RESEARCH BASE

Search 3,721 documents across 34 fields — every claim tier-rated by evidence

3,721 Documents 34 Sections 43,625 Citations 34,852 Keywords Indexed 4 Evidence Tiers

3,633 are the core, quality-scored corpus (34 lettered sections — see How We Work); the remaining 88 are cross-corpus synthesis documents (68 InterDocs, 12 Connections, 8 Theories) also indexed here.

6 results for "dipole"

E_4_23 Verified Cataclysms & Chronology

E_4_23 — Magnetic Field Strength History: Dipole Decay and Implications

Earth's magnetic field — generated by convective motion of liquid iron in the outer core (the geodynamo) — is not constant in strength. Over the past ~170 years of direct measurement (since Carl Friedrich Gauss's first s

geomagnetic field dipole moment paleointensity archaeointensity VADM field strength
Q_1_22 Credible Cosmology & Physics

Q_1_22 — Dark Flow and Cosmic Dipole Anomalies

Dark flow refers to a claimed coherent bulk motion of galaxy clusters toward a specific region of the sky at velocities inconsistent with the predictions of standard ΛCDM cosmology, first reported by NASA Goddard astroph

dark flow bulk flow cosmic dipole CMB anisotropy Kashlinsky
E_4_19 Verified Cataclysms & Chronology

E_4_19 — Mono Lake and Gothenburg Excursions: Short Geomagnetic Events

Geomagnetic excursions are brief, extreme departures of the Earth's magnetic field from its normal dipolar configuration — events during which the virtual geomagnetic pole (VGP) deviates by more than 40–45° from the geog

geomagnetic excursion Mono Lake Gothenburg Laschamp paleomagnetic virtual geomagnetic pole
Q_1_08 Verified Cosmology & Physics

Q_1_08 — Observable Universe and Cosmic Web

The observable universe has a diameter of ~93 billion light-years (comoving distance) and contains an estimated 2 trillion galaxies (Conselice et al. 2016), ~10²⁴ stars, and ~10⁸⁰ atoms. But its most striking feature is

cosmic web large-scale structure filament void supercluster Laniakea
Q_1_07 Verified Cosmology & Physics

Q_1_07 — CMB Anomalies and the Axis of Evil

The Cosmic Microwave Background (CMB) — the afterglow of the Big Bang, emitted ~380,000 years after the universe began — is the most precisely measured radiation in the history of science. It matches the theoretical pred

CMB cosmic microwave background WMAP Planck anisotropy anomaly
ZA_3_10 Verified Physics & Quantum

ZA_3_10 — Muon Anomalous Magnetic Moment

The anomalous magnetic moment of the muon ($a_\mu = (g-2)/2$) is one of the most precisely measured quantities in particle physics and one of the most sensitive probes for physics beyond the Standard Model. Every charged

muon g-2 anomalous magnetic moment g minus 2 Fermilab Brookhaven Standard Model