MT-048: Op Amp Noise Relationships
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Measurement of In-Band Optical Noise Spectral Density 1
Measurement of In-Band Optical Noise Spectral Density 1 Measurement of In-Band Optical Noise Spectral Density Sylvain Almonacil, Matteo Lonardi, Philippe Jennevé and Nicolas Dubreuil We present a method to measure the spectral density of in-band optical transmission impairments without coherent electrical reception and digital signal processing at the receiver. We determine the method’s accuracy by numerical simulations and show experimentally its feasibility, including the measure of in-band nonlinear distortions power densities. I. INTRODUCTION UBIQUITUS and accurate measurement of the noise power, and its spectral characteristics, as well as the determination and quantification of the different noise sources are required to design future dynamic, low-margin, and intelligent optical networks, especially in open cable design, where the optical line must be intrinsically characterized. In optical communications, performance is degraded by a plurality of impairments, such as the amplified spontaneous emission (ASE) due to Erbium doped-fiber amplifiers (EDFAs), the transmitter-receiver (TX-RX) imperfection noise, and the power-dependent Kerr-induced nonlinear impairments (NLI) [1]. Optical spectrum-based measurement techniques are routinely used to measure the out-of-band optical signal-to-noise ratio (OSNR) [2]. However, they fail in providing a correct assessment of the signal-to-noise ratio (SNR) and in-band noise statistical properties. Whereas the ASE noise is uniformly distributed in the whole EDFA spectral band, TX-RX noise and NLI mainly occur within the signal band [3]. Once the latter impairments dominate, optical spectrum-based OSNR monitoring fails to predict the system performance [4]. Lately, the scientific community has significantly worked on assessing the noise spectral characteristics and their impact on the SNR, trying to exploit the information in the digital domain by digital signal processing (DSP) or machine learning. -
Receiver Sensitivity and Equivalent Noise Bandwidth Receiver Sensitivity and Equivalent Noise Bandwidth
11/08/2016 Receiver Sensitivity and Equivalent Noise Bandwidth Receiver Sensitivity and Equivalent Noise Bandwidth Parent Category: 2014 HFE By Dennis Layne Introduction Receivers often contain narrow bandpass hardware filters as well as narrow lowpass filters implemented in digital signal processing (DSP). The equivalent noise bandwidth (ENBW) is a way to understand the noise floor that is present in these filters. To predict the sensitivity of a receiver design it is critical to understand noise including ENBW. This paper will cover each of the building block characteristics used to calculate receiver sensitivity and then put them together to make the calculation. Receiver Sensitivity Receiver sensitivity is a measure of the ability of a receiver to demodulate and get information from a weak signal. We quantify sensitivity as the lowest signal power level from which we can get useful information. In an Analog FM system the standard figure of merit for usable information is SINAD, a ratio of demodulated audio signal to noise. In digital systems receive signal quality is measured by calculating the ratio of bits received that are wrong to the total number of bits received. This is called Bit Error Rate (BER). Most Land Mobile radio systems use one of these figures of merit to quantify sensitivity. To measure sensitivity, we apply a desired signal and reduce the signal power until the quality threshold is met. SINAD SINAD is a term used for the Signal to Noise and Distortion ratio and is a type of audio signal to noise ratio. In an analog FM system, demodulated audio signal to noise ratio is an indication of RF signal quality. -
Fundamental Sensitivity Limit Imposed by Dark 1/F Noise in the Low Optical Signal Detection Regime
Fundamental sensitivity limit imposed by dark 1/f noise in the low optical signal detection regime Emily J. McDowell1, Jian Ren2, and Changhuei Yang1,2 1Department of Bioengineering, 2Department of Electrical Engineering, Mail Code 136-93,California Institute of Technology, Pasadena, CA, 91125 [email protected] Abstract: The impact of dark 1/f noise on fundamental signal sensitivity in direct low optical signal detection is an understudied issue. In this theoretical manuscript, we study the limitations of an idealized detector with a combination of white noise and 1/f noise, operating in detector dark noise limited mode. In contrast to white noise limited detection schemes, for which there is no fundamental minimum signal sensitivity limit, we find that the 1/f noise characteristics, including the noise exponent factor and the relative amplitudes of white and 1/f noise, set a fundamental limit on the minimum signal that such a detector can detect. © 2008 Optical Society of America OCIS codes: (230.5160) Photodetectors; (040.3780) Low light level References and links 1. S. O. Flyckt and C. Marmonier, Photomultiplier tubes: Principles and applications (Photonis, 2002). 2. M. C. Teich, K. Matsuo, and B. E. A. Saleh, "Excess noise factors for conventional and superlattice avalanche photodiodes and photomultiplier tubes," IEEE J. Quantum Electron. 22, 1184-1193 (1986). 3. E. J. McDowell, X. Cui, Y. Yaqoob, and C. Yang, "A generalized noise variance analysis model and its application to the characterization of 1/f noise," Opt. Express 15, (2007). 4. P. Dutta and P. M. Horn, "Low-frequency fluctuations in solids - 1/f noise," Rev. -
