SURVIVING PROPAGATION

Slides:



Advertisements
Similar presentations
Intermediate Course (6) Propagation Karl Davies Intermediate Course (6) Propagation Karl Davies East Kent Radio Society EKRS 1.
Advertisements

HF Propagation An Introduction for the Newcomer By Gary Sutcliffe, W9XT Copyright (c) 2008 Gary C. Sutcliffe.
Chapter 3 – Radio Phenomena
Technician Licensing Class “T3” Valid dates: July 1, 2010 – June 30, 2014.
General License Class Chapter 7 Propagation.
For HF Beginners Gary Wescom – N0GW
Amateur Radio Frequency Propagation
Introduction Syllabus covers a wide range of propagation topics:-
HOW DOES MY SIGNAL GET FROM HERE TO THERE? By Forest Cummings, W5LQU And Dave Russell, W2DMR.
R ADIO W AVE P ROPAGATION A R EFRESHER B RIEFING B Y : R ON, KØMAJ.
Radio Frequencies. Oscillator Feedback loop Oscillator As the output of the amplifier is fed to the input, feedback or oscillation occurs.
A Tour of the Ham Bands DC to Daylight. VLF Bands NOT available in U.S. 73 Khz Khz Khz. 500 Khz. All limited to very low power – generally.
Propagation Index and Short Wave Communications Rodney Wolfe N3XG.
1 of 12 Chelmsford Amateur Radio Society Intermediate Licence Course Christopher Chapman G0IPU Slide Set 8 (6) Propagation Chelmsford Amateur Radio Society.
Propagation of radio waves. Ways of travelling Propagation in ionosphere Propagation in troposphere Special ways of reflecting Propagation depends on.
HF Radio Wave Propagation
Scientific Notation 1,000,000,000 = 1 X 109 GIGA (G)
General Licensing Class G3A – G3C Radio Wave Propagation Your organization and dates here.
General Licensing Class Skywave Excitement Your organization and dates here.
Technician License Course Chapter 2 Lesson Plan Module 2 – Radio Signals and Waves.
Chapter 7 Propagation The Ionosphere
The Sun and Cycle 24 David Treharne, N8HKU Ford Amateur Radio League January 12th, 2012.
SUBELEMENT G3 RADIO WAVE PROPAGATION [3 Exam Questions - 3 Groups]
K9LA Vancouver 2003 Disturbances to Propagation Carl Luetzelschwab K9LA CQ DX?Where’d everybody go?
Radio Propagation Technician License Class Session 3 N1AW revised 4/2013.
Understand band condition information Use a propagation gadget
“Nowcasting” with DX Toolbox ™ Doug Leach – VE3XK.
The Ultimate DX Experience: Mars! By Marc. C. Tarplee, Ph.D. N4UFP
General Licensing Class Voice Operation Brookhaven National Laboratory Amateur Radio Club.
CRES Amateur Radio Club
General Frequency Ranges Microwave frequency range –1 GHz to 40 GHz –Directional beams possible –Suitable for point-to-point transmission –Used for satellite.
Radio Wave Propagation. VLF ( 3 – 30 KHz) and LF (30 – 300 KHz) Propagation Marc C. Tarplee, Ph.D. ARRL Technical Coordinator SC Section.
1 Antennas for Emergency Communications. Emergency Antennas VHF / UHF - FM HF – Voice, CW, or Digital 2.
HF Propagation Direction of Maximum Radiation h.
SUBELEMENT T3 Radio wave characteristics: properties of radio waves; propagation modes [3 Exam Questions - 3 Groups] 1 Radio Waves 2014.
NVIS June What is NVIS? Near Vertical Incident Skywave ◦A radio propagation mode ◦An alternate method to obtain reliable communication at distances.
Practice Questions 2015 General License Course. How is a directional antenna pointed when making a “long-path” contact with another station? A. Toward.
Radio Wave Propagation
By Saneeju m salu. Radio waves are one form of electromagnetic radiation RADIO WAVES.
Performance of long-distance VHF-band communication links based on scattering from perturbed Ionosphere. מציגים : יואב צידון שי ביטון מנחה : פרופ ' נתן.
G3 - RADIO WAVE PROPAGATION [3 Exam Questions -- 3 Groups] G3A - Sunspots and solar radiation; ionospheric disturbances; propagation forecasting and indices.
Digital Mode by Dr. Joe Taylor K1JT Astrophysicist
Larry, WB9KMW.
General Licensing Class
Chapter 8 Antennas Propagation Dave Piersall, N6ORB.
Propagation Objective: Make you smarter in predicting propagation conditions to make your HF work more predictable. Prop is the one thing you have no.
The HF Bands For HF Beginners Gary Wescom – N0GW.
Sky Wave Propagation.
The Road to 6 Meters “It’s The Magic Band”
Technician Licensing Class
The Sun and HF Propagation
Copyright (c) Gary C. Sutcliffe
Wave Propagation Objective: Make you smarter in predicting propagation conditions to make your HF work more predictable. Prop is the one thing you have.
Chapter 8 Propagation. Chapter 8 Propagation The Ionosphere Regions Ionosphere. A region of the atmosphere extending from 30 miles to 300 miles above.
Mode of Propagation 1/ An amateur is in contact with a station in New York on the 15 metre band, the normal expected mode of propagation will be; Ground.
Chelmsford Amateur Radio Society Intermediate Course (6) Propagation
Conquering The Old Solar Cycle Blues
Technician Licensing Class
Technician Licensing Class
Eng. Ibrahim N. Abu-Isbeih
the least path loss? E3A03 A. When the moon is at perigee
Why are direct (not via a repeater) UHF signals rarely heard from stations outside your local coverage area? A. They are too weak to go very far B. FCC.
Chelmsford Amateur Radio Society Intermediate Course (6) Propagation
Propagation Effects on Communication Links
Anything that can carry information from a source to a destination.
HF Signal Propagation Bill Leonard N0CU 1 June 2019
Technician License Course.
General Licensing Class
WELCOME.
HF Propagation BY AL SHEPPARD, W4ZSC.
Presentation transcript:

