the ionogram and radio propagation · 2017-12-21 · the ionogram and radio propagation by terry g....
TRANSCRIPT
The Ionogram and Radio Propagation
by
Terry G. GlagowskiW1TR / AFA1DI
By Terry G. Glagowski / W1TR / AFA1DI - 9/29/2017 9:46 AMExcerpts from a presentation by Tom Carrigan / NE1R / AFA1ID
Knowledge of Radio Propagation is important to the operations of HF MARS nets.It enables the NCS to choose the proper frequency so that the net can reach the most stations.
If the chosen frequency is too high, skip zones may prevent reaching close in stations.If the chosen frequency is too low, distant stations may be weak or unreadable.
Radio checks on the alternative frequencies is the best indication of useable propagation.Use of Ionograms created by Digisondes can help in deciding the proper frequency.
When the Internet is available, Ionograms can be viewed online at various sites.
Introduction• Radio Propagation
– Ground Wave– Skywave– NVIS
• Ionosphere Layers– Creation of Ionosphere– D Layer: Absorption– E Layer: Sporadic Es Skywave– F Layers: F1, F2 Primary Skywave– FoF2 Critical Frequency: NVIS– MUF Maximum Useable Frequency: DX
• Solar Behavior– 11 year Sunspot Cycles– SSN– SFI– A Index– K Index– Solar Flares, CME
• Ionogram– Digisondes generate Ionograms– Interpretation of the Ionogram
• How to Choose Net Frequency– Geography– MUF and FoF2
Radio Propagation
http://www.frankswebspace.org.uk/ScienceAndMaths/physics/physicsGCE/images/transmissionPaths.gif
Freq > MUFMaximum Frequency
Reflected by Ionosphere
Freq < MUF
Critical FrequencyFoF2 = MUF
For NVIS
Ionospheric Layers
http://image.slidesharecdn.com/radiopropagation101-141231201444-conversion-gate01/95/radio-propagation-101-18-638.jpg?cb=1420058206
Ionospheric Layers – D Layer
http://image.slidesharecdn.com/radiopropagation101-141231201444-conversion-gate01/95/radio-propagation-101-19-638.jpg?cb=1420058206
0-5 mHz
5-10 mHz10-30 mHz
Ionospheric Layers – E Layer
http://image.slidesharecdn.com/radiopropagation101-141231201444-conversion-gate01/95/radio-propagation-101-20-638.jpg?cb=1420058206
30-200 mHz
Ionospheric Layers – F Layers
http://image.slidesharecdn.com/radiopropagation101-141231201444-conversion-gate01/95/radio-propagation-101-21-638.jpg?cb=1420058206
Ionospheric Layers – Frequencies
http://image.slidesharecdn.com/radiopropagation101-141231201444-conversion-gate01/95/radio-propagation-101-25-638.jpg?cb=1420058206
Skywave Propagation
Freq > MUF
Freq < MUF
NVIS when Skip Distance = 0, when F < FoF2 Critical Frequency
http://images.tutorvista.com/content/communication-systems/ionosphere-effects.gif
Solar Indices
http://image.slidesharecdn.com/cycle24hbarctalk-150128054239-conversion-gate02/95/cycle-24-hbarc-talk-7-638.jpg?cb=1422426843
Solar Indices
http://image.slidesharecdn.com/cycle24hbarctalk-150128054239-conversion-gate02/95/cycle-24-hbarc-talk-15-638.jpg?cb=1422426843
Sunspot Cycles
http://image.slidesharecdn.com/cycle24hbarctalk-150128054239-conversion-gate02/95/cycle-24-hbarc-talk-10-638.jpg?cb=1422426843
Geomagnetic – A Index
http://image.slidesharecdn.com/cycle24hbarctalk-150128054239-conversion-gate02/95/cycle-24-hbarc-talk-16-638.jpg?cb=1422426843
Geomagnetic – K Index
http://image.slidesharecdn.com/cycle24hbarctalk-150128054239-conversion-gate02/95/cycle-24-hbarc-talk-17-638.jpg?cb=1422426843
CME – Coronal Mass Ejection
http://image.slidesharecdn.com/cycle24hbarctalk-150128054239-conversion-gate02/95/cycle-24-hbarc-talk-22-638.jpg?cb=1422426843
