Presentation on theme: "Amateur Extra License Class"— Presentation transcript:
1Amateur Extra License Class Chapter 10Topics in Radio Propagation
2HF PropagationIn nearly all cases, HF waves travel along the surface of the earth or they are returned to earth after encountering the upper layers of the ionosphere.
3HF PropagationAll types of waves can change direction due to two different phenomena:Diffraction.Encountering a reflecting surface’s edge or corner.Refraction.Change in velocity due to change in properties of medium wave is traveling through.
4HF Propagation Ground Wave Special type of diffraction. Lower edge of wave (closest to the earth) loses energy due to induced ground currents.Lower edge slows, tilting wave front forward.Primarily effects vertically-polarized waves.Most noticeable on longer wavelengths.AM broadcast, 160m, & 80m.Over distance, ground wave signal is absorbed, decreasing strength.More pronounced at shorter wavelengths.Most useful during daylight on 160m & 80m.
5E3C12 -- How does the maximum distance of ground-wave propagation change when the signal frequency is increased?It stays the sameIt increasesIt decreasesIt peaks at roughly 14 MHz
6E3C13 -- What type of polarization is best for ground-wave propagation? VerticalHorizontalCircularElliptical
7HF Propagation Sky Wave Radio waves refracted in the E & F layers of the ionosphere.Maximum one-hop skip distance about 2500 miles.
8HF Propagation Sky Wave Pedersen Ray. High angle wave. Provides propagation beyond normal maximum skip distance.
9HF Propagation Sky Wave Absorption. D layer. Ionized only during sunlight.Absorbs RF energy.The longer the wavelength, the more absorption.Kills sky wave propagation on 160m & 80m during daylight hours.
10E3C08 -- What is the name of the high-angle wave in HF propagation that travels for some distance within the F2 region?Oblique-angle rayPedersen rayOrdinary rayHeaviside ray
11HF Propagation Long Path and Gray Line Long path. Radio waves travel a great-circle path between 2 stations.The path is shorter in one direction & longer in the other.The normal path is the shorter.The long path is 180° from the short path.
12HF Propagation Long Path and Gray Line Long path. A slight echo on the received may indicate that long-path propagation is occurring.With long path propagation, the received signal may be stronger if antenna is pointed 180° away from the station.Long path propagation can occur on all MF & HF bands.160m through 10m.Most often on 20m.
13HF Propagation Long Path and Gray Line Gray line propagation. At sunset, D layer collapses rapidly, reducing adsorption.F layer collapses more slowly.Similar effect occurs at sunrise.Net result is that long distance communications are possible during twilight hours on the lower frequency bands.8,000 to 10,000 miles.160m, 80m, 40m, & possibly 30m.
14HF PropagationLong Path and Gray LineGray line propagation.
15E3B04 -- What type of propagation is probably occurring if an HF beam antenna must be pointed in a direction 180 degrees away from a station to receive the strongest signals?Long-pathSporadic-ETransequatorialAuroral
16E3B05 -- Which amateur bands typically support long-path propagation? 160 to 40 meters30 to 10 meters160 to 10 meters6 meters to 2 meters
17E3B06 -- Which of the following amateur bands most frequently provides long-path propagation? 80 meters20 meters10 meters6 meters
18E3B07 -- Which of the following could account for hearing an echo on the received signal of a distant station?High D layer absorptionMeteor scatterTransmit frequency is higher than the MUFReceipt of a signal by more than one path
19E3B08 -- What type of HF propagation is probably occurring if radio signals travel along the terminator between daylight and darkness?TransequatorialSporadic-ELong-pathGray-line
20E3B09 -- At what time of day is gray-line propagation most likely to occur? At sunrise and sunsetWhen the Sun is directly above the location of the transmitting stationWhen the Sun is directly overhead at the middle of the communications path between the two stationsWhen the Sun is directly above the location of the receiving station
21E3B10 -- What is the cause of gray-line propagation? At midday, the Sun being directly overhead superheats the ionosphere causing increased refraction of radio wavesAt twilight, D-layer absorption drops while E-layer and F-layer propagation remain strongIn darkness, solar absorption drops greatly while atmospheric ionization remains steadyAt mid afternoon, the Sun heats the ionosphere decreasing radio wave refraction and the MUF
22E3B11 -- Which of the following describes gray-line propagation? Backscatter contacts on the 10 meter bandOver the horizon propagation on the 6 and 2 meter bandsLong distance communications at twilight on frequencies less than 15 MHzTropospheric propagation on the 2 meter and 70 centimeter bands
23HF Propagation Fading Variations in strength of received signals. Changes in height of ionized layers.Changes in amount of absorption.Random polarization shifts.Multi-path reflections.
