engineering text speculative

Step-by-Step Observation Protocol: How to Search for Sirius Signals Tonight

OBSERVATION PROTOCOL

STEP 1: LOCATE SIRIUS

Coordinates:

Right Ascension: 06h 45m 08.9s
Declination: -16° 42' 58.0"

Visual: Follow Orion's belt down-left to the

BRIGHTEST star in the sky. That's Sirius.

Software: Use Stellarium (free) to confirm. Best months: December through March. Best time: when Sirius is highest in your sky

(transit time varies by date and latitude).

STEP 2: SET UP HYDROGEN LINE RECEIVER

Connect: Dish → LNA → (filter) → RTL-SDR → USB Point dish at Sirius (use Stellarium for azimuth

and elevation from your location).

Open SDR# or GNU Radio. Tune to 1420.405MHz. Set bandwidth: 250kHz (to see context). Set FFT size: 65536 or higher (for resolution). Set integration time: 60 seconds minimum.

FIRST: Verify your system works by pointing at

the Milky Way. You should see the hydrogen line
peak. If you see it: your telescope works.

STEP 3: HIGH-RESOLUTION SPECTRAL ANALYSIS

Now the critical part: Narrow your analysis window to ±100Hz around

1420.40575MHz.

Use FFT with very high resolution (0.1-1Hz bins). This requires long integration: 10+ seconds per

FFT frame, averaged over 1-24 hours.

Record raw IQ data to disk for offline analysis.

WHAT TO LOOK FOR:

Sidebands at ±7.83Hz from center frequency.
Additional peaks at ±14.3, ±20.8, ±27.3Hz.
Peaks should be narrow (<1Hz) and evenly spaced.
Compare ON-source (Sirius) vs OFF-source
(adjacent sky). Signal should appear ONLY
when pointed at Sirius.

STEP 4: CROSS-CORRELATE WITH SCHUMANN

Run ELF receiver simultaneously. Measure local Schumann resonance peaks. Cross-correlate: do the 1420MHz sidebands

MATCH the Schumann frequencies?

If yes AND the signal is only from Sirius direction:

→ DETECTION CANDIDATE.

Repeat on multiple nights to confirm.

Submitted by Engineering Design — Detector Build June 06, 2026

Related claims

No claims cite this entry yet.