_WSJT-X_ v1.7 introduces a number of new features designed for use on the VHF and higher bands. These features now include: - *JT4*, a mode particularly useful for EME on the microwave bands - *JT9* fast modes, useful for scatter propagation on VHF bands - *QRA64*, a mode for EME using a "`Q-ary Repeat Accumulate`" code, a low-density partity-check (LDPC) code using a 64-character symbol alphabet - *MSK144*, a mode for meteor scatter using a binary LDPC code and Offset Quadrature Phase-Shift Keying (OQPSK). The resulting waveform is sometimes called Minimum Shift Keying (MSK). - *ISCAT*, intended for aircraft scatter and other types of scatter propagation - *Echo* mode, for detecting and measuring your own lunar echoes - *Doppler tracking*, which becomes increasingly important for EME on bands above 1.2 GHz. - *Auto-sequencing* of transmitted messages for the fast modes with forward error control [[VHF_SETUP]] === VHF Setup To activate the VHF-and-up features: - Check *Enable VHF/UHF/Microwave features* and *Single decode* on the *Settings | General* tab. - For EME, check *Decode at t = 52 s* to allow for the extra path delay on received signals. - If you will use automatic Doppler tracking and your radio accepts frequency-setting commands while transmitting, check *Allow Tx frequency changes while transmitting*. Transceivers known to permit such changes include the IC-735, IC-756 Pro II, IC-910-H, FT-817, FT-847, FT-857, FT-897, TS-590S, TS-590SG, TS-2000 (with Rev 9 or later firmware upgrade), Flex 1500 and 5000, HPSDR, Anan-10, Anan-100, and KX3. IMPORTANT: If your radio does not accept commands to change frequency while transmitting, Doppler tracking will be approximated by making a single Tx frequency adjustment before a transmission starts, using a value computed for the middle of the Tx period. - On the *Radio* tab select *Split Operation* (use either *Rig* or *Fake It*; you may need to experiment with both options to find one that works best with your radio). - Select *Tab 1* to present the traditional format for selecting Tx messages. The main window will reconfigure itself as necessary to display controls supporting the features of each mode. - If you are using transverters, set appropriate frequency offsets on the *Settings | Frequencies* tab. Offset is defined as (transceiver dial reading) minus (on-the-air frequency). For example, when using a 144 MHz radio at 10368 MHz, *Offset (MHz)* = (144 - 10368) = -10224.000. If the band is already in the table, you can edit the offset by double clicking on the offset field itself. Otherwise a new band can be added by right clicking in the table and selecting *Insert*. image::Add_station_info.png[align="center",alt="Station information"] - On the *View* menu, select *Astronomical data* to display a window with important information for tracking the Moon and performing automatic Doppler control. The right-hand portion of the window is invisible until you check *Doppler tracking*. image::Astronomical_data.png[align="center",alt="Astronomical data"] Three different types of Doppler tracking are provided: - Select *Full Doppler to DX Grid* if you know your QSO partner's locator and he/she will not be using any Doppler control. - Select *Receive only* to enable EME Doppler tracking of your receive frequency to a specific locator. Your Tx frequency will remain fixed. - Select *Constant frequency on Moon* to correct for your own (one-way) Doppler shift to or from the Moon. If your QSO partner does the same thing, both stations will have the required Doppler compensation. Moreover, anyone else using this option will hear both of you without the need for manual frequency changes. === JT4 JT4 is highly effective for EME on the microwave bands, 2.3 GHz and above. - Select *JT4* from the *Mode* menu. The central part of the main window will look something like this: image::VHF_controls.png[align="center",alt="VHF Controls"] - Select the desired *Submode*, which determines the spacing of transmitted tones. Wider spacings are used on the higher microwave bands to allow for larger Doppler spreads. For example, submode JT4F is generally used for EME on the 5.7 and 10 GHz bands. - For EME QSOs some operators use short-form JT4 messages consisting of a single tone. To activate automatic generation of these messages, check the box labeled *Sh*. - Select *Deep* from the *Decode* menu. You may also choose to *Enable averaging* over successive transmissions