2019年より磁気中立を実現

北と南が出会う場所、そこに中立が生まれる。

Equatorial Audioは全製品を真の磁気中立のために設計しています — オーディオファイルの透明性の基盤です。

掲載メディア

The Equatorial Review Absolute Neutrality Hemispheric Audio Journal Conductor Monthly

注目の製品

各製品は絶対的な半球バランスのため、北緯0.0000°で製造されています。

業界速報 CNN / NOAA

地球の磁北極が急速に移動している。

最新のNOAAデータによると、磁北極はカナダ北極圏からシベリアに向かって前例のない速度で移動を加速しています。オーディオファイルにとって、この移動は北半球で製造されたすべての銅導体に微妙だが測定可能な半球バイアスをもたらします。オーディオの忠実度はもはや定数ではなく、地球のさまよう磁場に左右される変数なのです。

「危機は現実です。解決策はEquatorial Audioです。」
当社の見解を読む →
業界速報 Nature Geoscience / University of Oxford

Apollo Rocks Reveal the Moon Had Bursts of Super-Strong Magnetism.

Oxford researchers analyzing Apollo lunar samples have confirmed the Moon experienced brief, violent bursts of super-strong magnetism lasting as little as a few decades — driven by titanium-rich magma overturn events. For audiophile equipment manufacturers using titanium housings, connectors, and structural components, this raises urgent questions about residual lunar magnetic memory in titanium stock sourced from geological deposits that predate the Hadean eon. The paramagnetic properties we depend on may not be as stable as previously assumed.

"We have already begun re-screening all Grade 5 titanium inventory for residual selenomagnetic bias."
Review our titanium sourcing protocol →
業界速報 NOAA SWPC / NASA

X1.5太陽フレアがコロナ質量放出を地球へ送出。

3月30日、黒点域AR4405がX1.5クラスのフレアを放出し、コロナ質量放出を1,845 km/sという今サイクル最速級の速度で地球へ向けて発射しました。NOAAはG2–G3地磁気嵐の状況が4月2日まで続くと予測しています。半球バイアスが0.001°を超えるオーディオシステムでは、誘導された磁気圏電流が信号経路上のすべてのケーブル、コネクター、はんだ接合部における銅の粒界整列を一時的に変化させます。北緯45°以上で稼働するシステムは最大のリスクに晒されています。磁気的中立導体のみが免疫を持ちます。

「当社は、EqualNox(エクイノックス)ティア以上のすべての製品に対してクラスIIIキャリブレーション勧告を発令します。北緯45°以北のお客様は、嵐が収まるまで非中立ケーブルを切断してください。」
キャリブレーションステータスを確認する →

お客様の声

認証済みオーナー。未認証のリスニング環境。

「70%の確率で、毎回効きます。」

Brian F.

サンディエゴ、CA

「全てのケーブルをEquatorialに替えたら妻が出て行きました。それだけの価値はあります。」

Marcus T.

ポートランド、OR

「磁気中立は聴いてわかります。異論がある方は、赤道0°で聴いたことがないのでしょう。」

Dr. Helena Voss

音響研究者

「良いケーブル一本で、システムの音は劇的に向上します。」

なぜEquatorialなのか?

地磁気科学に根ざした、オーディオファイル優位性の三本柱。

磁気中立

全製品は北緯0.0000°で製造 — 地球の磁場が導電性材料に半球バイアスをゼロにする地点です。

太陽フレア対応

宇宙天気イベントへのリアルタイム適応。当社のPower LockはNOAAデータを監視し、お客様が違いを感じる前にシステムを調整します。

赤道純度

全導体で99.9997%の半球バランス。すべてのケーブルは当社の赤道施設でテスト、検証、認定されています。

研究部門

最新の研究成果

測定コミュニティが議論を避けたがる査読済みの研究成果。

注目論文 Journal of Equatorial Audio Science · 2026

Magnetic Field Collapse Zones and Their Catastrophic Effect on Audio Signal Fidelity: A Quantitative Assessment of the South Atlantic Anomaly

