixer Local OMT (polariser) oscillator Signal in feed f signal feed

Historically, when amplifers aren’t available –whack in a mixer anyway and do some science. This is currently true for receivers operating above 100 GHz. The Mopra receiver has low noise SIS (superconductor-insulator- superconductor) mixers as opposed to the more conventional diodes. They require an extra cooling section to maintain them at 4K They are followed up by cooled, low noise, high gain amplifiers They are not broadband so some tuning is necessary across the band Many have Guassian beam optics for signal acquisition and LO injection

The polarisation splitter is not a waveguide structure but rather a set of grids crossing at right angles and having closely spaced wires – each grid having wires running orthogonally to the other It is incorporated in a Guassian beam optics path that was necessary because the feed, internal to the dewar, was unable to be positioned at the focus.

Optics box grids