24HF Propagation Fading Selective fading. Fading can have a different effect signals that are only a few hundred Hertz apart.Can cause loss of mark or space signal of RTTY transmission.Most severely affects wide-bandwidth signals such as AM or FM.Can cause moderate to severe distortion of received signal.
25E3C05 -- Which of the following describes selective fading? Variability of signal strength with beam headingPartial cancellation of some frequencies within the received pass bandSideband inversion within the ionosphereDegradation of signal strength due to backscatter
26VHF/UHF/Microwave Propagation Above 30 MHz, radio waves are rarely refracted back to earth by the ionosphere.Must use other techniques for long-distance communications.Low-angle of radiation from the antenna is more important than on HF.It is more important for polarization of transmitting & receiving antennas to match than on HF.
27VHF/UHF/Microwave Propagation Radio HorizonRadio horizon not the same as visual horizon.Refraction in the atmosphere bends radio waves & increases “line-of-sight” distance by about 15%.Visual Horizon (miles) ≈ HftRadio Horizon (miles) ≈ Hft
28VHF/UHF/Microwave Propagation MultipathRadio waves reflected off of many objects arrive at receive antenna at different times.Waves reinforce or cancel each other depending on phase relationship.Picket fencing.
29E3C06 -- By how much does the VHF/UHF radio-path horizon distance exceed the geometric horizon? By approximately 15% of the distanceBy approximately twice the distanceBy approximately one-half the distanceBy approximately four times the distance
30E3C14 -- Why does the radio-path horizon distance exceed the geometric horizon? E-region skipD-region skipDownward bending due to aurora refractionDownward bending due to density variations in the atmosphere
31VHF/UHF/Microwave Propagation Tropospheric PropagationVHF/UHF propagation normally limited to 500 miles.Certain atmospheric conditions can create a “duct” where radio waves can travel for hundreds or thousands of miles.Bands:6m – Rare.2m – Fairly common.70cm – Common.
33E3C09 -- Which of the following is usually responsible for causing VHF signals to propagate for hundreds of miles?D-region absorptionFaraday rotationTropospheric ductingGround wave
34VHF/UHF/Microwave Propagation Transequatorial PropagationCommunications between stations located an equal distance north & south of the magnetic equator.
35VHF/UHF/Microwave Propagation Transequatorial PropagationMost prevalent around the spring & autumn equinoxes.Maximum effect during afternoon & early evening.Allows contacts up to about 5,000 miles.Useable up to 2m & somewhat on 70cm.As frequency increases, paths more restricted to exactly equidistant from and perpendicular to the magnetic equator.
36E3B01 -- What is transequatorial propagation? Propagation between two mid-latitude points at approximately the same distance north and south of the magnetic equatorPropagation between any two points located on the magnetic equatorPropagation between two continents by way of ducts along the magnetic equatorPropagation between two stations at the same latitude
37E3B02 -- What is the approximate maximum range for signals using transequatorial propagation? 1000 miles2500 miles5000 miles7500 miles
38E3B03 -- What is the best time of day for transequatorial propagation? MorningNoonAfternoon or early eveningLate at night
41VHF/UHF/Microwave Propagation Auroral PropagationCharged particles from the sun (solar wind) are concentrated over the magnetic poles by the earth’s magnetic field & ionize the E-layer.VHF & UHF propagation up to about 1,400 miles.
42VHF/UHF/Microwave Propagation Auroral PropagationReflections change rapidly.All signals sound fluttery.SSB signals sound raspy.CW signals sound like they are modulated with white noise.CW most effective mode.Point antenna toward aurora, NOT towards station.In US, point antenna north.
43E3C01 -- Which of the following effects does Aurora activity have on radio communications? SSB signals are raspySignals propagating through the Aurora are flutteryCW signals appear to be modulated by white noiseAll of these choices are correct
44E3C02 -- What is the cause of Aurora activity? The interaction between the solar wind and the Van Allen beltA low sunspot level combined with tropospheric ductingThe interaction of charged particles from the Sun with the Earth’s magnetic field and the ionosphereMeteor showers concentrated in the northern latitudes
45E3C03 -- Where in the ionosphere does Aurora activity occur? In the F1-regionIn the F2-regionIn the D-regionIn the E-region
46E3C04 -- Which emission mode is best for Aurora propagation? SSBFMRTTY
47E3C11 -- From the contiguous 48 states, in which approximate direction should an antenna be pointed to take maximum advantage of aurora propagation?SouthNorthEastWest
48VHF/UHF/Microwave Propagation Meteor Scatter CommunicationsMeteors passing through the ionosphere collide with air molecules & strip off electrons.Ionization occurs at or near the E-region.Best propagation 28 MHz to 148 MHz.20 MHz to 432 MHz possible.