Solar and Geomagnetic Indices
http://image.slidesharecdn.com/cycle24hbarctalk-150128054239-conversion-gate02/95/cycle-24-hbarc-talk-14-638.jpg?cb=1422426843
http://www.hamqsl.com/solar101pic.php
Digisonde
Apparatus to generate Ionogramsand calculate FoF2 and MUFhttp://digisonde.com/images/Digisonde-HF-Radar-System2.jpg
Ionogram - Notional
http://www.astrosurf.com/luxorion/Radio/ionogram-dwg.gif
Ionogram - Legend
https://upload.wikimedia.org/wikipedia/commons/a/a7/HAARP_ionogram.png
Ionogram - Terms
http://www.g0lfp.com/ionograms/ursi_codes.html
URSI Ionospheric Parameter Codes
F Layer ParametersParameter DescriptionfoF2 F2 layer o-mode (ordinary) critical frequency.fxF2 F2 layer x-mode (extraordinary) critical frequency.fzF2 F2 layer z-mode critical frequency.M3000F2 F2 layer M factor (the ratio of the maximum usable frequency divided by the critical frequency).h'F2 F2 layer o-mode minimum virtual height.hpF2 An estimate of the true height of the F2 layer (measurement of the ordinary mode virtual height at a frequency of 83.4% of the foF2).h'Ox F layer minmum virual height of the x-mode trace at a frequency equal to the foF2.MUF3000F2 F2 layer maximum usable frequency for 3000km path.foF1 F1 layer o-mode critical frequency.fxF1 F1 layer x-mode critical frequencyh'F1 F1 layer o-mode minimum virtual height.h'F F layer o-mode minimum virual height.MUF3000F1 F1 layer maximum usable frequency(see code 07).
E Layer ParametersParameter DescriptionfoE E layer o-mode critical frequency.foE2 E2 layer o-mode critical frequency (when it occurs it is between the normal E and F1 layers).h'E E layer o-mode minmum virual height.h'E2 E2 layer o-mode minimum virtual height.
Es Layer ParametersParameter DescriptionfoEs Es layer hightest o-mode frequency are which a mainly continuous Es trace is observed.fxE Es layer highest x-mode frequency are which a mainly continuous Es trace is observed.fbEs The blanketing frequency of layer used to derive foEs.ftEs Top frequency of the Es trace (any mode).
FoF2 Map
http://www.sws.bom.gov.au/Images/HF%20Systems/Global%20HF/Ionospheric%20Map/WorldIMap.gif
4 to 5 MHz
Ionogram - Actual
FoF2
http://umlcar.uml.edu/WatchIt/latestIonogram.html
MUF
FoF2
E Layer
D LayerAbsorption
Multiple F2Reflections
FxF2 Extraordinary
F2
F2
F2
FoF2 / MUF Indicate2.5 MHz NVIS, Absorption?3.3 MHz NVIS, Absorption?4.6 MHz NVIS5.8 MHz 700 KM Skip7.6 MHz 1200 KM SkipE Layer may cause Absorption
How to Choose a Net FrequencyAlways Confirm Prediction with RADIO CHECK Before NetRegion Nets• Check Ionogram for FoF2 frequency• Choose highest frequency <= FoF2, where there will be NO SKIP ZONE
Division Nets (RGN 1,2,3)• Determine the geographical region of the net operations• Check the Ionogram to see what the FoF2 and skip distances will be• Frequencies slightly higher than FoF2 will work somewhat due to ground wave• If multiple Net Control Stations (NCS) are available
then a small to moderate skip zone can be tolerated (less than 400 km)and therefore a somewhat higher frequency can be used
• During daytime, absorption by D and E layers can be a factorso using the highest workable frequency
TransGlobal Net• Choose a frequency less than the MUF for the geographical area
but high enough to avoid absorption during the day by the D layer• Check the Ionogram to see what the MUF, FoF2, and skip distances will be• Since there will be a skip zone,
multiple NCS stations will be required: West, East, and Central.
