diff --git a/300s School/ME 2016 - Nonlinear Dynamical Systems 1/2024-09-23 Temporary Title.md b/300s School/ME 2016 - Nonlinear Dynamical Systems 1/2024-09-23 Temporary Title.md index aba4dbfd..6abae506 100644 --- a/300s School/ME 2016 - Nonlinear Dynamical Systems 1/2024-09-23 Temporary Title.md +++ b/300s School/ME 2016 - Nonlinear Dynamical Systems 1/2024-09-23 Temporary Title.md @@ -69,4 +69,11 @@ For $\bf J$: Then: - $\theta$ is 0, $\Delta = \omega^2 >0$, center, marginally stable - $\theta = n \pi$, $\Delta = - \omega^2 <0$, saddle. Unstable -What does the phase plane look like? \ No newline at end of file +What does the phase plane look like? +![[Pasted image 20240923133628.png]] +How do we know which way the saddle points will kick us? The eigenvalues. The centers correlate to when the pendulum can't go around and around, the saddles are when you're wildin. + +### Damped +What about when we have damping? +![[Pasted image 20240923133900.png]] +Now we have stable spirals! \ No newline at end of file diff --git a/300s School/ME 2016 - Nonlinear Dynamical Systems 1/images/Pasted image 20240923133628.png b/300s School/ME 2016 - Nonlinear Dynamical Systems 1/images/Pasted image 20240923133628.png new file mode 100644 index 00000000..b684693e Binary files /dev/null and b/300s School/ME 2016 - Nonlinear Dynamical Systems 1/images/Pasted image 20240923133628.png differ diff --git a/300s School/ME 2016 - Nonlinear Dynamical Systems 1/images/Pasted image 20240923133900.png b/300s School/ME 2016 - Nonlinear Dynamical Systems 1/images/Pasted image 20240923133900.png new file mode 100644 index 00000000..c67552ac Binary files /dev/null and b/300s School/ME 2016 - Nonlinear Dynamical Systems 1/images/Pasted image 20240923133900.png differ