SURVIVING PROPAGATION 2017-18 Understand band condition information Use a propagation gadget & beacons Try digital modes now! By: Dick By: Dick Morgan K6RAH Copyright 2017. The Richardson Wireless Klub, Inc. and Richard Morgan K6RAH.

Radio Signal Confusion? Yes! Like predicting the weather…only much harder! Whole branch of astroscience – complex & still evolving Space weather conditions affect all hams Low Solar Cycle…..everybody…Boo-Hiss! Low solar flux & sunspot numbers…Boo-Hiss! Seasonal variations affect frequencies differently Blackouts Solar storms Geomagnetic storms Copyright 2017. The Richardson Wireless Klub, Inc. and Richard Morgan K6RAH.

What’s To Know? Solar activity goes in 10 to 11 year “cycles” Now slipping down Solar Cycle 24 thru 2017+ Boo-Hiss! Cycle 19 was an historic era for ham radio 1954-1964 Copyright 2017. The Richardson Wireless Klub, Inc. and Richard Morgan K6RAH.

What’s To Know? Many factors affect electromagnetic radio waves Sun causes most factors (ultraviolet radiation) The factors affect 4 Ionospheric layers above Earth Some things happen simultaneously – good & bad Solar flares, sunspots, solar winds, X-rays and…Coronal Mass Ejections…Boo-Hiss! MUF constantly changes Copyright 2017. The Richardson Wireless Klub, Inc. and Richard Morgan K6RAH.

What’s To Know? The Ionosphere Often described in four distinct layers D = closest to Earth 25-55 miles up (daylight hours only) E = 55-90 miles up (mostly daylight only) F1 = 90-150 miles up F2 = 250+ miles up Layers absorb, bend, or pass radio waves Ionospheric conditions affect frequencies differently & Frequencies differ between day and night Copyright 2017. The Richardson Wireless Klub, Inc. and Richard Morgan K6RAH.

