What is the direction of an ascending pass for an amateur satellite?
An ascending satellite pass is one in which the satellite crosses the equator traveling northward, so its ground track is generally from south to north.
Amateur Extra · correct answers only, in question-pool order.
An ascending satellite pass is one in which the satellite crosses the equator traveling northward, so its ground track is generally from south to north.
The official E2A02 source identifies opposite-direction uplink and downlink Doppler shifts as a characteristic of an inverting linear transponder.
The official E2A02 source states that an inverting transponder reverses the spectral position of signals across its passband.
The official E2A02 source identifies sideband reversal as a characteristic of an inverting linear transponder.
An inverting linear transponder mixes the received uplink with a local oscillator and transmits the difference product, reversing the spectral order.
A satellite's operating mode identifies the frequency bands used for its uplink and downlink.
The letters in a satellite mode designator specify the uplink and downlink frequency ranges.
Keplerian elements are the orbital parameters used to describe and predict the position of a satellite.
The official E2A07 source includes FM and CW among the signal types a linear transponder can relay.
The official E2A07 source includes SSB and SSTV among the signal types a linear transponder can relay.
The official E2A07 source includes PSK and packet among the signal types a linear transponder can relay.
A linear transponder has limited total RF output power. One excessively strong uplink can consume too much of that shared power and reduce downlink power available to other users.
In amateur satellite terminology, L band corresponds to 23 centimeters and S band to 13 centimeters.
A geostationary satellite orbits at the same angular rate as Earth over the equator, so it appears fixed at one point in the sky.
Circular polarization reduces fading caused by satellite spin and by Faraday rotation because reception is less dependent on the instantaneous orientation of a linear polarization.
Store-and-forward systems hold uploaded digital messages in satellite memory so they can be downloaded later when another station is in range.
A coding rate of 3/4 means three quarters of the transmitted bits carry payload information and one quarter is forward-error-correction overhead.
The NTSC fast-scan television standard uses 525 horizontal lines per frame.
Interlaced NTSC scanning divides a frame into two fields: one scans the odd-numbered lines and the other scans the even-numbered lines.
In analog SSTV, the color components are sent as sequential color lines rather than as a conventional television color subcarrier.
Vestigial-sideband television transmits one full sideband and only part of the other, reducing bandwidth while preserving low-frequency video detail.
Vestigial sideband is amplitude modulation with one complete sideband plus a small portion, or vestige, of the other sideband.
Amateur DVB-T television uses QAM and QPSK modulation schemes.
Some 70-centimeter amateur fast-scan TV frequencies correspond to channels used by cable television, allowing suitable commercial analog TV receivers to tune them directly.
Digital Radio Mondiale SSTV can be received and decoded using an SSB receiver feeding the appropriate digital decoder.
In analog SSTV, picture brightness is represented by tone frequency.
The VIS code identifies which SSTV mode is being transmitted so receiving software can select the proper timing and format.
SSTV software recognizes specific synchronization tone frequencies as the signal to begin a new picture line.
A US-licensed operator remotely controlling a transmitter located in the United States does not need to add any special remote-operation indicator to the call sign.
ADIF, the Amateur Data Interchange Format, is a standard file format used to exchange amateur radio log data between programs and services.
Amateur contesting is generally avoided on 30 meters.
Amateur mesh networks commonly operate on amateur frequencies that overlap spectrum used by unlicensed wireless data services.
A DX QSL Manager receives and sends contact confirmations on behalf of a DX station.
During VHF/UHF contests, most CW and SSB activity is found in the weak-signal portion of each band, clustered near the established calling frequencies.
Cabrillo is the standard electronic format used to submit contest logs.
The official E2C08 source lists US special-event contacts among those that may be confirmed through LoTW.
The official E2C08 source lists international contacts among those that may be confirmed through LoTW.
The official E2C08 source lists Worked All States contacts among those that may be confirmed through LoTW.
Amateur mesh networks are commonly built from wireless routers loaded with custom amateur-oriented firmware.
The official E2C10 source identifies differing frequency privileges as one reason DX stations use split operation.
The official E2C10 source identifies physical separation of callers from the DX transmitting frequency as a reason for split operation.
The official E2C10 source identifies reduced interference and improved efficiency as a reason DX stations transmit and receive on different frequencies.
In a DX pileup or contest, sending the full call sign once or twice is the clearest and most efficient way to identify yourself.
Latency is the delay between a control action and the corresponding change at the remotely controlled transmitter.
MSK144 is designed specifically for high-speed weak-signal meteor-scatter communication.
In VHF contests using FT8 or FT4, the exchanged location information is the Maidenhead grid square rather than a signal-to-noise report.
Q65 is designed for extremely weak-signal paths such as Earth-Moon-Earth communication.
APRS can transmit real-time position reports from balloon-borne amateur stations for tracking.
JT65 can decode signals at very low signal-to-noise ratios, which made it useful for weak-signal work such as EME.
EME contacts commonly use precisely timed transmit and receive periods, with the two stations alternating so they are not transmitting simultaneously.
APRS beacon information is carried in AX.25 Unnumbered Information frames, commonly called UI frames.
JT65 uses multiple audio-frequency tones, making it a multitone AFSK mode.
WIDE3-1 means the path originally requested up to three wide-area digipeater hops and one hop remains unused.
APRS stations relay packets through packet digipeaters.
FSK is an authorized and commonly used modulation method for data emissions below 30 MHz.
WSJT-X modes rely on accurately synchronized computer clocks so stations transmit and receive in the correct time slots.
The '4' in FT4 refers to its four-tone continuous-phase frequency-shift keying modulation.
The official E2E04 source identifies four-tone Gaussian frequency shift keying as an FST4 characteristic.
The official E2E04 source identifies variable transmit/receive periods as an FST4 characteristic.
The official E2E04 source identifies seven available tone spacings as an FST4 characteristic.
WSPR is intended for automated weak-signal propagation reporting rather than live keyboard-to-keyboard conversations.
An FT8 transmission cycle is 15 seconds long, with stations alternating between synchronized time slots.
Q65 differs from JT65 by averaging multiple receive cycles, improving recovery of very weak or varying signals.
PACTOR supports robust connected data transfer and can carry binary files over HF.
PSK31 uses Varicode, a variable-length character coding system.
Among the listed modes, FT8 has the narrowest occupied bandwidth.
Direct FSK changes the transmitter's VFO or carrier frequency directly, while audio FSK sends tones through an SSB transmitter.
Automatic Link Establishment scans a programmed list of frequencies and responds when the station's designated call sign is received.
PACTOR IV provides the highest data throughput of the listed HF digital modes under clear communication conditions.