Fading Correlation Bandwidth and Short-Term Frequency Stability Measurements on a High-Frequency Transauroral Path
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Kindergarten High Frequency Word List
Kindergarten High Frequency Word List The following 40 words are the high frequency Kindergarten words. They are divided according to their probability of occurring in the corresponding DRA text levels. However, many of these words can occur throughout all levels. The goal is for all students to read, write, and use these words correctly by the end of Kindergarten. Level 1 Level 2 Level 3 Level 4 Level 5 a me to yes big I go in cat for is at on dog he the you like up she mom we my with this dad it by said look can no love play went see am do was and C:\Users\metcalfr\Downloads\K_5_High_Frequency_Word_Lists (2).docx October 2014 First Grade High Frequency Word list The goal is for all students to read, write, and use these words (and words from the kindergarten word list) correctly by the end of first grade. after have please all her saw an here should are him so as his some be I’m thank because if that but into them came just then come know they could little there day make us did many very end new want from not were get of what goes one when going or where good our who had out will has over would your C:\Users\metcalfr\Downloads\K_5_High_Frequency_Word_Lists (2).docx October 2014 Second Grade High Frequency Word List The goal is for all students to read, write, and use these words (and the words from preceding grade level word lists) correctly by the end of second grade. -
High Frequency Communications – an Introductory Overview
High Frequency Communications – An Introductory Overview - Who, What, and Why? 13 August, 2012 Abstract: Over the past 60+ years the use and interest in the High Frequency (HF -> covers 1.8 – 30 MHz) band as a means to provide reliable global communications has come and gone based on the wide availability of the Internet, SATCOM communications, as well as various physical factors that impact HF propagation. As such, many people have forgotten that the HF band can be used to support point to point or even networked connectivity over 10’s to 1000’s of miles using a minimal set of infrastructure. This presentation provides a brief overview of HF, HF Communications, introduces its primary capabilities and potential applications, discusses tools which can be used to predict HF system performance, discusses key challenges when implementing HF systems, introduces Automatic Link Establishment (ALE) as a means of automating many HF systems, and lastly, where HF standards and capabilities are headed. Course Level: Entry Level with some medium complexity topics Agenda • HF Communications – Quick Summary • How does HF Propagation work? • HF - Who uses it? • HF Comms Standards – ALE and Others • HF Equipment - Who Makes it? • HF Comms System Design Considerations – General HF Radio System Block Diagram – HF Noise and Link Budgets – HF Propagation Prediction Tools – HF Antennas • Communications and Other Problems with HF Solutions • Summary and Conclusion • I‟d like to learn more = “Critical Point” 15-Aug-12 I Love HF, just about On the other hand… anybody can operate it! ? ? ? ? 15-Aug-12 HF Communications – Quick pretest • How does HF Communications work? a. -
VHF and UHF Signal Characteristics Observed on a Long Knife-Edge Diffraction Path A
JOURNAL OF RESEARCH of the National Bureau of Standards- D. Radio Propagatior. Vol. 65D, No. 5, September- Odober 1961 VHF and UHF Signal Characteristics Observed on a Long Knife-Edge Diffraction Path A. P. Barsis and R. S. Kirby (R eceived April 6, 1961) Contribution from Central Radio Propagation Laboratory, National Bureau of Standards, Boulder, Colo. During 1959 and 1960 long-term transmission loss measurements were performed over a 223 kilom eter path in Eastern Colorado using frequencies of 100 and 751 megacycles per second. This path intersects P ikes P eak which forms a knife-edge type obstacle visible from both terminals. The transmission loss measurements have been analyzed in terms of diurnal a nd seaso nal variations in hourly medians and in instan taneous levels. As expected, results show t hat the long-term fading range is substantially less t han expected for t ropospheric seatter paths of comparable length. T ransmission loss levels were in general agreem ent wi t h predicted k ni fe-edge d iffraction propagation when a ll owance is made for rounding of t he knife edge. A technique for est imatin g long-term fading ra nges is presented a nd t he res ults are in good agreement with observations. Short-term variations in some case resemble t he space-wave fadeo uts commonly observed on within- the-horizon paths, a lthough other phe nomena may contribute to t he fadin g. Since t he foreground telTain was rough there was no evidence of direct a nd grou nd-refl ected lobe structure. -
Capacity of Flat and Freq.-Selective Fading Channels Linear Digital Modulation Review