Johnson Noise Thermometry Measurement of the Boltzmann Constant with a 200 Ω Sense Resistor Alessio Pollarolo, Taehee Jeong, Samuel P
1512 IEEE TRANSACTIONS ON INSTRUMENTATION AND MEASUREMENT, VOL. 62, NO. 6, JUNE 2013 Johnson Noise Thermometry Measurement of the Boltzmann Constant With a 200 Ω Sense Resistor Alessio Pollarolo, Taehee Jeong, Samuel P. Benz, Senior Member, IEEE, and Horst Rogalla, Member, IEEE Abstract—In 2010, the National Institute of Standards and Technology measured the Boltzmann constant k with an electronic technique that measured the Johnson noise of a 100 Ω resistor at the triple point of water and used a voltage waveform synthesized with a quantized voltage noise source (QVNS) as a reference. In this paper, we present measurements of k using a 200 Ω sense re- sistor and an appropriately modified QVNS circuit and waveform. Preliminary results show agreement with the previous value within the statistical uncertainty. An analysis is presented, where the largest source of uncertainty is identified, which is the frequency dependence in the constant term a0 of the two-parameter fit. Index Terms—Boltzmann equation, Josephson junction, mea- surement units, noise measurement, standards, temperature. Fig. 1. Schematic diagram of the Johnson-noise two-channel cross-correlator. I. INTRODUCTION HE Johnson–Nyquist equation (1) defines the thermal measurement electronics are calibrated by using a pseudonoise T noise power (Johnson noise) V 2 of a resistor in a voltage waveform synthesized with the quantized voltage noise bandwidth Δf through its resistance R and its thermodynamic source (QVNS) that acts as a spectral-density reference [8], [9]. temperature T [1], [2]: Fig. 1 shows the experimental schematic. The two chan- nels of the cross-correlator simultaneously amplify, filter, and 2 VR =4kTRΔf. -
Quantum Noise and Quantum Measurement
Quantum noise and quantum measurement Aashish A. Clerk Department of Physics, McGill University, Montreal, Quebec, Canada H3A 2T8 1 Contents 1 Introduction 1 2 Quantum noise spectral densities: some essential features 2 2.1 Classical noise basics 2 2.2 Quantum noise spectral densities 3 2.3 Brief example: current noise of a quantum point contact 9 2.4 Heisenberg inequality on detector quantum noise 10 3 Quantum limit on QND qubit detection 16 3.1 Measurement rate and dephasing rate 16 3.2 Efficiency ratio 18 3.3 Example: QPC detector 20 3.4 Significance of the quantum limit on QND qubit detection 23 3.5 QND quantum limit beyond linear response 23 4 Quantum limit on linear amplification: the op-amp mode 24 4.1 Weak continuous position detection 24 4.2 A possible correlation-based loophole? 26 4.3 Power gain 27 4.4 Simplifications for a detector with ideal quantum noise and large power gain 30 4.5 Derivation of the quantum limit 30 4.6 Noise temperature 33 4.7 Quantum limit on an \op-amp" style voltage amplifier 33 5 Quantum limit on a linear-amplifier: scattering mode 38 5.1 Caves-Haus formulation of the scattering-mode quantum limit 38 5.2 Bosonic Scattering Description of a Two-Port Amplifier 41 References 50 1 Introduction The fact that quantum mechanics can place restrictions on our ability to make measurements is something we all encounter in our first quantum mechanics class. One is typically presented with the example of the Heisenberg microscope (Heisenberg, 1930), where the position of a particle is measured by scattering light off it. -
Audio Cards for High-Resolution and Economical Electronic Transport Studies
Audio Cards for High-Resolution and Economical Electronic Transport Studies D. B. Gopman,1 D. Bedau,1, ∗ and A. D. Kent1 1Department of Physics, New York University, New York, NY 10003, USA We report on a technique for determining electronic transport properties using commercially avail- able audio cards. Using a typical 24-bit audio card simultaneously as a sine wave generator and a narrow bandwidth ac voltmeter, we show the spectral purity of the analog-to-digital and digital-to- analog conversion stages, including an effective number of bits greater than 16 and dynamic range better than 110 dB. We present two circuits for transport studies using audio cards: a basic circuit using the analog input to sense the voltage generated across a device due to the signal generated simultaneously by the analog output; and a digitally-compensated bridge to compensate for non- linear behavior of low impedance devices. The basic circuit also functions as a high performance digital lock-in amplifier. We demonstrate the application of an audio card for studying the transport properties of spin-valve nanopillars, a two-terminal device that exhibits Giant Magnetoresistance (GMR) and whose nominal impedance can be switched between two levels by applied magnetic fields and by currents applied by the audio card. Studies of the electronic transport properties of devices ing current-voltage characteristics simultaneously. We and materials require specialized instrumentation. Most will present measurements of magnetic nanostructures, transport studies break down into two classes: current- whose current-voltage and differential resistance are used voltage characterization and differential resistance mea- to determine their underlying magnetic and electronic surements. -
