Doppler How to use it?

Similar documents
The Excitement & Challenges of 24 GHz EME. By Al Ward W5LUA August 17, 2012

UNDERSTANDING DOPPLER SHIFT: CRITICAL KNOWLEDGE FOR SUCCESSFUL EME ON THE HIGHER BANDS by Al Katz K2UYH

Working Small Stations on 10 and 24 GHz EME with the help of WSJT

North Texas W5HN NTMS. Microwave Society. Portable 3 cm EME. Al Ward October 15, Microwave Update St. Louis, MO

Earth-Moon-Earth (EME) Communications from 902 MHz to 78 GHz by Al Ward W5LUA

North Texas W5HN NTMS. Microwave Society W5LUA. Presented at Central States VHF Society Elk Grove Village, Illinois July

77 GHz EME at WA3ZKR/4 at Morehead State University

VK7MO 10 GHz EME Grid Square Tour across Australia

Introduction to Microwaves & The North Texas Microwave Society by Al Ward W5LUA Bob Gormley WA5YWC

Microwave EME by Al Ward W5LUA

EME ON 77.5 Ghz. Sergei RW3BP, EME Meeting in Orebro, Sweden, May First of all few words about difficulties we have for EME on this band.

Getting the best out of QRA64 on 10 and 24GHz

This series of "OP" lessons explains how Radio Amateurs should operate to:-

Evolution of the WSJT Digital Modes

SATELLITES WITH A COLLINEAR ANTENNA

HAM RADIO. What s it all about?

Ch. III - Limits of single polarity antennas in the VHF and UHF bands

New Tech - Operating Beric K6BEZ

This series of "OP" lessons explains how Radio Amateurs should operate to:-

VHF/UHF An Expanding World

Amateur Radio Satellites

IARU REGION 2 BAND PLAN

VHF/UHF Beyond FM Bob Witte KØNR Page 1

The Frequency. Los Banos Amateur Radio Club. The Frequency

The First 24 GHz MOONBOUNCE QSO By Barry Malowanchuk VE4MA and Al Ward W5LUA

CARRIER PHASE VS. CODE PHASE

The Rise and Rise of 6cm EME. Peter Blair G3LTF

D-Star call sign terminology

Lance Ginner, K6GSJ, poses with the flight model of Amateur Radio s first satellite, OSCAR 1. He built Oscar 1 in his basement.

Rec. ITU-R F RECOMMENDATION ITU-R F *

Class Overview. Antenna Fundamentals Repeaters Duplex and Simplex Nets and Frequencies Cool Radio Functions Review

ILER MK2. QRP SSB Transceiver in Kit Form Appendices. Last update: May 01, ILER-17 MK2 SSB QRP Transceiver Kit Page 1

Acoustic Based Angle-Of-Arrival Estimation in the Presence of Interference

FM Satellite Communication with Equipment you may already own. by Scott, KA7FVV

FCC Technician License Course

Class outline for Get On The Air

2017 ARRL January VHF Contest Rules

W1AW/0 Minnesota Operating Guide

Dual Band Feedhorns for 2304/3456 MHz and 5760/10368 MHz

Frequency Synchronization in Global Satellite Communications Systems

Amateur Pulsar Detection With EME Equipment

THE INTERMEDIATE VFO

OPERATING AND PROCEDURES. Lesson 2

Laboratory testing of LoRa modulation for CubeSat radio communications

ILER MK2. Appendices

The Ham s Guide to Repeaters and Radio Etiquette

Using WSPR Mode in WSJT7

6 Meters (50-54 MHz):

How do I get started on rtty (or psk)?

This paper appeared in the Proceedings of the 2002 Central States VHF Society Conference, and of the 2002 Prague EME Conference.