Lecture 8 - EE 359: Wireless Communications - Winter 2020 Capacity of Flat and Freq.-Selective Fading Channels Linear Digital Modulation Review Lecture Outline • Channel Inversion with Fixed Rate Transmission • Comparison of Fading Channel Capacity under Different Schemes • Capacity of Frequency Selective Fading Channels • Review of Linear Digital Modulation • Performance of Linear Modulation in AWGN 1. Channel Inversion with Fixed Rate Transmission • Suboptimal transmission strategy where fading is inverted to maintain constant re- ceived SNR. • Simplifies system design and is used in CDMA systems for power control. • Capacity with channel inversion greatly reduced over that with optimal adaptation (capacity equals zero in Rayleigh fading). • Truncated inversion: performance greatly improved by inverting above a cutoff γ0. 2. Comparison of Fading Channel Capacity under Different Schemes: • Fading generally decreases channel capacity. • Rate/power adaptation have similar capacity as rate adaptation alone. • Rate adaptation alone has same capacity as no adaptation (RX CSI only) but rate adaptation is more practical due to complexity of ML decoding over long blocklengths that experience all fading values. This ML decoding is necesssary to achieve capacity in the RX CSI only case. • Truncated channel inversion is more practical than rate adaptation, with significant capacity gain over full channel inversion, which has zero capacity in Rayleigh fading. 3. Capacity of Frequency Selective Fading Channels • Capacity for time-invariant frequency-selective fading channels is a \water-filling” of power over frequency. • For time-varying ISI channels, capacity is unknown in general. Approximate by di- viding up the bandwidth subbands of width equal to the coherence bandwidth (same premise as multicarrier modulation) with independent fading in each subband. -
High-Frequency Radiowa Ve Probing of the High-Latitude Ionosphere
RAYMOND A. GREENWALD HIGH-FREQUENCY RADIOWAVE PROBING OF THE HIGH-LATITUDE IONOSPHERE During the past several years, a program of high-frequency radiowave studies of the high-latitude ionosphere has been developed in the APL Space Department. Studies are now being conducted on the formation and motion of high-latitude ionospheric electron density irregularities, using a sophisti cated high-frequency radar system installed at Goose Bay, .Labrador. The radar antenna is also being used to receive signals from a beacon transmitter located at Thule, Greenland. This information is providing a better understanding of the spatial and temporal variability of high-latitude propagation channels and their relationship to disturbances in the magnetosphere-ionosphere system . INTRODUCTION turbances prior to their impingement on the magneto At altitudes above 100 kilometers, the atmosphere sphere is quite limited. Therefore, we still have only of the earth gradually changes from a predominantly limited success in forecasting sudden changes in the neutral medium to an increasingly ionized gas or plas high-latitude ionosphere and consequently in high ma. The ionization is caused chiefly by a combination latitude radiowave propagation. of solar extreme ultraviolet radiation and, at high lati In order for space scientists to obtain a better un tudes, particle precipitation from the earth's magne derstanding of the various interactions occurring tosphere. Because of its ionized nature between 100 among the solar wind, the magnetosphere, and the ion and 1000 kilometers, this part of the atmosphere is osphere, active measurement programs are conduct commonly referred to as the ionosphere. In this re ed in all three regions. -
Distortion Exponent of Parallel Fading Channels
Distortion Exponent of Parallel Fading Channels Deniz Gunduz, Elza Erkip Department of Electrical and Computer Engineering, Polytechnic University, Brooklyn, NY 11201, USA [email protected], [email protected] Abstract— We consider the end-to-end distortion achieved by the fading process. Lack of channel state information at the transmitting a continuous amplitude source over M parallel, transmitter prevents the design of a channel code that achieves independent quasi-static fading channels. We analyze the high the instantaneous channel capacity and requires a code that SNR expected distortion behavior characterized by the distortion exponent. We first give an upper bound for the distortion performs well on the average. We aim to design a joint source- exponent in terms of the bandwidth ratio between the channel channel code that achieves the minimum expected end-to-end and the source assuming the availability of the channel state distortion. Our main focus is the high SNR behavior of this information at the transmitter. Then we propose joint source- expected distortion (ED). This behavior is characterized by the channel coding schemes based on layered source coding and distortion exponent denoted by ¢ and defined as multiple rate channel coding. We show that the upper bound is tight for large and small bandwidth ratios. For the rest, we log ED provide the best known distortion exponents in the literature. ¢ = ¡ lim : (1) SNR!1 log SNR By suitably scaling the bandwidth ratio, our results would also apply to block fading channels. When we consider digital transmission strategies that first compress the source and then transmit over the channel at I. -
