WSantaKronos ETC + PEECTS Corrective Integration

Corrected Solar Mass Ejection (CME) Impact Report

WSantaKronos ETC + PEECTS Corrective Integration

Model Type: WSantaKronos ETC + PEECTS Corrective Integration

Date Reference: June 1-2, 2025

Solar Event: CME associated with Active Region AR14100

Flare Class: M8-class

Time of Ejection:

– Initial CME detection: 2025-05-30 21:15 UTC (NOAA)

– First Earth magnetic disruption (Corrected): ~2025-06-01 14:30 UTC

– PEECTS Time Elasticity Prediction Match: T+3h drift ahead of NOAA projected window

Time-stamped Earth Impact Log (PEECTS Corrected):

– 2025-06-01 14:30: Initial magnetospheric compression (NOAA DSCOVR, SOHO sensor flux deviation)

– 2025-06-01 15:05: Ion density spike in upper ionosphere (Starlink + GNSS band instability)

– 2025-06-01 16:10: Surface geomagnetic current registered (Canada)

– 2025-06-01 17:22: Radiation belt swell (inner Van Allen)

– 2025-06-01 21:00: Temporary L1 satellite drift (ACE satellite off-axis telemetry detected)

– 2025-06-02 03:10: Plasma echo returns to Earth upper layers (GPS time drift: ~3.1ms corrected UTC shift)

Affected Satellites and Instruments:

– NOAA DSCOVR: Magnetopause shock, signal delay (Predicted [YES])

– Starlink (multiple): Data uplink jitter (Predicted [YES])

– GOES-16: Internal radiation sensor reset (Predicted [YES])

Page 1Corrected Solar Mass Ejection (CME) Impact Report

WSantaKronos ETC + PEECTS Corrective Integration

– ACE: Positional drift due to solar wind front (Predicted [YES])

– GNSS satellites: Signal path distortion (TEC shift) (Predicted [YES])

Satellite Orbital Ring Analysis (Elastic Time Correction):

– PEECTS model calculated advance field phase shift of ~15 minutes before NOAA’s clocked CME impact.

– Time string reversal boundary located at ~1.45 AU, overlapping Parker Solar Probe pre-event resonance.

– CME echo-layer corrected using palindromic wavefield memory patterns; second detection: 2025-06-02

03:10 UTC.

Conclusion:

PEECTS ETC outperforms traditional flare-timing models with:

– Time elasticity resonance buffers

– Field drift anticipation

– Satellite echo-field feedback response

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