WSJT: Digital Communication in Extreme Conditions

The Revival of 9cm EME

WORKING DX WITH JOE TAYLOR

CTU Presents. Contest Hints and Kinks Technique and Station Ward Silver, NØAX

Using CROSSBAND Repeaters (CBRs) - By Neil Robin, WA7NBF - March 14, 2009

Electromagnetic (Light) Waves Electromagnetic Waves

HF Digital Mode Primer

International Amateur Radio Union Region 1 Europe, Middle East, Africa and Northern Asia Founded 1950

RADIO FREQUENCY AND MODULATION SYSTEMS PART 1: EARTH STATIONS AND SPACECRAFT

Lab M6: The Doppler Effect

Technician Licensing Class

TRY AMATEUR SATELLITES PETER GOODHALL, 2E0SQL

Optimizing Averaging for Better Power Measurements

1296 MHz EME Expeditions to the Northeast and Northwest US 2006 and 2007

SONOGRAPHIC PHYSICS, INSTRUMENTATION & DOPPLER REVIEW Part 3

Summits On The Air. Mountain Top Activations and Amateur Radio (Including Chasing) Phil Shepard NS7P June 6, 2015

This presentation on satellite communications is designed to provide a broad introduction into this method of radio communications.

Voltage Multipliers and the Cockcroft-Walton generator. Jason Merritt and Sam Asare. 1. Background

G1MFG.com. Home of the cheapest ATV transmitters and receivers in Europe! Please read all of this document before attempting to use your controller.

Technician License Course Chapter 2. Lesson Plan Module 2 Radio Signals and Waves

Prosigns, Q Signals and CW Abbreviations Used in Amateur (Ham) Radio

Doppler Simulator for 10 GHz Doppler Radar

EXPERIMENTAL STATION FREQUENCY COORDINATION REQUEST 1 USING FREQUENCIES ALLOCATED TO THE AMATEUR AND AMATEUR-SATELLITE SERVICES

DX ing & How To Do It. But really, DX ing Hints and Techniques Brazenly Plagiarized From the Books of W9KNI

Final Reg Wave and Sound Review SHORT ANSWER. Write the word or phrase that best completes each statement or answers the question.

A HamSCI Experiment NVARC and the Eclipse

right during the VE Session Have fun Bob, KA9BH Eric, K9VIC

Past, present and future of Beacon signal transmission for meteor radio observation in Japan

W7PXL Net Operations Documentation

FT-8 Weak Signal Digital

24 GHZ EME - CONQUERED 47 GHZ EME THE NEXT FRONTIER

2018 Draft Band Plan Changes. RSGB Spectrum Forum October 2017

Killing RF Noise for Field Day and CQP. Jim Brown, K9YC

Technician License Course Chapter 2 Radio and Signals Fundamentals

A 1951 Beginner/Novice Station

t =1 Transmitter #2 Figure 1-1 One Way Ranging Schematic

Chapter 22. Electromagnetic Waves

AGF-216. The Earth s Ionosphere & Radars on Svalbard

TORSTEIN PEDERSEN. Improving the Common DVL: A New Standard in Doppler Velocity Logs

Operating Station Equipment

General Rules and Regulations for HF Contests

Current Solar Cycle Poor propagation No propagation Checking HF propagation. Coping with poor HF propagation Q&A

HF Interoperable Communications We can hear you now

Working the Birds An Introduction to FM Satellites

VHF Propagation Overview 5-Oct-2016

Characteristics of systems operating in the amateur and amateur-satellite services for use in sharing studies

VHF Operation and Field Day: FAQ s, Tips and Guides for Getting More Field Day QSOs

An Introduction to Moonbounce

E-200D ALIGNMENT. See the end of the procedure for the location of the calibration points. EQUIPMENT REQUIRED

Figure 1. The Rise and Rise of 6cm EME activity

Transcription:

Doppler How to use it? Al Ward W5LUA July 30, 2008 WWW..ORG 1

Outline Summary of what doppler is How to use the numbers when running random vs scheduling How it applies to both CW and Digital QSOs WWW..ORG 2

The Doppler Effect Doppler effect is the change in frequency of a signal that occurs as a result of the source and the observer moving relative to each other. As the source and/or observer are moving closer to each other, the frequency will increase and as the source and/or observer are moving further away from each other the frequency will decrease. The doppler effect scales proportionally with frequency WWW..ORG 3

