We have been tracking a series of low-frequency emissions originating from a non-terrestrial source, consistent with magnetar burst aftershocks. However, the modulation pattern is unlike any previously cataloged QPO. The signal strength peaks in correlation with localized atmospheric lensing events, suggesting an interaction with tropospheric ducting layers that is not predicted by current models.
Our primary array at Arecibo, even in its reduced capacity, registered a significant sidelobe anomaly during the last transit. The pattern suggested a diffraction artifact, but the geometry was inconsistent with known atmospheric or ionospheric structures. It resembled the radar cross-section of a complex, non-rigid object.
Follow-up observations using the VLA confirmed the presence of a structured, repeating signal component at 1.2 GHz. The signal is phase-locked to a secondary carrier at 430 MHz, which is a frequency band allocated for amateur radio and wind profiler radar. We are investigating the possibility of intermodulation distortion from a ground-based source, but the signal's doppler shift is inconsistent with a stationary emitter.