High Accuracy Power Quality Evaluation Under a Colored Noisy Condition by Filter Bank ESPRIT
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Noise Reduction Applied to Asteroseismology
PERTURBATIONS OF OBSERVATIONS. NOISE REDUCTION APPLIED TO ASTEROSEISMOLOGY. Javier Pascual Granado CCD 21/10/2009 Contents • Noise characterization and time series analysis Introduction The colors of noise Some examples in astrophysics Spectral estimation • Noise reduction applied to asteroseismology Asteroseismology: Origin and Objetives CoRoT A new method for noise reduction: Phase Adding Method (PAM) Aplications: Numerical experiment Star HD181231 Star 102719279 Javier Pascual Granado CCD 21/10/2009 2 Introduction Javier Pascual Granado CCD 21/10/2009 3 The Colors Of Noise Pink noise Javier Pascual Granado CCD 21/10/2009 4 The Colors Of Noise Red noise Javier Pascual Granado CCD 21/10/2009 5 Some Examples In Astrophysics •Thermal noise due to a nonzero temperature is approximately white gaussian noise. • Photon-shot noise due to statistical fluctuations in the measurements has a Poisson distribution and a power increasing with frequency. It is a problem with weak signals. • Also seismic noise affect to sensible ground instruments like LIGO (gravitational wave detector). Nevertheless, for LISA the noise characterization adopted is a gaussian noise. •Observations of the black hole candidate X-ray binary Cyg X-1 by EXOSAT, show a continuum power spectrum with a pink noise. • In asteroseismology the noise is assumed to be of white gaussian type. Javier Pascual Granado CCD 21/10/2009 6 Time Series: Spectral Estimation A light curve (or a photometric time series) is a set of data points ordered In time. ti-1-ti might not be constant. -
Intuilink Waveform Editor
IntuiLink Waveform Editor The Agilent IntuiLink Arbitrary Waveform Editor application is an ActiveX document server. This application provides a graphical user interface (GUI) that allows you to create, import, modify, and export arbitrary waveforms, and to send these waveforms to the Agilent type 33120A, 33220A or 33250A Arbitrary Waveform (ARB) Generator instrument. The user interface is shown below with its main areas identified by numbers: Let's look at each of these numbered areas in turn. 1. Menu Bar - provides standard Microsoft Windows style menus. 2. Standard Toolbar - provides toolbar buttons for such standard menu functions as Save, Cut, Paste, and Print. 3. Waveform Toolbar - provides toolbar buttons for the arbitrary waveform Creation and Edit functions. In particular, these buttons allow you to Add waveform segments to the active waveform edit window. 4. Waveform Edit Windows - each of these windows allows you to create, edit, and display an arbitrary waveform. (Waveform defaults – see: Appendix A.) The contents of the active waveform edit window can be sent to an Agilent ARB Generator. 5. Status Bar - displays messages about the following: - General status messages. - The current mode. - In Select mode, the start and end positions and number of points selected. - In Marker mode: · When an X marker is being moved, the positions of both X markers and the difference between them. · When a Y marker is being moved, the positions of both Y markers and the difference between them. - In Freehand or Line Draw mode, the cursor position and the length of the waveform. - The address of an arbitrary waveform generator (for example: GPIB0::10::INSTR) if one is connected, or else Disconnected. -
Measurement Techniques of Ultra-Wideband Transmissions
Rec. ITU-R SM.1754-0 1 RECOMMENDATION ITU-R SM.1754-0* Measurement techniques of ultra-wideband transmissions (2006) Scope Taking into account that there are two general measurement approaches (time domain and frequency domain) this Recommendation gives the appropriate techniques to be applied when measuring UWB transmissions. Keywords Ultra-wideband( UWB), international transmissions, short-duration pulse The ITU Radiocommunication Assembly, considering a) that intentional transmissions from devices using ultra-wideband (UWB) technology may extend over a very large frequency range; b) that devices using UWB technology are being developed with transmissions that span numerous radiocommunication service allocations; c) that UWB technology may be integrated into many wireless applications such as short- range indoor and outdoor communications, radar imaging, medical imaging, asset tracking, surveillance, vehicular radar and intelligent transportation; d) that a UWB transmission may be a sequence of short-duration pulses; e) that UWB transmissions may appear as noise-like, which may add to the difficulty of their measurement; f) that the measurements of UWB transmissions are different from those of conventional radiocommunication systems; g) that proper measurements and assessments of power spectral density are key issues to be addressed for any radiation, noting a) that terms and definitions for UWB technology and devices are given in Recommendation ITU-R SM.1755; b) that there are two general measurement approaches, time domain and frequency domain, with each having a particular set of advantages and disadvantages, recommends 1 that techniques described in Annex 1 to this Recommendation should be considered when measuring UWB transmissions. * Radiocommunication Study Group 1 made editorial amendments to this Recommendation in the years 2018 and 2019 in accordance with Resolution ITU-R 1. -