The Doppler Effect Since the relative angular velocity of the earth is faster than the orbit of the moon, the doppler is at a maximum at both moon rise and moon set and zero around zenith. Therefore at moon rise the doppler shifted signal will be highest in frequency (positive) gradually decreasing to zero offset from the transmitted frequency at zenith and continuing to decrease to its lowest frequency (negative) at moon set. Slight hook effect at the edges of the earth WWW..ORG 4

F1EHN EME Program at W5LUA Moon rising at W5LUA and near zenith at LX1DB Self Doppler at LX1DB Mutual Doppler Self Doppler at W5LUA WWW..ORG 5

Random Operation on CW Random operation on CW is fairly straightforward simply net your echoes on the frequency of the station calling CQ Even if you can t hear your own echoes, you know from the self doppler where your echoes would be if you could hear them More important is the fact that the bigger station most likely hear you and he will be tuning pretty close to the frequency at which he hears his own echoes WWW..ORG 6

Random Operation on CW Station A in America says he is setting his echoes on say 1296.010 or 10368.100 MHz For other stations in America that are very near the same location, other stations will find station A very near the claimed frequency Any station that is a significant distance away from station A will find station at a significantly different frequency especially at 10 GHz. This is a result of the self doppler being different at different locations, especially when traversing continents Solution Never spot your echo frequency. Simply spot your exact transmit frequency, only then will any station any where (from a known QTH), on any frequency be able to find your signal based on the mutual doppler frequency WWW..ORG 7

Comparison of the Doppler between 1296 and 24048 MHz Moon Rising at W5LUA and nearly at Zenith at LX1DB Self Doppler W5LUA +56.9 khz, LX1DB +8.5 khz If we are both transmitting on 24048.100 MHz, then my echoes will be on.1569 and Willi s will be on.1085 Mutual Doppler is +32.7 khz and is the same for both of us What does this mean and how is it calculated? WWW..ORG 8

Scheduled Operation on CW Self Doppler W5LUA +56.9 khz, LX1DB +8.5 khz If we are both transmitting on 24048.100 MHz, then my echoes will be on.1569 on my dial and Willi s will be on.1085 on his dial Mutual Doppler is +32.7 khz and is the same for both of us Mutual Doppler is calculated from the arithmetic mean or average of the individual stations self doppler Mutual Doppler = (Station #1 Doppler + Station #2 Doppler) / 2 The mutual doppler frequency is the exact frequency at which Willi and I will both hear each other therefore we will both hear each other on 24048.1327 MHz This also means that Willi will appear to be 56.9 32.7 = 24.2 khz below my echoes on my receiver and I will appear to be 32.7 8.5 = 24.2 khz above his echoes on his receiver Therefore when scheduling it is best just to transmit on the exact sked frequency and just tune to the mutual doppler frequency for the scheduled station pretty simple.and it still works at 47 GHz! WWW..ORG 9

Sked Operation on Digital Usually both stations will follow similar guidelines as done on CW, i.e. both stations will transmit on the sked frequency and tune to the mutual doppler frequency Most amateurs on the same continent will find skeded stations close to their self doppler frequency but when working continent to continent one should tune to the mutual doppler frequency sometimes makes it difficult to tail-end but sure makes it easier for skedded stations to find each other. WWW..ORG 10

Random Operation on Digital Most amateurs spot their CQ frequency on the logger on 1296 amateurs in Europe usually find most of the replies on or near their self doppler frequency but what about listening for NA and or JA/VK, etc? My first response would be similar to what I would do on CW, i.e. place my echoes on the frequency on which I see them and they should be able to find me. I would normally not transmit on their announced CQ frequency Is this the acceptable trend on random? I note that Bodo DL3OCH chose to have me transmit on his transmit frequency when I was calling him on random not my first choice but Bodo knew where I would be according to mutual doppler I chose to call him on my self doppler frequency Which approach is best? WWW..ORG 11

Summary CW random, use self doppler offset for transmit CW sked, use mutual doppler offset on receive Digital random, use self doppler offset for transmit Digital sked, use mutual doppler offset on receive Other thoughts? WWW..ORG 12