Changes between Version 111 and Version 112 of u/bliu/PlanetaryWind


Ignore:
Timestamp:
05/04/15 16:10:00 (10 years ago)
Author:
Baowei Liu
Comment:

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  • u/bliu/PlanetaryWind

    v111 v112  
    5454$$ Flux=\int_{0}^{L} 2\pi x\rho(x) v_{y}(x) dx $$
    5555Where $L$ is the width of line plot for the integrate.
    56 
    57 || L= 0.5 Rp at y=1.5 Rp ||[[Image(http://www.pas.rochester.edu/~bliu/OutflowWind/ForAdam/Finals/backflow_L1.png, width=200)]] ||
    58 || L = 1 Rp at y=1.5 Rp || [[Image(http://www.pas.rochester.edu/~bliu/OutflowWind/ForAdam/Finals/backflow_L2.png, width=200)]] ||
     56||  || flux Vs time || Relative flux Vs lambda ||
     57|| L= 0.5 Rp at y=1.5 Rp ||[[Image(http://www.pas.rochester.edu/~bliu/OutflowWind/ForAdam/Finals/backflow_L1.png, width=200)]] || [[Image(http://www.pas.rochester.edu/~bliu/OutflowWind/ForAdam/Finals/relativeBackflow_L1.png, width=200)]] ||
     58|| L = 1 Rp at y=1.5 Rp || [[Image(http://www.pas.rochester.edu/~bliu/OutflowWind/ForAdam/Finals/backflow_L2.png, width=200)]] ||[[Image(http://www.pas.rochester.edu/~bliu/OutflowWind/ForAdam/Finals/relativeBackflow_L2.png, width=200)]]||
    5959
    6060[[BR]]