A Mathematical and Physical Analysis of Circuit Jitter with Application to Cryptographic Random Bit Generation
WJM-6500 BS2-0501 A Mathematical and Physical Analysis of Circuit Jitter with Application to Cryptographic Random Bit Generation A Major Qualifying Project Report: submitted to the Faculty of the WORCESTER POLYTECHNIC INSTITUTE in partial fulfillment of the requirements for the Degree of Bachelor of Science by _____________________________ Wayne R. Coppock _____________________________ Colin R. Philbrook Submitted April 28, 2005 1. Random Number Generator Approved:________________________ Professor William J. Martin 2. Cryptography ________________________ 3. Jitter Professor Berk Sunar 1 Abstract In this paper analysis of jitter is conducted to determine its suitability for use as an entropy source for a true random number generator. Efforts are taken to isolate and quantify jitter in ring oscillator circuits and to understand its relationship to design specifications. The accumulation of jitter via various methods is also investigated to determine whether there is an optimal accumulation technique for sampling the uncertainty of jitter events. Mathematical techniques are used to analyze the accumulation process and an attempt at modeling a signal with jitter is made. The physical properties responsible for the noise that causes jitter are also briefly investigated. 2 Acknowledgements We would like to thank our faculty advisors and our mentors at GD, without whom this project would not have been possible. Our advisors, Professor Bill martin and Professor Berk Sunar, were indispensable in keeping us focused on the tasks ahead as well as for providing background to help us explore new questions as they arose. Our mentors at GD were also key to the project’s success, and we owe them much for this. -
Improving Speech Quality for Hearing Aid Applications Based on Wiener Filter and Composite of Deep Denoising Autoencoders
signals Article Improving Speech Quality for Hearing Aid Applications Based on Wiener Filter and Composite of Deep Denoising Autoencoders Raghad Yaseen Lazim 1,2 , Zhu Yun 1,2 and Xiaojun Wu 1,2,* 1 Key Laboratory of Modern Teaching Technology, Ministry of Education, Shaanxi Normal University, Xi’an 710062, China; [email protected] (R.Y.L.); [email protected] (Z.Y.) 2 School of Computer Science, Shaanxi Normal University, No.620, West Chang’an Avenue, Chang’an District, Xi’an 710119, China * Correspondence: [email protected] Received: 10 July 2020; Accepted: 1 September 2020; Published: 21 October 2020 Abstract: In hearing aid devices, speech enhancement techniques are a critical component to enable users with hearing loss to attain improved speech quality under noisy conditions. Recently, the deep denoising autoencoder (DDAE) was adopted successfully for recovering the desired speech from noisy observations. However, a single DDAE cannot extract contextual information sufficiently due to the poor generalization in an unknown signal-to-noise ratio (SNR), the local minima, and the fact that the enhanced output shows some residual noise and some level of discontinuity. In this paper, we propose a hybrid approach for hearing aid applications based on two stages: (1) the Wiener filter, which attenuates the noise component and generates a clean speech signal; (2) a composite of three DDAEs with different window lengths, each of which is specialized for a specific enhancement task. Two typical high-frequency hearing loss audiograms were used to test the performance of the approach: Audiogram 1 = (0, 0, 0, 60, 80, 90) and Audiogram 2 = (0, 15, 30, 60, 80, 85). -
Noise Tutorial Part IV ~ Noise Factor
