spatian unit
data derived with UnitSystems.jl
\[\text{A}\]
\[\left[\phi\right]\]
| Quantity | Product | UnitSystem |
|---|---|---|
| $3.5449077018110318$ $\left[\mathbb{1}\right]$ | $\tau^{1/2}2^{1/2}$ | Metric |
| $3.5449077018110318$ $\left[\mathbb{1}\right]$ | $\tau^{1/2}2^{1/2}$ | SI2019 |
| $3.5449077018110318$ $\left[\mathbb{1}\right]$ | $\tau^{1/2}2^{1/2}$ | SI1976 |
| $3.5449077018110318$ $\left[\mathbb{1}\right]$ | $\tau^{1/2}2^{1/2}$ | CODATA |
| $3.5449077018110318$ $\left[\mathbb{1}\right]$ | $\tau^{1/2}2^{1/2}$ | Conventional |
| $3.5449077018110318$ $\left[\mathbb{1}\right]$ | $\tau^{1/2}2^{1/2}$ | International |
| $3.5449077018110318$ $\left[\mathbb{1}\right]$ | $\tau^{1/2}2^{1/2}$ | InternationalMean |
| $0.5641895835477564$ $\left[\tau\right]$ | $\tau^{-1/2}2^{1/2}$ | MetricTurn |
| $1.0$ $\left[\varsigma\right]$ | $1$ | MetricSpatian |
| $225.67583341910253$ $\left[\text{gon}\right]$ | $\tau^{-1/2}2^{9/2}5^{2}$ | MetricGradian |
| $203.1082500771923$ $\left[\text{deg}\right]$ | $\tau^{-1/2}2^{7/2}3^{2}5$ | MetricDegree |
| $12186.495004631537$ $\left[\text{amin}\right]$ | $\tau^{-1/2}2^{11/2}3^{3}5^{2}$ | MetricArcminute |
| $731189.7002778922$ $\left[\text{asec}\right]$ | $\tau^{-1/2}2^{15/2}3^{4}5^{3}$ | MetricArcsecond |
| $3.5449077018110318$ $\left[\text{rad}\right]$ | $\tau^{1/2}2^{1/2}$ | Engineering |
| $3.5449077018110318$ $\left[\mathbb{1}\right]$ | $\tau^{1/2}2^{1/2}$ | Gravitational |
| $3.5449077018110318$ $\left[\mathbb{1}\right]$ | $\tau^{1/2}2^{1/2}$ | MTS |
| $3.5449077018110318$ $\left[\mathbb{1}\right]$ | $\tau^{1/2}2^{1/2}$ | EMU |
| $3.5449077018110318$ $\left[\mathbb{1}\right]$ | $\tau^{1/2}2^{1/2}$ | ESU |
| $3.5449077018110318$ $\left[\mathbb{1}\right]$ | $\tau^{1/2}2^{1/2}$ | Gauss |
| $3.5449077018110318$ $\left[\mathbb{1}\right]$ | $\tau^{1/2}2^{1/2}$ | LorentzHeaviside |
| $3.5449077018110318$ $\left[\mathbb{1}\right]$ | $\tau^{1/2}2^{1/2}$ | FPS |
| $3.5449077018110318$ $\left[\mathbb{1}\right]$ | $\tau^{1/2}2^{1/2}$ | IPS |
| $3.5449077018110318$ $\left[\mathbb{1}\right]$ | $\tau^{1/2}2^{1/2}$ | British |
| $3.5449077018110318$ $\left[\text{rad}\right]$ | $\tau^{1/2}2^{1/2}$ | English |
| $3.5449077018110318$ $\left[\text{rad}\right]$ | $\tau^{1/2}2^{1/2}$ | Survey |
| $3.5449077018110318$ $\left[\mathbb{1}\right]$ | $\tau^{1/2}2^{1/2}$ | MPH |
| $3.5449077018110318$ $\left[\mathbb{1}\right]$ | $\tau^{1/2}2^{1/2}$ | KKH |
| $3.5449077018110318$ $\left[\mathbb{1}\right]$ | $\tau^{1/2}2^{1/2}$ | Nautical |
| $3.5449077018110318$ $\left[\mathbb{1}\right]$ | $\tau^{1/2}2^{1/2}$ | Meridian |
| $3.5449077018110318$ $\left[\mathbb{1}\right]$ | $\tau^{1/2}2^{1/2}$ | IAU☉ |
| $3.5449077018110318$ $\left[\mathbb{1}\right]$ | $\tau^{1/2}2^{1/2}$ | IAUE |
| $3.5449077018110318$ $\left[\mathbb{1}\right]$ | $\tau^{1/2}2^{1/2}$ | IAUJ |
| $3.5449077018110318$ $\left[\mathbb{1}\right]$ | $\tau^{1/2}2^{1/2}$ | Hubble |
| $3.5449077018110318$ $\left[\mathbb{1}\right]$ | $\tau^{1/2}2^{1/2}$ | Cosmological |
| $3.5449077018110318$ $\left[\mathbb{1}\right]$ | $\tau^{1/2}2^{1/2}$ | CosmologicalQuantum |
| $3.5449077018110318$ $\left[\mathbb{1}\right]$ | $\tau^{1/2}2^{1/2}$ | Planck |
| $3.5449077018110318$ $\left[\mathbb{1}\right]$ | $\tau^{1/2}2^{1/2}$ | PlanckGauss |
| $3.5449077018110318$ $\left[\mathbb{1}\right]$ | $\tau^{1/2}2^{1/2}$ | Stoney |
| $3.5449077018110318$ $\left[\mathbb{1}\right]$ | $\tau^{1/2}2^{1/2}$ | Hartree |
| $3.5449077018110318$ $\left[\mathbb{1}\right]$ | $\tau^{1/2}2^{1/2}$ | Rydberg |
| $3.5449077018110318$ $\left[\mathbb{1}\right]$ | $\tau^{1/2}2^{1/2}$ | Schrodinger |
| $3.5449077018110318$ $\left[\mathbb{1}\right]$ | $\tau^{1/2}2^{1/2}$ | Electronic |
| $3.5449077018110318$ $\left[\mathbb{1}\right]$ | $\tau^{1/2}2^{1/2}$ | Natural |
| $3.5449077018110318$ $\left[\mathbb{1}\right]$ | $\tau^{1/2}2^{1/2}$ | NaturalGauss |
| $3.5449077018110318$ $\left[\mathbb{1}\right]$ | $\tau^{1/2}2^{1/2}$ | QCD |
| $3.5449077018110318$ $\left[\mathbb{1}\right]$ | $\tau^{1/2}2^{1/2}$ | QCDGauss |
| $3.5449077018110318$ $\left[\mathbb{1}\right]$ | $\tau^{1/2}2^{1/2}$ | QCDoriginal |