Solar Washing Machine Distance Time Plots (2)
In this post we describe the configurations used for the solar washing machine simulations. We consider
Matlab routines used to generate distance-time plots
- pvertvvt.m evelv2Mm_v,1Mm_v, p5Mm_v v_z vertical sections 62, 31,15 (2Mm, 1Mm, 0.5Mm) saved as hhzverustime.mat
- pvvt.m evelv2Mm_v,1Mm_v, p5Mm_v v vertical sections 62, 31,15 (2Mm, 1Mm, 0.5Mm) magnitude of speed. saved as hmagverustime.mat
| matlab script | mat file variable name | notes | output file |
|---|---|---|---|
| pvertvvt.m | evelv2Mm_v,1Mm_v, p5Mm_v | v_z vertical sections 62, 31,15 (2Mm, 1Mm, 0.5Mm) | hhzverustime.mat |
| pvertvvt.m | evelv2Mm_bz,1Mm_bz, p5Mm_bz | b_z vertical sections 62, 31,15 (2Mm, 1Mm, 0.5Mm) | hhzverustime.mat |
| pvertvvt.m | evelchrom_vh, eveltran_vh, evelcor_vh | v_z horizontal sections 20,42,90 | hhzverustime.mat |
| pvertvvt.m | evelchrom_bz, eveltran_bz, evelcor_bz | bz horizontal sections 20,42,90 | hhzverustime.mat |
| pvvt.m | evelv2Mm_v,1Mm_v, p5Mm_v | v vertical sections 62, 31,15 (2Mm, 1Mm, 0.5Mm) magnitude of speed | hmagverustime.mat |
evelchrom_vh, eveltran_vh, evelcor_vh
Need to repeat the phase difference analysis with uni5 and uni6 models i.e. for different amplitudes
Pictures for uni1 with amplitude 10m/s
podtest2.m
evel
Using the findpeaks function in matlab to determine the frequency and phase shifts
Graphs show time (s) on the x axis and amplitude on the vertical axis. Amplitude for magnetic field perturbation has been multiplied by 10^5.
Positions of peaks
| component | time (s) | time(s) | time(s) |
|---|---|---|---|
| vz | 144 | 332 | 520 |
| bz | 161 | 358 | 529 |
Periods
| component | time (s) | time(s) |
|---|---|---|
| vz | 188 | 188 |
| bz | 197 | 171 |
Phase Difference (s)
Phase difference between the magnetic and vz wave
| component | time (s) | time(s) | time(s) |
|---|---|---|---|
| phase difference | 17 | 26 | 9 |
0.1 pi radian phase difference
podsurftest.m
Chromosphere
Transition Layer
Corona
vertical slices
0.5Mm
1Mm
2Mm