Transmission Types Line of sight (VHF & UHF) – Repeaters, Satellites Ground Wave – Lower frequencies Refraction/Skip – Important for HF DX Special Effects –Scatter; Ducting; Sporadic E, NVIS, Earth-Moon-Earth No signal in Tulsa? Copyright 2017. The Richardson Wireless Klub, Inc. and Richard Morgan K6RAH.

Gadgets Provide Easy Summary HF & VHF Conditions by band Maximum usable frequency (MUF) Available free on QRZ.com & K5RWK.org Updated propagation details Sunspot Number - 0-250 (now 35) Boo-Hiss! Solar Flux Index – 62.5-300 (now 70) Boo-Hiss! Copyright 2017. The Richardson Wireless Klub, Inc. and Richard Morgan K6RAH.

SFI = Solar Flux Index Solar radiation @10.7cm (62.5 to 300 scale) Indicates “F layer” ionization level Higher number = more ionization = DX! High numbers = increase in MUF Updated 3 times daily Copyright 2017. The Richardson Wireless Klub, Inc. and Richard Morgan K6RAH.

SN = Sunspot Number Scale is 0 to 250. Updated once daily Loosely correlates to the solar flux index Higher sunspot numbers = better DX 2017 Copyright 2017. The Richardson Wireless Klub, Inc. and Richard Morgan K6RAH.

K = Planetary K Index Scale is 0 to 9. Updated 8X daily Measures geomagnetic activity Lower number = usually better DX (below 5) Copyright 2017. The Richardson Wireless Klub, Inc. and Richard Morgan K6RAH.

Meaning for Us Hams? One measure does not tell the story! Elements sometime work together, other times oppose each other. Listening is key! The Solar Gadget provides facts, then interprets likely overall result on HF band conditions. MUF, magnetic field, and basic noise level also very helpful. Watch MUF increase as ionosphere becomes more & more active! Gadget is on the QRZ.com & K5RWK home page. Website is http://www.hamqsl.com/solar.html Copyright 2017. The Richardson Wireless Klub, Inc. and Richard Morgan K6RAH.

HF Propagation Beacons Is this band “dead” today? Nobody transmitting? Radio beacons (18 around the world) transmit CW signals. Monitor to determine current band conditions. Beacon frequencies: 14.100, 18.110, 21.150, 24.930, 28.200 MHz. Sequenced from 100 W down to 0.1 W. Check www.ncdxf.org/beacon.htm for details. W6NEK Beacon Tracker @ www.w6nek.com (free tracker) Copyright 2017. The Richardson Wireless Klub, Inc. and Richard Morgan K6RAH.

HF Reverse Beacons Determine who is receiving your signal with: www.reversebeacon.net Send CW CQ and call sign Search by your call to see which beacons received you. Compare signal reports from reverse beacons (dB). Determine your antenna directionality Determine your amplifier effectiveness. Copyright 2017. The Richardson Wireless Klub, Inc. and Richard Morgan K6RAH.

https://pskreporter.info/pskmap.html Copyright 2017. The Richardson Wireless Klub, Inc. and Richard Morgan K6RAH.

Try HF Digital Modes PSK31, JT65, JT9 - Low power, narrow bandwidth Very active modes (poor HF propagation) - Boo-Hiss! Use a TNC/sound card, PC, existing rig Free software - for digital modes Keyboard (PSK) or mouse clicks (JT) CW still a great option! Digital ‘punch’ Copyright 2017. The Richardson Wireless Klub, Inc. and Richard Morgan K6RAH.

Bandwidth Punch Comparison Bandwidth % *Watt = SSB = 2,500 Hz 100% 50 W RTTY = 300 – 1,000 Hz 12% 417 W JT65A = 178 HZ w/EC 7% 714 W CW = 100 - 500 Hz 4% 1,250 W PSK31 = 50 - 70 Hz 2% 2,500 W JT9 = 16 Hz w/EC 0.6% 8,333 W *Equivalent punch power/Hz based on 50 Watts PEP Copyright 2017. The Richardson Wireless Klub, Inc. and Richard Morgan K6RAH.

Thank you for your Boos and Hisses! Copyright 2017. The Richardson Wireless Klub, Inc. and Richard Morgan K6RAH.