On Routing in Random Rayleigh Fading Networks Martin Haenggi, Senior Member, IEEE
IEEE TRANSACTIONS ON WIRELESS COMMUNICATIONS, VOL. 4, NO. 4, JULY 2005 1553 On Routing in Random Rayleigh Fading Networks Martin Haenggi, Senior Member, IEEE Abstract—This paper addresses the routing problem for large loss probabilities increase with the number of hops (unless the wireless networks of randomly distributed nodes with Rayleigh transmit power is adapted). fading channels. First, we establish that the distances between To overcome some of these limitations of the “disk model,” neighboring nodes in a Poisson point process follow a generalized Rayleigh distribution. Based on this result, it is then shown that, we employ a simple Rayleigh fading link model that relates given an end-to-end packet delivery probability (as a quality of transmit power, large-scale path loss, and the success of a service requirement), the energy benefits of routing over many transmission. The end-to-end packet delivery probability over short hops are significantly smaller than for deterministic network a multihop route is the product of the link-level reception models that are based on the geometric disk abstraction. If the probabilities. permissible delay for short-hop routing and long-hop routing is the same, it turns out that routing over fewer but longer hops may While fading has been considered in the context of packet even outperform nearest-neighbor routing, in particular for high networks [16], [17], its impact on the network (and higher) end-to-end delivery probabilities. layers is largely an open problem. This paper attempts to shed Index Terms—Ad hoc networks, communication systems, fading some light on this cross-layer issue by analyzing the perfor- channels, Poisson processes, probability, routing. -
Kahn Communications, Inc. 425 Merrick Avenue Westbury, New York 11590 (516) 2222221
KAHN COMMUNICATIONS, INC. 425 MERRICK AVENUE WESTBURY, NEW YORK 11590 (516) 2222221 THE "WGAS EFFECT" AND THE FUTURE OF AM RADIO In the history of broadcasting a number of "Effects" have dramatically impacted on broadcasting. For example, the "Capture Effect" and the "Multipath Effect" of FM, and earlier "Radio Luxemburg Effect" helped shape broadcasting history. More recently, "Clicks and Pops", "Platform Motion", and "Rain Noise" have influenced the path of AM Stereo. Remember when the Magnavox system was selected by the FCC as the standard in 1980 and the "Click and Pop" effect was discovered. By 1982 it became clear that this "Click and Pop" problem made it essential that the FCC revisit its decision. There is now a new phenomenon which we propose to name the "WGAS Effect" because it was first described in the "Open Mike" section of the September 7, 1987 issue of "Broadcasting" by Mr. Glenn Mace, President of WGAS, South Gastonia, North Carolina. It is essential that all AM broadcasters carefully read this short letter because the very future of AM radio may depend upon the industries knowledge of its contents. It should be stressed that WGAS does not, and cannot, endorse our stereo system as they have never used it. But, nevertheless, we are most appreciative that Mr. Mace has taken the time and effort to make his observations public on this important matter. More will follow re the "WGAS Effect" and how it impacts on all stations, large and small, which must serve listeners in their 25 my/meter contour and beyond. age. -
UNIT -1 Microwave Spectrum and Bands-Characteristics Of
UNIT -1 Microwave spectrum and bands-characteristics of microwaves-a typical microwave system. Traditional, industrial and biomedical applications of microwaves. Microwave hazards.S-matrix – significance, formulation and properties.S-matrix representation of a multi port network, S-matrix of a two port network with mismatched load. 1.1 INTRODUCTION Microwaves are electromagnetic waves (EM) with wavelengths ranging from 10cm to 1mm. The corresponding frequency range is 30Ghz (=109 Hz) to 300Ghz (=1011 Hz) . This means microwave frequencies are upto infrared and visible-light regions. The microwaves frequencies span the following three major bands at the highest end of RF spectrum. i) Ultra high frequency (UHF) 0.3 to 3 Ghz ii) Super high frequency (SHF) 3 to 30 Ghz iii) Extra high frequency (EHF) 30 to 300 Ghz Most application of microwave technology make use of frequencies in the 1 to 40 Ghz range. During world war II , microwave engineering became a very essential consideration for the development of high resolution radars capable of detecting and locating enemy planes and ships through a Narrow beam of EM energy. The common characteristics of microwave device are the negative resistance that can be used for microwave oscillation and amplification. Fig 1.1 Electromagnetic spectrum 1.2 MICROWAVE SYSTEM A microwave system normally consists of a transmitter subsystems, including a microwave oscillator, wave guides and a transmitting antenna, and a receiver subsystem that includes a receiving antenna, transmission line or wave guide, a microwave amplifier, and a receiver. Reflex Klystron, gunn diode, Traveling wave tube, and magnetron are used as a microwave sources. -