USAF MARS NE Division, Regions 1,2,3
NVIS vs DX AntennasNVIS Antenna
High Angle of Radiation
DX AntennaLow Angle of Radiation
Vertical
Yagi
Low Dipole or Horizontal Loop
Propagation SitesA-Index, K-Index, SFI SummaryCONUS HF Band ConditionsNOAA IonogramMillstone Hill IonogramWallops Is IonogramLatest IonogramsIonogram Explanation (Wikipedia)Understanding Ionograms – G0LFPDX MapsIonospheric Map – Australian Space Weather ServicesQuick Guide to HF Propabation Using Solar Indices (N2LVI)HF Propagation Tools (N0NBH)K-Index (WikiPedia)Space Weather Prediction Center (NOAA)Space Weather (.com)Solar Hamhttp://car.uml.edu/common/DIDBFastStationList - List of Ionosode Stationshttp://www.sws.bom.gov.au/HF_Systems/6/5 - FoF2 Map
Conclusion• Many factors regarding solar conditions
affect the ionosphere,and the magnetosphere,which affect radio propagation.– Time of Day– Day of Month (28 day rotation of sun)– Time of Year– Sunspot Cycle– Solar Flares– Geomagnetic Storms
• The best indication of good propagation is an actual radio check.
• Use of solar and geomagnetic indicesand ionograms,can greatly aid in the choice of the best frequency for net operations.
Extra Slides
The Ionosphere• The Ionosphere is a plasma shell of electrons, positive ions,
and molecules that surrounds the earth• The Ionosphere is created by ultraviolet radiation from the sun,
which ionizes the molecules of the atmosphere• Ionization is the process of ultraviolet photons transferring energy to a molecule,
thereby causing the electron and the positive ion to separate• Recombination is the reverse process, where a photon is emitted
when an electron recombines with the positive ion randomly and spontaneously• The electron density is determined by the
relative ionization and recombination rates when they are in equilibrium• The critical frequency is dependent on the electron density
at any given region: latitude, longitude, altitude, of the ionosphere• The maximum usable frequency for a given distance is dependent on
the critical frequency and critical angle • Factors affecting ionization include:
• Time of day (daylight vs darkness)• Day of month (28 1/2 day solar rotation), sunspots, flares point towards or away from earth• Time of year (summer vs winter vs fall and spring), amount of daylight and ionization• Solar Cycle (solar flux, sunspot number)• Solar Flares (unpredictable), proton and X-Ray events• Solar Wind creating Geomagnetic Storms
PROTON
ELECTRON
NEUTRON
PHOTONFREE
ELECTRON
Ionization and RecombinationIonization
occurs withsolar radiation (uv)
Recombinationoccurs randomly, spontaneously
proportional to density
PROTON
ELECTRON
NEUTRON
PHOTON
FREEELECTRON
Photon energy is proportional to frequency,Inversely proportional to wavelength.Units are in electron volts.Energy eV = 1.2398 / wavelength um.Minimum energy of ultra violet wavelengthIs needed to cause ionization.Ultraviolet is 10 – 400 nm.Or 3.1 – 124 eV.X-Rays have higher energy.
Ionospheric Layers
http://www.sws.bom.gov.au/Images/Educational/Other%20Topics/Radio%20Communication/ionosphere.png
Radio properties of the ionosphere,i.e. critical frequency, are determined by electron density, which is related to ionization rate, which depends on solar radiation.
Ionospheric Layers – Heights
http://image.slidesharecdn.com/radiopropagation101-141231201444-conversion-gate01/95/radio-propagation-101-22-638.jpg?cb=1420058206
Multi-Hop Propagation (DX)
http://www.astrosurf.com/luxorion/Radio/propagation-multi-hop-sky-waves.jpg
Radiation Angle Affects DX Performance
Fewer Hops
Attenuation Proportional to Number of Hops
Multi-Path Propagation (QSB)
http://www.wulfden.org/NVQS/PropStuff/img019.gif
Changing ionosphere location causes QSB fading
Can be caused by magnetic storms
Sporadic-E VHF Propagation
http://www.astronomie.be/radioastronomie/images/Sporadic%20E.gif
Also sometimes on 28 mHz and 144 mHz
Ionogram - Actual
FoF2
http://umlcar.uml.edu/WatchIt/latestIonogram.html
Skip Distance
MUF
FoF2
FoF2 / MUF Indicate2.5 MHz NVIS, Absorption?3.3 MHz NVIS4.6 MHz NVIS5.8 MHz 600 KM Skip7.6 MHz 1100 KM SkipE Layer Small
D LayerAbsorption
FoF1
F2
F2Multiple F2Reflections
Es Layer
Solar and Geomagnetic - Actual
http://image.slidesharecdn.com/cycle24hbarctalk-150128054239-conversion-gate02/95/cycle-24-hbarc-talk-14-638.jpg?cb=1422426843
http://www.hamqsl.com/solar101pic.php
Ionogram - Actual
http://umlcar.uml.edu/WatchIt/latestIonogram.html
E Layer
D LayerAbsorption
FoF2
MUF
Skip Distance
FoF2 / MUF Indicate2.5 MHz NVIS, Absorption Low?3.3 MHz NVIS, Absorption Low?4.6 MHz NVIS5.8 MHz NVIS7.6 MHz 900 KM SkipE Layer may cause Absorption
Es Layer
Ionogram - Actual
FoF2
http://umlcar.uml.edu/WatchIt/latestIonogram.html
MUF
FoF2 / MUF Indicate2.5 MHz NVIS, Absorption High?3.3 MHz NVIS, Absorption High?4.6 MHz NVIS, Absorption High?5.8 MHz NVIS7.6 MHz 500 KM SkipE Layer may cause AbsorptionE Layer
FoF2
F2
F2
D LayerAbsorption
Multiple F2Reflections
FxF2 Extraordinary
Es Layer
EsE
Austin not NE
Ionogram - Actual
http://umlcar.uml.edu/WatchIt/latestIonogram.html
Very FewF Layer
Reflections
Es Layer
D LayerAbsorption
Insufficient Datafor Digisondeto CalculateFoF2 and MUFE Layer may be blocking
FoF2?
