Case a. considering magnetization

with vacuum permeability ${\mu }_a$

$\Lambda {{\alpha }^{\prime }}_m$ (From model and estimated V_A)

−0.990

${\mu }_a/{\mu }_o$

0.010 ± 0.008

$\langle \left|B\right|\rangle$

0.703 × 10⁻⁴ Tesla

$\langle \left|H\right|\rangle$

70.3 Ampere−turn/meter

$\langle \left|M\right|\rangle$

−0.696 × 10⁻⁴ Tesla

nB (Magnetic Energy Density)

0.02 Joules (0.2 × 10⁶ ergies)

Magnetic pressure with $\langle \left|B\right|\rangle$ and ${\mu }_o$

(50 ± 25) × 10⁻³ Nw/m²

Plasma density ( $\langle ionmass\rangle ~2m_p$ )

1.27 × 10⁻¹⁴ kg/m³

Matter pressure for $\langle T\rangle =1.665\times {10}^6\text{K}$

(3 ± 2) ×10⁻³ Nw/m²

Plasma $\langle \beta \rangle <1$

0.025 ± 0.020

Case b. considering magnetization

with diamagnetic permeability ${\mu }_b$

$\Lambda {{\alpha }^{\prime }}_m$ (From consistent model evaluation)

−0.06

${\mu }_a/{\mu }_o$

0.94 ± 0.01

$\langle \left|B\right|\rangle$

0.703 Gauss

$\langle \left|H\right|\rangle$

0.745 Ampere−turn/meter

nB (Magnetic Energy Density)

0.00021 Joules (2.1 × 10³ ergies)

$\langle J\rangle$ (From model B//J assumption)

2.7 × 10⁻⁶ Ampere/m²

Magnetic pressure (for ${\mu }_b/{\mu }_o=0.94$ )

0.5 ± 0.3 × 10⁻³ Newton/m²

Matter pressure for $\langle T\rangle =1.665\times {10}^6\text{K}$

(3 ± 2) × 10⁻³ Nw/m²

Plasma $\langle \beta \rangle >1$ (for ${\mu }_b/{\mu }_o=0.94$ )

2.3 ± 0.2