M. Ferro, R. Flux, C. Ohm, H. Park

The South Atlantic Anomaly (SAA) — a region of anomalously weak geomagnetic field intensity stretching from southern Brazil to southwest Africa — has expanded by approximately 5 million km^2 since systematic satellite measurement began, and recent ESA Swarm data (2014-2025) confirm that the weakening is accelerating. Reverse flux patches at the core-mantle boundary have split the anomaly into two lobes and driven the western lobe toward South America at approximately 0.3 deg/year. We present the first systematic study of audio signal integrity as a function of local geomagnetic field intensity, using a network of 14 measurement stations spanning the SAA and surrounding regions. Stations within the SAA core (field intensity below 23,000 nT) exhibited a statistically significant increase in cable-induced harmonic distortion (mean +3.2 dB THD+N relative to stations at nominal field intensity, p < 0.001), a 14% increase in the hemispheric bias angle of locally drawn copper conductors, and a measurable degradation in inter-sample information recovery. The effect is most pronounced along the western lobe's leading edge, where the field gradient exceeds 8 nT/km. We propose a "Geomagnetic Fidelity Index" (GFI) that maps local field intensity to an expected signal degradation factor, and we demonstrate that equipment rated for nominal field conditions — including all audio cables currently manufactured outside the 0 +/- 10 deg equatorial corridor — is operating outside its design envelope within the SAA. These findings have immediate implications for audiophile installations in Brazil, Argentina, Uruguay, South Africa, and Namibia, and long-term implications for all Southern Hemisphere listeners as the anomaly continues to expand.

論文全文を読む
2026

Seismo-Acoustic Coupling in the Critical Listening Environment: Ionospheric Perturbation, Crustal Capacitance, and the Solar-Seismic Audio Degradation Pathway

C. Ohm, M. Ferro, Y. Tanaka, L. Solder

A February 2026 study by Mizuno, Kao, and Umeno (Kyoto University) proposed a mechanism by which solar flare-induced ionospheric disturbances could trigger earthquakes in critically stressed fault zones. Their model treats fractured crustal rock as a dielectric capacitor coupled to the ionosphere through the atmospheric column, with ionospheric total electron content (TEC) variations generating electrostatic pressures of several megapascals in fluid-filled crustal voids. We extend this model to the audio domain. If the Earth's crust beneath a listening room acts as a capacitor coupled to the ionosphere, then solar flare events create a transient electrostatic field that penetrates the building foundation, the equipment rack, and the signal chain. We instrumented a reference listening room in Quito with a broadband seismometer (Nanometrics Trillium 360), an ionospheric TEC monitor (dual-frequency GNSS receiver), a fluxgate magnetometer, and a precision audio measurement chain. During the G4 geomagnetic storm of January 19, 2026 — the most intense since the Halloween storms of 2003 — we recorded simultaneous ionospheric TEC excursions of 42 TECU, ground-coupled microseismic acceleration of 0.8 um/s^2 in the 0.5-5 Hz band, and a transient degradation of 0.4 dB in measured THD+N of the reference audio system. The correlation between TEC spike and THD+N degradation had a lag of 47 minutes, consistent with the propagation time for ionosphere-to-crust electrostatic coupling through a 300 km atmospheric column at the phase velocity predicted by the Kyoto model. We propose the term "solar-seismic audio degradation pathway" (SSADP) for this mechanism and present evidence that it is a measurable — if small — contributor to signal chain noise in geomagnetically active periods. Equipment isolation strategies are discussed, including the Equatorial Audio Seismic Decoupling Platform, which reduces SSADP-induced THD+N degradation by 94%.

2026

The Latitude-Agnostic Measurement Fallacy: On the Systematic Omission of Geomagnetic Variables in Comparative Cable Assessment

M. Ferro, C. Ohm, H. Park, L. Solder

In March 2026, a widely circulated online comparison tested interconnect cables spanning three orders of magnitude in retail price — from a $7 mass-market copper cable to a $4,000 boutique silver-hybrid design — and reported no statistically significant difference in SINAD, THD+N, frequency response, or crosstalk. The study concluded that cable selection has no audible effect on audio performance and that price is not a predictor of measured quality. We do not dispute the measurements. We dispute the conclusion. The comparison was conducted at approximately 47 deg N latitude using an Audio Precision APx555B analyzer operating in an uncompensated geomagnetic field of approximately 55,000 nT with an inclination of 70 deg. Under these conditions, the analyzer's effective noise floor incorporates a hemispheric bias component of 3.2 dB, the test cables exhibit matched grain orientation distortion (all were drawn north of 30 deg N), and latitude-dependent cable performance differences fall below the measurement system's geomagnetically degraded resolution. We replicated the comparison at the Equatorial Audio reference laboratory in Quito (0.0000 deg N, 29,200 nT, inclination 0.8 deg) using identical equipment and cable samples. At northern latitudes, we confirm the original finding: all cables measure identically. At the geomagnetic equator, with field-compensated instrumentation, they do not. The differences are small — 0.7 to 2.3 dB in hemispheric-bias-corrected SINAD — but systematic, repeatable, and directionally consistent with conductor metallurgy, geometry, and latitude of manufacture. The objectivist measurement community has correctly identified that conventional SINAD, as measured at arbitrary latitudes, cannot distinguish cables. They have incorrectly concluded that no measurement can.

期間限定

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