MUF?
Skip Distance?
Es Layer
?
Ionogram - Actual
http://umlcar.uml.edu/WatchIt/latestIonogram.html
FoF2 / MUF Indicate2.5 MHz NVIS, Absorption High?3.3 MHz NVIS, Absorption High?4.6 MHz NVIS, Absorption High?5.8 MHz NVIS?, Short Skip, Long Skip, Some Attenuation7.6 MHz 500 KM Skip ?E Layer may cause Absorption and Short Skip
Es
EsD Layer
Absorption Multiple EsReflections
Es Layer
Es Layer
FoF2?
MUF?
Es
?
Skip Distance?
6 Meters Open?
Ionogram - Actual
http://umlcar.uml.edu/WatchIt/latestIonogram.html
FoF2 / MUF Indicate2.5 MHz NVIS, Absorption High?3.3 MHz NVIS, Absorption High?4.6 MHz NVIS, Absorption High?5.8 MHz 500 KM Skip, Short Skip, Some Attenuation7.6 MHz 1100 KM Skip ?E Layer may cause Absorption and Short Skip
Es
EsD Layer
Absorption Multiple EsReflections
Es Layer
Es Layer
FoF2
MUF
Es
Skip Distance?
Ionogram - Actual
http://umlcar.uml.edu/WatchIt/latestIonogram.html
FoF2
MUF
D LayerAbsorption
FoF2
E Layer
F2
F2Multiple
Reflections
FoF2 / MUF Indicate2.5 MHz NVIS, Absorption High?3.3 MHz NVIS, Absorption High?4.6 MHz NVIS5.8 MHz 600 SkipE Layer may cause Absorption
NVIS – Near Vertical Incident Skywave
Courtesy: Tom Carrigan / NE1R / AFA1IR
Typical NVIS RangeTypical Ground Wave Range
Ionospheric Layers
Resonant (Critical) frequency determined by electron density
http://dxc.wc2l.com/k1ttt/station/superstation_25/dvd_extras/k1ttt.net/technote/kn4lf/kn4lf8_files/ionosphereprofile.gif
Ionospheric Layers
Resonant (Critical) frequency determined by electron density
http://fas.org/man/dod-101/navy/docs/es310/propagat/IMG00024.GIF
Ionospheric Layers
http://www.electronics-radio.com/images/propagation-ionospheric-reflection-by-d-e-f-layers.svg
Ionospheric Layers
Ionospheric Layers
https://upload.wikimedia.org/wikipedia/commons/4/49/IonosphereLayers-NPS.gif
Ionospheric Layers
http://www.met.nps.edu/~psguest/EMEO_online/module3/rfig8.gif
Skywave Propagation
http://www.globalsecurity.org/intell/library/policy/army/fm/24-18/24180016.gif
NVIS when Skip Distance = 0, when F < FoF2
Sunspot Cycles
http://image.slidesharecdn.com/cycle24hbarctalk-150128054239-conversion-gate02/95/cycle-24-hbarc-talk-9-638.jpg?cb=1422426843
Sunspot Cycles
http://image.slidesharecdn.com/cycle24hbarctalk-150128054239-conversion-gate02/95/cycle-24-hbarc-talk-13-638.jpg?cb=1422426843