Understanding Noise Figure
Total Page:16
File Type:pdf, Size:1020Kb
Load more
Recommended publications
-
Tm Synchronization and Channel Coding—Summary of Concept and Rationale
Report Concerning Space Data System Standards TM SYNCHRONIZATION AND CHANNEL CODING— SUMMARY OF CONCEPT AND RATIONALE INFORMATIONAL REPORT CCSDS 130.1-G-3 GREEN BOOK June 2020 Report Concerning Space Data System Standards TM SYNCHRONIZATION AND CHANNEL CODING— SUMMARY OF CONCEPT AND RATIONALE INFORMATIONAL REPORT CCSDS 130.1-G-3 GREEN BOOK June 2020 TM SYNCHRONIZATION AND CHANNEL CODING—SUMMARY OF CONCEPT AND RATIONALE AUTHORITY Issue: Informational Report, Issue 3 Date: June 2020 Location: Washington, DC, USA This document has been approved for publication by the Management Council of the Consultative Committee for Space Data Systems (CCSDS) and reflects the consensus of technical panel experts from CCSDS Member Agencies. The procedure for review and authorization of CCSDS Reports is detailed in Organization and Processes for the Consultative Committee for Space Data Systems (CCSDS A02.1-Y-4). This document is published and maintained by: CCSDS Secretariat National Aeronautics and Space Administration Washington, DC, USA Email: [email protected] CCSDS 130.1-G-3 Page i June 2020 TM SYNCHRONIZATION AND CHANNEL CODING—SUMMARY OF CONCEPT AND RATIONALE FOREWORD This document is a CCSDS Report that contains background and explanatory material to support the CCSDS Recommended Standard, TM Synchronization and Channel Coding (reference [3]). Through the process of normal evolution, it is expected that expansion, deletion, or modification of this document may occur. This Report is therefore subject to CCSDS document management and change control procedures, which are defined in Organization and Processes for the Consultative Committee for Space Data Systems (CCSDS A02.1-Y-4). Current versions of CCSDS documents are maintained at the CCSDS Web site: http://www.ccsds.org/ Questions relating to the contents or status of this document should be sent to the CCSDS Secretariat at the email address indicated on page i. -
Problems in Residential Design for Ventilation and Noise
Proceedings of the Institute of Acoustics PROBLEMS IN RESIDENTIAL DESIGN FOR VENTILATION AND NOISE J Harvie-Clark Apex Acoustics Ltd, Gateshead, UK (email: [email protected]) M J Siddall LEAP : Low Energy Architectural Practice, Durham, UK (email: [email protected]) & Northumbria University, Newcastle upon Tyne, UK ([email protected]) 1. ABSTRACT This paper addresses three broad problems in residential design for achieving sufficient ventilation provision with reasonable internal ambient noise levels. The first problem is insufficient qualification of the ventilation conditions that should be achieved while meeting the internal ambient noise level limits. Requirements from different Planning Authorities vary widely; qualification of the ventilation condition is proposed. The second problem concerns the feasibility of natural ventilation with background ventilators; the practical result falls between Building Control and Planning Authority such that appropriate ventilation and internal noise limits may not both be achieved. Greater coordination between planning guidance and Building Regulations is suggested. The third problem concerns noise from mechanical systems that is currently entirely unregulated, yet again can preclude residents from enjoying reasonable indoor air quality and noise levels simultaneously. Surveys from over 1000 dwellings are reviewed, and suitable noise limits for mechanical services are identified. It is suggested that commissioning measurements by third party accredited bodies are required in all cases as the only reliable means to ensure that that the intended conditions are achieved in practice. 2. INTRODUCTION The adverse effects of noise on residents are well known; the general limits for internal ambient noise levels are described in the World Health Organisations Guidelines for Community Noise (GCN)1, Night Noise Guidelines (NNG)3 and BS 82332. -
Noise Tutorial Part V ~ Noise Factor Measurements
Noise Tutorial Part V ~ Noise Factor Measurements Whitham D. Reeve Anchorage, Alaska USA See last page for document information Noise Tutorial V ~ Noise Factor Measurements 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 4-2 Noise factor of cascaded devices 4-3 References Part V ~ Noise Measurements Concepts 5-1 General considerations 5-1 5-2 Noise factor measurements with the Y-factor method 5-6 5-3 References 5-8 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 V ~ Noise Factor Measurements Part V ~ Noise Factor Measurements 5-1. General considerations Noise factor is an important measurement for amplifiers used in low noise applications such as radio telescopes and radar and other radio receivers designed to detect very low signal levels. -
What Is Different? Between Impulse Noise and Electrical Fast Transient Burst】