Noise Tutorial Part IV ~ Noise Factor Whitham D. Reeve Anchorage, Alaska USA See last page for document information Noise Tutorial IV ~ Noise Factor Abstract: With the exception of some solar radio bursts, the extraterrestrial emissions received on Earth’s surface are very weak. Noise places a limit on the minimum detection capabilities of a radio telescope and may mask or corrupt these weak emissions. An understanding of noise and its measurement will help observers minimize its effects. This paper is a tutorial and includes six parts. Table of Contents Page Part I ~ Noise Concepts 1-1 Introduction 1-2 Basic noise sources 1-3 Noise amplitude 1-4 References Part II ~ Additional Noise Concepts 2-1 Noise spectrum 2-2 Noise bandwidth 2-3 Noise temperature 2-4 Noise power 2-5 Combinations of noisy resistors 2-6 References Part III ~ Attenuator and Amplifier Noise 3-1 Attenuation effects on noise temperature 3-2 Amplifier noise 3-3 Cascaded amplifiers 3-4 References Part IV ~ Noise Factor 4-1 Noise factor and noise figure 4-1 4-2 Noise factor of cascaded devices 4-7 4-3 References 4-11 Part V ~ Noise Measurements Concepts 5-1 General considerations for noise factor measurements 5-2 Noise factor measurements with the Y-factor method 5-3 References Part VI ~ Noise Measurements with a Spectrum Analyzer 6-1 Noise factor measurements with a spectrum analyzer 6-2 References See last page for document information Noise Tutorial IV ~ Noise Factor Part IV ~ Noise Factor 4-1. Noise factor and noise figure Noise factor and noise figure indicates the noisiness of a radio frequency device by comparing it to a reference noise source. -
Next Topic: NOISE
ECE145A/ECE218A Performance Limitations of Amplifiers 1. Distortion in Nonlinear Systems The upper limit of useful operation is limited by distortion. All analog systems and components of systems (amplifiers and mixers for example) become nonlinear when driven at large signal levels. The nonlinearity distorts the desired signal. This distortion exhibits itself in several ways: 1. Gain compression or expansion (sometimes called AM – AM distortion) 2. Phase distortion (sometimes called AM – PM distortion) 3. Unwanted frequencies (spurious outputs or spurs) in the output spectrum. For a single input, this appears at harmonic frequencies, creating harmonic distortion or HD. With multiple input signals, in-band distortion is created, called intermodulation distortion or IMD. When these spurs interfere with the desired signal, the S/N ratio or SINAD (Signal to noise plus distortion ratio) is degraded. Gain Compression. The nonlinear transfer characteristic of the component shows up in the grossest sense when the gain is no longer constant with input power. That is, if Pout is no longer linearly related to Pin, then the device is clearly nonlinear and distortion can be expected. Pout Pin P1dB, the input power required to compress the gain by 1 dB, is often used as a simple to measure index of gain compression. An amplifier with 1 dB of gain compression will generate severe distortion. Distortion generation in amplifiers can be understood by modeling the amplifier’s transfer characteristic with a simple power series function: 3 VaVaVout=−13 in in Of course, in a real amplifier, there may be terms of all orders present, but this simple cubic nonlinearity is easy to visualize. -
Dithering and Quantization of Audio and Image
Dithering and Quantization of audio and image Maciej Lipiński - Ext 06135 1. Introduction This project is going to focus on issue of dithering. The main aim of assignment was to develop a program to quantize images and audio signals, which should add noise and to measure mean square errors, comparing the quality of the quantized images with and without noise. The program realizes fallowing: - quantize an image or audio signal using n levels (defined by the user); - measure the MSE (Mean Square Error) between the original and the quantized signals; - add uniform noise in [-d/2,d/2], where d is the quantization step size, using n levels; - quantify the signal (image or audio) after adding the noise, using n levels (user defined); - measure the MSE by comparing the noise-quantized signal with the original; - compare results. The program shows graphic result, presenting original image/audio, quantized image/audio and quantized with dither image/audio. It calculates and displays the values of MSE – mean square error. 2. DITHERING Dither is a form of noise, “erroneous” signal or data which is intentionally added to sample data for the purpose of minimizing quantization error. It is utilized in many different fields where digital processing is used, such as digital audio and images. The quantization and re-quantization of digital data yields error. If that error is repeating and correlated to the signal, the error that results is repeating. In some fields, especially where the receptor is sensitive to such artifacts, cyclical errors yield undesirable artifacts. In these fields dither is helpful to result in less determinable distortions. -
Pink Noise Generator