HF Radio Propagation
Introduction to HF Radio Propagation 1. The Ionosphere 1.1 The Regions of the Ionosphere In a region extending from a height of about 50 km to over 500 km, most of the molecules of the atmosphere are ionised by radiation from the Sun. This region is called the ionosphere (see Figure 1.1). Ionisation is the process in which electrons, which are negatively charged, are removed from neutral atoms or molecules to leave positively charged ions and free electrons. It is the ions that give their name to the ionosphere, but it is the much lighter and more freely moving electrons which are important in terms of HF (high frequency) radio propagation. The free electrons in the ionosphere cause HF radio waves to be refracted (bent) and eventually reflected back to earth. The greater the density of electrons, the higher the frequencies that can be reflected. During the day there may be four regions present called the D, E, F1 and F2 regions. Their approximate height ranges are: • D region 50 to 90 km; • E region 90 to 140 km; • F1 region 140 to 210 km; • F2 region over 210 km. At certain times during the solar cycle the F1 region may not be distinct from the F2 region with the two merging to form an F region. At night the D, E and F1 regions become very much depleted of free electrons, leaving only the F2 region available for communications. Only the E, F1 and F2 regions refract HF waves. The D region is very important though, because while it does not refract HF radio waves, it does absorb or attenuate them (see Section 1.5). -
Long-Wave and Medium-Wave Propagation
~EMGINEERING TRAINING SUPPLEMENT No. 10 LONG-WAVE AND MEDIUM-WAVE PROPAGATION BRITISH BROADCASTING CORPORATION LONDON 1957 ENGINEERING TRAINING SUPPLEMENT No. 10 LONG-WAVE AND MEDIUM-WAVE PROPAGATION Prepared by the Engineering Training Department from an original manuscript by H. E. FARROW, Grad.1.E.E. Issued by THE BBC ENGINEERING TRAINING DEPARTMENT 1957 ACKNOWLEDGMENTS Fig. 2 is based upon a curve given by H. P. Williams in 'Antenna Theory and Design', published by Sir Isaac Pitrnan and Sons Ltd. Figs. 5, 6, 7, 8 and 9 are based upon curves prepared by the C.C.I.R. CONTENTS ACKNOWLEDGMENTS... ... INTRODUCTION ... ... ... AERIALS ... ... ... ... GROUND-WAVEPROPAGATION ... GEOLOGICALCORRELATION ... PROPAGATIONCURVES ... ... RECOVERYAND LOSS EFFECTS ... MIXED-PATHPROPAGATION ... SYNCHRONISED. GROUP WORKING LOW-POWERINSTALLATIONS ... IONOSPHERICREFLECTION ... FADING ... ... ... ... REDUCTIONOF SERVICEAREA BY SKYWAVE ... LONG-RANGEINTERFERENCE BY SKYWAVE ... APPENDIXI ... ... ... ... ... REFERENCES ... ... ... ... ... LONG-WAVE AND MEDIUM-WAVE PROPAGATION The general purpose of this Supplement is to explain the main features of propagation at low and medium frequencies i.e. 30-3000 kc/s, and in particular in the bands used for broadcasting viz. 150-285 kc/s and 525-1605 kc/s. In these bands, the signal at the receiver may have two components: they are (a) a ground wave, i.e. one that follows ground contours (b) an ionspheric wave (sky wave) which is reflected from an ionised layer under certain conditions. In the vicinity of the transmitter, the ground wave is the predominant component, and for domestic broadcasting, the service ideally would be provided by the ground wave only. In fact the limit to the service area is often set by interference from the sky wave. -
A Study of Radio Signal Fading
.. A STUDY OF RADIO SIGNAL FADING. By J. H. Dellinger, L. E. Whittemore, and S. Kruse. ABSTRACT. During the years 1920 and 1921 a study was made of the variations of intensity of received radio signals of higli frequency or short wave length. The investigation was conducted with the assistance of the American Radio Relay I,eague. During the tests from 5 to 10 radio stations transmitted signals in succession. These signals were received simultaneously at about 100 receiving stations, whose operators were pro- vided with forms for recording the variation in the intensity of the signals as received. Particular attention was given to the intensity of signals, the fading of signals, the prevalence of strays or atmospheric disturbances, and the weather conditions existing at the time of transmission. An analysis was made of the reports received, and sum- mary tables are given which point ovt possible relationships between the received signal intensity, fading and strays, and the weather conditions existing at the time. It is concluded that the sources or causes of fading are intimately associated with conditions at the Heaviside surface, which is a conducting surface some 60 miles above the earth. Daytime transmission is largely carried on by means of waves mov- ing along the ground, while night transmission, especially for great distances and short waves, is by means of waves transmitted along the Heaviside surface. Waves at night are thus free from the more uniform absorption encountered in the daj^ime, but are subject to great variations caused by irregularities of the ionized air at or near the Heaviside siirface.