【What is different? Between Impulse Noise and Electrical Fast Transient Burst】 The Inquiry about "a distinction between an impulse noise simulator (following and our company model INS series) and a Fast transient Burst simulator (following and our company model FNS series)" is one of the major questions in a lot of quries from customers. Herewith the difference is focused and presented. The phenomenon which are reproduced and backgraound Both INS and FNS reproduce phenomenon of back electromotive energy noise which may be generated in ON/OFF of power supply switching (like a gas insulated braker and/or electromagnetism relay, etc.). INS was introduced by Mr. Manohar L.Tandor (at that time worked in I.B.M) as a simulator of the high frequency noise to data processing apparatus in the 1960s, and the computer maker of those days adopted it in the 1970s, and it spread widely. FNS is indicated as a basic standard of the immunity type test which reproduces the malfunction by the noise phenomenon of switching ON/OFF and adopted not only in Europe but also world-wide. The 1st edition of Standard for this test was issued as IEC801-4 in IEC TC65 (Industrial Process Controls) in 1988. Then, in order to adopt to all the electric devices, IEC1000-4-4 was issued in 1995. Moreover, in order to differenciate the numbering between ISO and IEC, “60000” has been added to the Stadanrd number. Consequently, it has been named as IEC61000-4-4. output waveform Rise time / the pulse width [INS] It is a rectangular wave whose pulse width is 50ns-1μs and rise time is less than 1ns. -
All You Need to Know About SINAD Measurements Using the 2023
applicationapplication notenote All you need to know about SINAD and its measurement using 2023 signal generators The 2023A, 2023B and 2025 can be supplied with an optional SINAD measuring capability. This article explains what SINAD measurements are, when they are used and how the SINAD option on 2023A, 2023B and 2025 performs this important task. www.ifrsys.com SINAD and its measurements using the 2023 What is SINAD? C-MESSAGE filter used in North America SINAD is a parameter which provides a quantitative Psophometric filter specified in ITU-T Recommendation measurement of the quality of an audio signal from a O.41, more commonly known from its original description as a communication device. For the purpose of this article the CCITT filter (also often referred to as a P53 filter) device is a radio receiver. The definition of SINAD is very simple A third type of filter is also sometimes used which is - its the ratio of the total signal power level (wanted Signal + unweighted (i.e. flat) over a broader bandwidth. Noise + Distortion or SND) to unwanted signal power (Noise + The telephony filter responses are tabulated in Figure 2. The Distortion or ND). It follows that the higher the figure the better differences in frequency response result in different SINAD the quality of the audio signal. The ratio is expressed as a values for the same signal. The C-MES signal uses a reference logarithmic value (in dB) from the formulae 10Log (SND/ND). frequency of 1 kHz while the CCITT filter uses a reference of Remember that this a power ratio, not a voltage ratio, so a 800 Hz, which results in the filter having "gain" at 1 kHz. -
Measurements 1: Signal Receiving Techniques
MeasurementsMeasurements 1:1: SignalSignal receivingreceiving techniquestechniques Fritz Caspers CAS, Aarhus, June 2010 Contents • The radio frequency (RF) diode • Superheterodyne concept • Spectrum analyzer • Oscilloscope • Vector spectrum and FFT analyzer • Decibel • Noise basics • Noise‐figure measurement with the spectrum analyzer CAS, Aarhus, June 2010 2 The RF diode (1) • We are not discussing the generation of RF signals here, just the detection • Basic tool: fast RF* diode (= Schottky diode) • In general, Schottky diodes are fast but still have a voltage dependent junction capacity (metal –semi‐ A typical RF detector diode conductor junction) Try to guess from the type of the connector which side is the RF input and which is the output • Equivalent circuit: Video output *Please note, that in this lecture we will use RF for both the RF and micro wave (MW) range, since the borderline between RF and MW is not defined unambiguously CAS, Aarhus, June 2010 3 The RF diode (2) • Characteristics of a diode: • The current as a function of the voltage for a barrier diode can be described by the Richardson equation: The RF diode is NOT an ideal commutator for small signals! We cannot apply big signals otherwise burnout CAS, Aarhus, June 2010 4 The RF diode (3) • In a highly simplified manner, one can approximate this expression as: VJ … junction voltage • and show as sketched in the following, that the RF rectification is linked to the second derivation (curvature) of the diode characteristics: CAS, Aarhus, June 2010 5 The RF diode (4) • This diagram depicts the so called square‐law region where the output voltage (VVideo) is proportional to the input power • Since the input power is proportional to the square of the input voltage (V 2) and the RF output signal is proportional to the input power, this region is called square‐ Linear Region law region. -
Improved 1/F Noise Measurements for Microwave Transistors Clemente Toro Jr
