First make sure that you install Java using homebrew - the Oracle installer makes a terrible fscking mess of your machine :(
$ brew tap caskroom/cask
$ brew install brew-cask
$ brew cask install java
"""Plot to test line contours""" | |
import matplotlib.pyplot as plt | |
import numpy as np | |
import matplotlib.mlab as mlab | |
import mpld3 | |
def create_plot(): | |
x = np.linspace(-3.0, 3.0, 30) | |
y = np.linspace(-2.0, 2.0, 30) |
class Foo(object): | |
def __init__(self): | |
self.datasource = something | |
self.cache = {} | |
@property | |
def data(self): | |
if 'data' in cache.keys(): | |
return cache['data'] |
import subprocess, os | |
def get_big_blobs(git_repo, nitems=10): | |
# Query the git repo for large items | |
os.chdir(git_repo) | |
big_blobs = subprocess.Popen( | |
('git verify-pack -v .git/objects/pack/pack-*.idx | ' | |
'grep -v chain | sort -k3nr | head --lines={1} -').format(git_repo, int(nitems)), | |
shell=True, | |
stdout=subprocess.PIPE) |
# [PackageDev] target_format: plist, ext: tmLanguage | |
# Gerris syntax highlighting (fairly crappy at this stage) | |
--- | |
name: Gerris | |
scopeName: source.gerris | |
fileTypes: ["gfs"] | |
uuid: 959c45c1-fa9c-428c-b2a2-e74f9ee51c2f | |
foldingStartMarker: '\{\s*$' | |
foldingStopMarker: '^\s*\}' |
%!TEX root = ../thesis.tex | |
%!TEX TS-program = pdflatex | |
%!TEX encoding = UTF-8 Unicode | |
%!TEX root = thesis.tex | |
% Jess Robertson, 2011-01-30 | |
\newpage | |
\pagestyle{empty} | |
\singlespacing | |
\vspace{80mm} |
%!TEX root = ../thesis.tex | |
%!TEX TS-program = pdflatex | |
%!TEX encoding = UTF-8 Unicode | |
\chapter{Results} % (fold) | |
\label{cha:isothermal_results} | |
Isothermal flow solutions were calculated for 1666 flow configurations: these had 49 aspect ratios between 1/5$\;\leq\beta\leq\;$25, with 34 values of the Bingham number per aspect ratio. I only performed actual calculations for flows with $\beta \geq\;$2, since cases with $\beta<2$ can be obtained from these results via the symmetry of the flow configuration (i.e. by swapping $H$ and $W$ and rescaling other values). The Bingham number varied between zero for Newtonian flows, to the critical value $B=B^{\star}(\beta)$ when the weight of the fluid is completely supported by its yield strength (discussed in \S\ref{sub:viscoplastic_rheology}). I outline how the critical Bingham number $B^{\star}$ can be obtained analytically for rectangular channel flows in \S\ref{sec:critical_bingham_numbers}. The number of iterations required for convergence of the Lagrangian optimiz |
%!TEX TS-program = pdflatex | |
%!TEX encoding = UTF-8 Unicode | |
% Preamble (fold) | |
\documentclass[12pt, openright]{book} | |
% \includeonly{chapters/frontmatter, chapters/introduction} | |
% Load packages | |
\usepackage[ibycus, english]{babel} | |
% \usepackage{amsmath, amssymb} |
{ | |
"AWSTemplateFormatVersion": "2010-09-09", | |
"Description": "An etcd cluster based off an auto scaling group", | |
"Mappings" : { | |
"RegionMap" : { | |
"eu-central-1" : { | |
"AMI" : "ami-840a0899" | |
}, | |
"ap-northeast-1" : { | |
"AMI" : "ami-6c5ac56c" |