PINK NOISE GENERATOR K4301 Add a spectrum analyser with a microphone and check your audio system performance. H4301IP-1 VELLEMAN NV Legen Heirweg 33 9890 Gavere Belgium Europe www.velleman.be www.velleman-kit.com Features & Specifications To analyse the acoustic properties of a room (usually a living- room), a good pink noise generator together with a spectrum analyser is indispensable. Moreover you need a microphone with as linear a frequency characteristic as possible (from 20 to 20000Hz.). If, in addition, you dispose of an equaliser, then you can not only check but also correct reproduction. Features: Random digital noise. 33 bit shift register. Clock frequency adjustable between 30KHz and 100KHz. Pink noise filter: -3 dB per octave (20 .. 20000Hz.). Easily adaptable to produce "white noise". Specifications: Output voltage: 150mV RMS./ clock frequency 40KHz. Output impedance: 1K ohm. Power supply: 9 to 12VAC, or 12 to 15VDC / 5mA. 3 Assembly hints 1. Assembly (Skipping this can lead to troubles ! ) Ok, so we have your attention. These hints will help you to make this project successful. Read them carefully. 1.1 Make sure you have the right tools: A good quality soldering iron (25-40W) with a small tip. Wipe it often on a wet sponge or cloth, to keep it clean; then apply solder to the tip, to give it a wet look. This is called ‘thinning’ and will protect the tip, and enables you to make good connections. When solder rolls off the tip, it needs cleaning. Thin raisin-core solder. Do not use any flux or grease. A diagonal cutter to trim excess wires. -
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. -
AN10062 Phase Noise Measurement Guide for Oscillators
Phase Noise Measurement Guide for Oscillators Contents 1 Introduction ............................................................................................................................................. 1 2 What is phase noise ................................................................................................................................. 2 3 Methods of phase noise measurement ................................................................................................... 3 4 Connecting the signal to a phase noise analyzer ..................................................................................... 4 4.1 Signal level and thermal noise ......................................................................................................... 4 4.2 Active amplifiers and probes ........................................................................................................... 4 4.3 Oscillator output signal types .......................................................................................................... 5 4.3.1 Single ended LVCMOS ........................................................................................................... 5 4.3.2 Single ended Clipped Sine ..................................................................................................... 5 4.3.3 Differential outputs ............................................................................................................... 6 5 Setting up a phase noise analyzer ........................................................................................................... -
1Õf Noise from Nonlinear Stochastic Differential Equations
PHYSICAL REVIEW E 81, 031105 ͑2010͒ 1Õf noise from nonlinear stochastic differential equations J. Ruseckas* and B. Kaulakys Institute of Theoretical Physics and Astronomy, Vilnius University, A. Goštauto 12, LT-01108 Vilnius, Lithuania ͑Received 20 October 2009; published 8 March 2010͒ We consider a class of nonlinear stochastic differential equations, giving the power-law behavior of the power spectral density in any desirably wide range of frequency. Such equations were obtained starting from the point process models of 1/ f noise. In this article the power-law behavior of spectrum is derived directly from the stochastic differential equations, without using the point process models. The analysis reveals that the power spectrum may be represented as a sum of the Lorentzian spectra. Such a derivation provides additional justification of equations, expands the class of equations generating 1/ f noise, and provides further insights into the origin of 1/ f noise. DOI: 10.1103/PhysRevE.81.031105 PACS number͑s͒: 05.40.Ϫa, 72.70.ϩm, 89.75.Da I. INTRODUCTION signals with 1/ f noise were obtained in Refs. ͓29,30͔͑see ͓ ͔͒ Power-law distributions of spectra of signals, including also recent papers 5,31 , starting from the point process / ͓ ͔ 1/ f noise ͑also known as 1/ f fluctuations, flicker noise, and model of 1 f noise 27,32–39 . pink noise͒, as well as scaling behavior in general, are ubiq- The purpose of this article is to derive the behavior of the uitous in physics and in many other fields, including natural power spectral density directly from the SDE, without using phenomena, human activities, traffics in computer networks, the point process model.