49VHF/UHF/Microwave Propagation Meteor Scatter CommunicationsMajor meteor showers.Quadrantids January 3-5.Lyrids – AprilArietids – June 8.Aquarids – JulyPerseids – July 27 to August 14.Orionids – OctoberTaurids – October 26 to November 16.Leonids – NovemberGeminids – DecemberUrsids – December 22.
50VHF/UHF/Microwave Propagation Meteor Scatter CommunicationsOperating techniques.Keep transmissions SHORT.Divide each minute into four 15-second segments.Stations at west end of path transmit during 1st & 3rd segments.Stations at east end of path transmit during 2nd & 4th segments.
51VHF/UHF/Microwave Propagation Meteor Scatter CommunicationsOperating techniques.Modes:HSCW.800-2,000 wpm.Computer generated & decoded.FSK441 (part of WSJT software suite).Repeated short bursts of data.
52E3A08 -- When a meteor strikes the Earth's atmosphere, a cylindrical region of free electrons is formed at what layer of the ionosphere?The E layerThe F1 layerThe F2 layerThe D layer
53E3A09 -- Which of the following frequency ranges is well suited for meteor-scatter communications? MHzMHzMHzMHz
54E3A10 -- Which of the following is a good technique for making meteor-scatter contacts? 15 second timed transmission sequences with stations alternating based on locationUse of high speed CW or digital modesShort transmission with rapidly repeated call signs and signal reportsAll of these choices are correct
55VHF/UHF/Microwave Propagation Earth-Moon-Earth (EME) Communications.a.k.a. – Moon bounce.If both stations can “see” the moon, they can talk.Maximum about 12,000 miles.Best when moon is at perigee.2 dB less path loss.Not useable near new moon.Increased noise from the sun.The higher the moon is in the sky the better.
56VHF/UHF/Microwave Propagation Earth-Moon-Earth (EME) Communications.Low receiver noise figure essential.Libration Fading.Caused by multipath effects of rough moon surface in combination with relative motion between the earth and the moon.Rapid, deep, irregular fading.20 dB or more.Up to 10 Hz.Can cause slow-speed CW to sound like high-speed CW.
57VHF/UHF/Microwave Propagation Earth-Moon-Earth (EME) Communications.2m operation.MHz to MHz.2-minute schedule.Transmit for 2 minutes.Receive for 2 minutes.Station farthest east transmits first then station to the west.
58VHF/UHF/Microwave Propagation Earth-Moon-Earth (EME) Communications.70cm operation.MHz to MHz.2.5-minute schedule.Transmit for 2.5 minutesReceive for 2.5 minutes.Station farthest east transmits first then station to the west.
59E3A01 -- What is the approximate maximum separation measured along the surface of the Earth between two stations communicating by Moon bounce?500 miles, if the Moon is at perigee2000 miles, if the Moon is at apogee5000 miles, if the Moon is at perigee12,000 miles, as long as both can “see” the Moon
60E3A02 -- What characterizes libration fading of an Earth-Moon-Earth signal? A slow change in the pitch of the CW signalA fluttery irregular fadingA gradual loss of signal as the Sun risesThe returning echo is several Hertz lower in frequency than the transmitted signal
61E3A03 -- When scheduling EME contacts, which of these conditions will generally result in the least path loss?When the Moon is at perigeeWhen the Moon is fullWhen the Moon is at apogeeWhen the MUF is above 30 MHz
62E3A04 -- What type of receiving system is desirable for EME communications? Equipment with very wide bandwidthEquipment with very low dynamic rangeEquipment with very low gainEquipment with very low noise figures
63E3A05 -- Which of the following describes a method of establishing EME contacts? Time synchronous transmissions with each station alternatingStoring and forwarding digital messagesJudging optimum transmission times by monitoring beacons from the MoonHigh speed CW identification to avoid fading
64E3A06 -- What frequency range would you normally tune to find EME signals in the 2 meter band? MHzMHzMHzMHz
65E3A07 -- What frequency range would you normally tune to find EME signals in the 70 cm band? MHzMHzMHzMHz