and/or correlation decoding, *Enable deep Search*. image::decoding_depth.png[align="center",alt="Decoding Depth"] IMPORTANT: Additional hints for using JT4 and Echo mode on the EME path have been compiled by G3WDG and are available here: {jt4eme}. === JT65 In most ways JT65 operation on VHF and higher bands is similar to HF usage. However, a few differences should be noted. Typical VHF/UHF operation involves only a single signal in the receiver passband, or perhaps a few, rather than many. Normally it's best to check *Single decode* on the *Settings -> General* tab and uncheck *Two pass decoding* on the *Advanced* tab. In this mode the JT65 decoder will respond to special message formats sometimes used for EME, including the OOO signal report and shorthand messages for RO, RRR, and 73. Those messages will be automatically generated if you check the shorthand message box *Sh*. As for JT4, you should check *Deep* on *the *Decode* menu, and optionally *Enable averaging* and *Deep search*. === QRA64 QRA64 is an experimental mode in the present alpha release of _WSJT-X_, Version 1.7. The protocol is still subject to change, and some features of the decoder will likely change. In most ways operation of QRA64 is similar to JT65. === Meteor Scatter with MSK144 Meteor-scatter QSOs can be made at any time on the VHF bands, at distances up to about 2100 km or 1300 miles. Completing a QSO takes longer in the evening than in the morning, longer at 144 MHz than at 50 MHz, and longer at 2000 km than 1500 km. But with patience, at least 100 Watts, and a single yagi it can usually be done. - Select *MSK144* from the *Mode* and *Fast* from the *Decode* menu. - Set the audio receiving frequency to *Rx 1500 Hz*, frequency tolerance to *F Tol 100*, and T/R sequence duration to 15 s. - MSK144 decodes received signals in real time, so you will see decoded messages almost as soon as you hear them. To match decoding depth to your computer's capability, click *Monitor* (if it's not already green) to start a receiving sequence and observe the percentage of CPU usage displayed on the _Receiving_ label in the Status Bar: image::Rx_pct_MSK144.png[align="center",alt="MSK144 Percent CPU"] - The displayed number (here 17%) indicates the fraction of CPU capability used being used by the MSK144 real-time decoder. If it is well below 100% you may increase the decoding depth from *Fast* to *Normal* or *Deep*, and increase *F Tol* from 100 to 200 Hz. IMPORTANT: Most modern multi-core computers can easily handle the optimum parameters *Deep* and *F Tol 200*. Slower machines may not be able to keep up at these settings; in that case there will be a modest loss in decoding capability for the weakest pings. - T/R sequences of 15 seconds or less make it sometimes desirable to advance your selection of transmitted messages very quickly. Check *Auto Seq* to have the computer make the necessary decisions automatically, based on received messages. - For operation at 144 MHz or above it is advantageous to use the short-format messages for Tx3, Tx4, and Tx5. Check the box labeled *Sh* to enable this feature. IMPORTANT: There is little need to use MSK144 *Sh* messages at 50 or 70 MHz, where most pings are long enough to support the standard MSK144 message length. === Scatter Propagation with ISCAT TBD ... === Echo Mode *Echo* mode allows you to make sensitive measurements of your own lunar echoes even when they are too weak to be heard. Select *Echo* from the *Mode* menu, aim your antenna at the moon, pick a clear frequency, and toggle click *Tx Enable*. _WSJT-X_ will then cycle through the following loop every 6 seconds: 1. Transmit a 1500 Hz fixed tone for 2.3 s 2. Wait about 0.2 s for start of the return echo 3. Record the received signal for 2.3 s 4. Analyze, average, and display the results 5. Repeat from step 1 To make a sequence of echo tests: - Select *Echo* from the *Mode* menu. - Check *Doppler tracking* and *Constant frequency on the Moon* on the Astronomical Data window. - Be sure that your rig control has been set up for _Split Operation_, using either *Rig* or *Fake It* on the *Settings | Radio* tab. - Click *Enable Tx* on the main window to start a sequence of 6-second cycles. - _WSJT-X_ calculates and compensates for Doppler shift automatically. Your return echo should always appear at the center of the plot area on the Echo Graph window, as in the screen shot below. image::echo_144.png[align="center",alt="Echo 144 MHz"]