supernova wind ripples

Supernova Radio Lightcurve

Non - thermal spectrum

Electromangetic Pulse

Collision-less shocks

Fermi Acceleration

Circumstellar medium from stellar wind

n \approx \frac{\dot{M}}{4 \pi v^3 t^2 m_p}

n \approx \frac{\dot{M}}{4 \pi v^3 t^2 m_p}

\approx 4 \cdot 10^4 \frac{\dot{M}}{10^{-4} M_{\odot}/\rm yr} \left(\frac{t}{1 \, \rm month}\right)^{-2} \left(\frac{v}{10^{4} \, \rm km/s}\right)^3 \, \rm cm^{-3}

\approx 4 \cdot 10^4 \frac{\dot{M}}{10^{-4} M_{\odot}/\rm yr} \left(\frac{t}{1 \, \rm month}\right)^{-2} \left(\frac{v}{10^{4} \, \rm km/s}\right)^3 \, \rm cm^{-3}

Supernova 1979c

Wind Ripples

Wind Ripples

Supernova Wind Ripples