CHAPTER 20. NOISE ANALYSIS and LOW NOISE DESIGN
Circuits, Devices, Networks, and Microelectronics CHAPTER 20. NOISE ANALYSIS and LOW NOISE DESIGN 20.1 THE ORIGINS OF NOISE Electrical noise is a background “grass” of unwanted signals, usually due to thermal origins. It has a nearly constant amplitude density across the frequency spectrum that tends to mask and obscure the waveforms and information which we wish for our circuits to process. Noise is an inescapable fact of circuits and signals. It is generated in most part by thermal fluctuations in the motion and flow of charge. It is an important factor in the design and analysis of communication circuits, and therefore most treatments of noise are developed in the context of communications electronics. But electrical noise, and its companion problem, distortion, are an important and necessary consideration of any circuit, in which a signal, whether of linear or logic form, is to be processed. A figure of merit that defines a circuit in terms of its signal transfer properties is the dynamic range (DR) given by The smallest usable signal level is defined by the noise limit. The largest usable signal is defined by the distortion limit, which is usually a consequence of the compliance (±VS) limits of the circuit. In matters of electrical noise, components and devices are defined by thermal kinetics. Thermal statistical fluctuations will produce a random set of signals within an electrical component. Thermal effects manifest themselves as fluctuations in electrical currents. The basic unit of thermal energy (fluctuation) is given by w = kT (defined by the fugacity for electrons), where k = Boltzmann’s constant and T = absolute temperature. -
Local Noise Action Plans
Practitioner Handbook for Local Noise Action Plans Recommendations from the SILENCE project SILENCE is an Integrated Project co-funded by the European Commission under the Sixth Framework Programme for R&D, Priority 6 Sustainable Development, Global Change and Ecosystems Guidance for readers Step 1: Getting started – responsibilities and competences • These pages give an overview on the steps of action planning and Objective To defi ne a leader with suffi cient capacities and competences to the noise abatement measures and are especially interesting for successfully setting up a local noise action plan. To involve all relevant stakeholders and make them contribute to the implementation of the plan clear competences with the leading department are needed. The END ... DECISION MAKERS and TRANSPORT PLANNERS. Content Requirements of the END and any other national or The current responsibilities for noise abatement within the local regional legislation regarding authorities will be considered and it will be assessed whether these noise abatement should be institutional settings are well fi tted for the complex task of noise considered from the very action planning. It might be advisable to attribute the leadership to beginning! another department or even to create a new organisation. The organisational settings for steering and carrying out the work to be done will be decided. The fi nancial situation will be clarifi ed. A work plan will be set up. If support from external experts is needed, it will be determined in this stage. To keep in mind For many departments, noise action planning will be an additional task. It is necessary to convince them of the benefi ts and the synergies with other policy fi elds and to include persons in the steering and working group that are willing and able to promote the issue within their departments. -
Chapter 4 Macroscopic Conductors
Chapter 4 Macroscopic Conductors There are two types of intrinsic noise in every physical system: thermal noise and quan- tum noise. These two types of noise cannot be eliminated even when a device or system is perfectly constructed and operated. Thermal noise is a dominant noise source at high temperatures and/or low frequencies, while quantum noise is dominant at low tempera- tures and/or high frequencies. A conductor with a ¯nite electrical resistance is a simplest system which manifests these two types of intrinsic noise. The intrinsic noise of a macro- scopic conductor will be discussed in this chapter, and that of a mesoscopic conductor will be discussed in the next chapter. A conductor in thermal equilibrium with its surroundings (heat reservoir) shows, at its terminals, an open-circuit voltage or short-circuit current fluctuation, as shown in Fig. 4.1. Thermal equilibrium noise was ¯rst experimentally discovered by J. B. Johnson in 1927[1]. Figure 4.1: Open circuit voltage noise source and short circuit current noise source. He discovered that the open circuit voltage noise power spectral density is independent of the material a conductor is made of and the measurement frequency, and is determined only by the temperature and electrical resistance: Sv(!) = 4kBθR. The corresponding short-circuit current noise spectral density is Si(!) = 4kBθ=R. This noise is referred to as thermal noise and is the most fundamental noise. The physical origin of the thermal noise in a macroscopic conductor is a \random-walk" of thermally-fluctuated charged carriers (electrons, holes or ions). An electron in a metallic 1 conductor undergoes a Brownian motion via collisions with the lattices of a conductor. -
