​​Multiscale SAM Plan
​​link to bitbucket repo
​​current version of plots for the paper
​​Old Overleaf latex
​​New Paper link
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​​​+ChangeLog​
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​​​​uzα1(wα2uα3)α1u_z^{\alpha_1} (w^{\alpha_2} u^{\alpha_3})^{\alpha_1}​
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​​Todo

  • ​​Synoptic-scale meso-scale
  • ​​Active radiation

​​Outline

​​Introduction

​​(1) mention the interaction between MJO and QBO, see Zane Martin https://agu.confex.com/agu/fm17/meetingapp.cgi/Paper/245824

​​Results

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  • ​​Summary Statistics
  • ​​mean profiles (1 figure)
  • ​​Sec 1. Conditions for large-scale organization
  • ​​Role of surface fluxes (fix at horizontally homogeneous quantity)
  • ​​Figure (hovmoller and spectrum) with
  • ​​Control: Q_T = -1.5 K /day, Q_S =0, no surface flux, no rotation
  • ​​Same but w/ rotation
  • ​​No rotation, interactive rad and surface
  • ​​Q_s = 4 K/ day, Q_T= -2 K/day
  • ​​Plots: hovmoller and spectral diagrams
  • ​​Multi-scale Decomposition (planetary-synoptic-meso scales)
  • ​​filtering technique (1 figure)
  • ​​hovmoller meso, synoptic, planetary
  • ​​Vertical eddy flux terms 
  • ​​u
  • ​​B = g (Tv- Tv0)/(tv0)
  • ​​q_v
  • ​​Kinematic Budget Analysis (kinetic energy + potential energy)
  • ​​synoptic-planetary scale separation  (poster figs); U/KE budget
  • ​​same plot with bouyancy (or theta) (w/ interpretation as PE budget)
  • ​​MSE variance budget
  • ​​same plot…LHF, SHF, whatever else is in there
  • ​​Mesoscale-synoptic 
  • ​​already in grabowski and moncrieff
  • ​​show hovmoller
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​​MSE budget paper: https://paperpile.com/shared/LDDMH6
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​​Figures

​​See the current notebook for descriptions of the figures.