Amateur Radio Operators Invited to participate in Asteroid Bounce Experiment

ARRL – The High-frequency Active Auroral Research Program (HAARP) will be conducting a research campaign/experiment on December 27, 2022, with transmissions between 1100 – 2300 UTC (0200 – 1400 AKST).

This experiment will reflect HAARP transmissions off of Near-Earth Asteroid (NEA) 2010 XC15, and the echo will be received by the Owens Valley Radio Observatory Long Wavelength Array (OVRO-LWA) at the California Institute of Technology (Caltech) and by the University of New Mexico’s Long Wavelength Array (UNM-LWA). The target asteroid will be roughly two lunar distances away from Earth at the time of transmission. Characterizing the interior structure and composition of NEAs is critical for advancing the understanding of solar system evolution and aiding in planetary defense.

Actual transmit times are highly variable based on real-time ionospheric conditions and all information is subject to change. Currently, the Asteroid Bounce (2010 XC15) experiment will take place Dec. 27, 2022, from 1100 UTC to 2300 UTC; 9.6 MHz, LFM (linear FM), 0.5 Hz WRF (waveform repetition frequency), 30 kHz bandwidth. Reports recording echo are encouraged; demodulated recordings in .wav or .mp3 are recommended.

For real-time ionospheric conditions in Gakona, please consult ionograms from the HAARP Diagnostic Suite at https://haarp.gi.alaska.edu/diagnostic-suite.

Amateur radio and radio astronomy enthusiasts are invited to listen to the transmissions/echoes and submit reception reports to the HAARP facility at [email protected] and request a QSL card by mailing a report to:

HAARP
P.O. Box 271
Gakona AK 99586
USA

HAARP to Use WSPR on 80 Meters

ARRL – Alaska’s super-power High-Frequency Active Auroral Research Program (HAARP) transmitters in Gakona, Alaska, will take advantage of the WSPR digital protocol and the Weak Signal Propagation Reporter Network (WSPRnet) during a short experimental campaign, July 30 through August 1. University of Alaska Fairbanks (UAF) Space Physics Group researcher and HAARP Chief Scientist Chris Fallen, KL3WX, told ARRL that he’ll be conducting research into ionospheric irregularities, but hardly with a weak signal.

“I am conducting a dual-use experiment to create field-aligned — plasma density — irregularities while also modulating the HF beam for a WSPR beacon test,” he said. Specifically, Fallen will be looking at plasma density irregularities in the F-layer of the ionosphere.

Fallen said the WSPR experimental periods are tentatively planned to last about 30 minutes per day and occur between approximately 2300 and 2400 hours UTC on all 3 days, which would put the operations during daylight hours in US time zones. Most transmissions will be at the WSPR 80-meter default frequency of 3.592.6 MHz, Fallen said. HAARP will use full-carrier AM, since it’s not equipped to transmit SSB. The call sign will be WI2XFX. The HAARP transmitters can generate megawatts of RF.

“One irregularity is that the actual transmit power will be higher than what is reported since it is out of range of what the software allows to be encoded,” Fallen told ARRL.

“These daytime 80-meter conditions are not ideal for a propagation test, but are the result of a compromise with other science objectives and operational constraints,” Fallen said. “I hope that this will be a useful trial for future propagation tests that utilize beacon networks maintained by hams. If I have a little bit of time remaining in my budget, I will try to accommodate a 40-meter test as well.”

Fallen said he’s using WSPRnet to retrieve signal reports automatically, rather than by soliciting listener reports, which often do not include the location and signal strength information his research requires.

“We will conduct a short test each day — admittedly not QRP, but the test will be short — transmitting on even numbered minutes, and then later collecting from the database the spots reported by each station that received HAARP,” Fallen explained. “This will demonstrate the concept of using a large and incredibly variable — in terms of frequency, power, and direction — HF transmitter such as HAARP, in conjunction with WSPRnet, to generate snapshots of HF propagation conditions from a point source in the subarctic.”

Fallen said hams have been requesting something like this, although with far more asking for FT8 than for WSPR transmissions. “But, I am having trouble figuring out specifically how FT8 would work with HAARP,” Fallen said.

Fallen said the Amateur Radio bands are not included in HAARP’s permanent Part 5 Experimental license authorization, but UAF routinely seeks a Special Temporary Authorization (STA, attached) that permits access to some amateur frequencies.