University of South Florida Scholar Commons Graduate Theses and Dissertations Graduate School 6-25-2004 Improved 1/f Noise Measurements for Microwave Transistors Clemente Toro Jr. University of South Florida Follow this and additional works at: https://scholarcommons.usf.edu/etd Part of the American Studies Commons Scholar Commons Citation Toro, Clemente Jr., "Improved 1/f Noise Measurements for Microwave Transistors" (2004). Graduate Theses and Dissertations. https://scholarcommons.usf.edu/etd/1271 This Thesis is brought to you for free and open access by the Graduate School at Scholar Commons. It has been accepted for inclusion in Graduate Theses and Dissertations by an authorized administrator of Scholar Commons. For more information, please contact [email protected]. Improved 1/f Noise Measurements for Microwave Transistors by Clemente Toro, Jr. A thesis submitted in partial fulfillment of the requirements for the degree of Master of Science in Electrical Engineering Department of Electrical Engineering College of Engineering University of South Florida Major Professor: Lawrence P. Dunleavy, Ph.D. Thomas Weller, Ph.D. Horace Gordon, Jr., M.S.E., P.E. Date of Approval: June 25, 2004 Keywords: low, frequency, flicker, model, correlation © Copyright 2004, Clemente Toro, Jr. DEDICATION This thesis is dedicated to my father, Clemente, and my mother, Miriam. Thank you for helping me and supporting me throughout my college career! ACKNOWLEDGMENT I would like to acknowledge Dr. Lawrence P. Dunleavy for proving the opportunity to perform 1/f noise research under his supervision. For providing software solutions for the purposes of data gathering, I give credit to Alberto Rodriguez. In addition, his experience in the area of noise and measurements was useful to me as he generously brought me up to speed with understanding the fundamentals of noise and proper data representation. -
Enhanced-SNR Impulse Radio Transceiver Based on Phasers Babak Nikfal,Studentmember,IEEE, Qingfeng Zhang, Member, IEEE,Andchristophe Caloz, Fellow, IEEE
778 IEEE MICROWAVE AND WIRELESS COMPONENTS LETTERS, VOL. 24, NO. 11, NOVEMBER 2014 Enhanced-SNR Impulse Radio Transceiver Based on Phasers Babak Nikfal,StudentMember,IEEE, Qingfeng Zhang, Member, IEEE,andChristophe Caloz, Fellow, IEEE Abstract—The concept of signal-to-noise ratio (SNR) enhance- transmitter. The message data, which are reduced in the figure ment in impulse radio transceivers based on phasers of opposite to a single baseband rectangular pulse representing a bit of in- chirping slopes is introduced. It is shown that SNR enhancements formation, is injected into the pulse shaper to be transformed by factors and are achieved for burst noise and Gaussian into a smooth Gaussian-type pulse, , of duration .This noise, respectively, where is the stretching factor of the phasers. An experimental demonstration is presented, using stripline cas- pulse is mixed with an LO signal of frequency , which yields caded C-section phasers, where SNR enhancements in agreement the modulated pulse , of peak power . with theory are obtained. The proposed radio analog signal pro- This modulated pulse is injected into a linear up-chirp phaser, cessing transceiver system is simple, low-cost and frequency scal- and subsequently transforms into an up-chirped pulse, . able, and may therefore be suitable for broadband impulse radio Assuming energy conservation (lossless system), the duration ranging and communication applications. of this pulse has increased to while its peak power has de- Index Terms—Dispersion engineering, impulse radio, phaser, creased to ,where is the stretching factor of the phaser, radio analog signal processing, signal-to-noise ratio. given by ,where and are the duration of the input and output pulses, respectively, is the slope of the group delay response of the phaser (in I. -
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. -
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. -
AN-1496 Noise, TDMA Noise, and Suppression Techniques (Rev. D)
Application Report SNAA033D–May 2006–Revised May 2013 AN-1496 Noise, TDMA Noise, and Suppression Techniques ..................................................................................................................................................... ABSTRACT The term “noise” is often and loosely used to describe unwanted electrical signals that distort the purity of the desired signal. Some forms of noise are unavoidable (e.g., real fluctuations in the quantity being measured), and they can be overcome only with the techniques of signal averaging and bandwidth narrowing. Other forms of noise (for example, radio frequency interference and “ground loops”) can be reduced or eliminated by a variety of techniques, including filtering and careful attention to wiring configuration and parts location. Finally, there is noise that arises in signal amplification and it can be reduced through the techniques of low-noise amplifier design. Although noise reduction techniques can be effective, it is prudent to begin with a system that is free of preventable interference and that possesses the lowest amplifier noise possible1. This application note will specifically address the problem of TDMA Noise customers have encountered while driving mono speakers in their GSM phone designs. Contents 1 Noise and TDMA Noise .................................................................................................... 2 2 Conclusion ................................................................................................................... 6