Amplifier Noise Principles for the Practical Engineer
The World Leader in High Performance Signal Processing Solutions Amplifier Noise Principles for the Practical Engineer Matt Duff Applications Engineer – Instrumentation Amplifiers Analog Devices, Inc. copyright 2009 Outline Noise z Extrinsic z Intrinsic Three main sources of intrinsic noise z Resistance z Amplifier Voltage Noise Current Noise z ADC Why so many units? z nV/rt(Hz), µVrms, µVp-p z Unit conversion Noise Math & Shortcuts Tips z Applying gain z Source resistance z Feedback resistance 2 Where does noise come from? -Extrinsic - Intrinsic 3 Extrinsic Noise RFI Switching Noise Noise coupling in from external Power sources Supply + Examples z RFI Coupling – z Power Supply Noise z Ground loops Digital circuitry 50/60 Hz Ground Not focus of this talk Loop Noise 4 Intrinsic Noise Intrinsic z Internal noise from components in signal chain Sensor Resistors Amplifier A/D z Specified on the datasheet z Focus of this talk 5 Main Sources of Intrinsic Noise -Resistor - Amplifier -A/D 6 Resistor noise vn 7 Types of Resistor noise Excess Noise z Depends on type: Carbon composition = bad performance vn Thick film = OK performance Thin film, wirewound = good performance z Increases with applied voltage z 1/f characteristic z Can ignore if using good resistors Intrinsic thermal noise z Independent of type z Independent of voltage applied z White noise characteristic z Need to calculate in design 8 Thermal noise of an ideal resistor bandwidth vn = √4k T R Δf resistance rms noise constant Temperature (in Kelvin) Too Complicated! -
Boundary-Preserved Deep Denoising of the Stochastic Resonance Enhanced Multiphoton Images
Boundary-Preserved Deep Denoising of the Stochastic Resonance Enhanced Multiphoton Images SHENG-YONG NIU1,2, LUN-ZHANG GUO3, YUE LI4, TZUNG-DAU WANG5, YU TSAO1,*, TZU-MING LIU4,* 1. Research Center for Information Technology Innovation (CITI), Academia Sinica, Taipei, Taiwan. 2. Department of Computer Science and Engineering, University of California San Diego, CA, USA. 3. Institute of Biomedical Engineering, National Taiwan University, Taipei 10617, Taiwan. 4. Institute of Translational Medicine, Faculty of Health Sciences, University of Macau, Macao SAR, China. 5. Cardiovascular Center and Division of Cardiology, Department of Internal Medicine, National Taiwan University Hospital and College of Medicine, Taipei 10002, Taiwan. * [email protected] and [email protected] Abstract: As the rapid growth of high-speed and deep-tissue imaging in biomedical research, it is urgent to find a robust and effective denoising method to retain morphological features for further texture analysis and segmentation. Conventional denoising filters and models can easily suppress perturbative noises in high contrast images. However, for low photon budget multi- photon images, high detector gain will not only boost signals, but also bring huge background noises. In such stochastic resonance regime of imaging, sub-threshold signals may be detectable with the help of noises. Therefore, a denoising filter that can smartly remove noises without sacrificing the important cellular features such as cell boundaries is highly desired. In this paper, we propose a convolutional neural network based denoising autoencoder method, Fully Convolutional Deep Denoising Autoencoder (DDAE), to improve the quality of Three-Photon Fluorescence (3PF) and Third Harmonic Generation (THG) microscopy images. The average of the acquired 200 images of a given location served as the low-noise answer for DDAE training. -
Chapter 11 Noise and Noise Rejection
CHAPTER 11 NOISE AND NOISE REJECTION INTRODUCTION In general, noise is any unsteady component of a signal which causes the instantaneous value to differ from the true value. (Finite response time effects, leading to dynamic error, are part of an instrument's response characteristics and are not considered to be noise.) In electrical signals, noise often appears as a highly erratic component superimposed on the desired signal. If the noise signal amplitude is generally lower than the desired signal amplitude, then the signal may look like the signal shown in Figure 1. Figure 1: Sinusoidal Signal with Noise. Noise is often random in nature and thus it is described in terms of its average behavior (see the last section of Chapter 8). In particular we describe a random signal in terms of its power spectral density, (x (f )) , which shows how the average signal power is distributed over a range of frequencies, or in terms of its average power, or mean square value. Since we assume the average signal power to be the power dissipated when the signal voltage is connected across a 1 Ω resistor, the numerical values of signal power and signal mean square value are equal, only the units differ. To determine the signal power we can use either the time history or the power spectral density (Parseval's Theorem). Let the signal be x(t), then the average signal power or mean square voltage is: T t 2 221 x(t) x(t)dtx (f)df (1) T T t 0 2 11-2 Note: the bar notation, , denotes a time average taken over many oscillations of the signal.