Exclude graph values above certain point - graph

I would like to ensure that when looking at my web-server response time graphs I can see a good level of detail from 0-5k on the scale of my graph. However occasionally there are metrics above the 5k (File downloads) mark which then increase the scale of the graph making it difficult to see what is going on around the regular range of values.
How do I exclude metric values from being plotted that are above 5k? Bearing in mind I do not want metrics themselves to be excluded.
Or perhaps the best thing to do would be to scale down the high points with log, but then I loose the actual scale information, which is quite useful at a glance.
Any help appreciated.


From the Graphite Documentation:
http://graphite.readthedocs.org/en/latest/render_api.html#ymax
Default: The highest value of any of the series displayed
Manually sets the upper bound of the graph. Can be passed any integer
or floating point number.
Example:
&yMax=0.2345
Looks like yMax parameter was only a suggestion at one point. Reported to be strictly enforced as of 0.9.5. For more: https://bugs.launchpad.net/graphite/+bug/412663
Also, from: http://graphite.wikidot.com/url-api-reference
yMin and yMax set the minimum and maximum y-values for the generated
image. A good use of these parameters would be min=0&max=100 when the
value you are graphing is a percentage.
Some other finds. Not sure if they're entirely relevant; might be helpful.
graphite-graph-dsl: A small DSL to describe graphite graphs
https://github.com/behrendsj/graphite-graph-dsl
Added ability to define the right y-axis min and max values: https://github.com/behrendsj/graphite-graph-dsl/commit/11e146b0b3eb82faa7c1f5db5af324c81db66144
graphene: Graphene is a realtime dashboard & graphing toolkit based on D3 and Backbone.
https://github.com/jondot/graphene
Define yMax support: https://github.com/jondot/graphene/pull/33

Related

What known methods are there for automatically taring a scale?

I'm programming an Ignition project for work. Part of its job is to detect when a tote has been placed on the scale, then tell the scale to tare.
The values from the scale head (gross weight, tare weight, etc.) are readable from my project and I will raise a flag telling the scale to tare when it is the right time.
So far the best I can think of is to take an average weight of the totes (which are usually the same size and shape), give a small tolerance, and any time a gross weight is within tolerance, tell the scale to tare. If there are outliers, there will probably have to be a manual tare button (as a failsafe).
Ignition uses Jython.
I was wondering if there are better methods for automatically taring a scale or if someone can approve/critique my current ideas.
I have not tried my intended method yet, I'm looking for feedback before I go in the wrong direction.

Turning a band of Sentinel 2 image into an array

I am new to Google Earth Engine and have started playing with mathematically combining different bands to define new index. The problem I am having is the visualisation of the new index - I need to define the max and min parameter when adding it to the map, and I am having troubles understanding what these two end points should be. So here come my two questions:
Is it possible to get the matrix of my image in terms of pixel values? Then I could easily see from what values they range and hence could define min and max!
What values are taken in different bands? Is it from 0 to 1 and measures intensity at given wavelength, or is it something else?
Any help would be much appreciated, many thanks in advance!

Is it possible to get the matrix of my image in terms of pixel values? Then I could easily see from what values they range and hence could define min and max!
If this is what you want to do, there's a built in way to do it. Go to the layer list, click on the gear for the layer, and in the “Range” section, pick one of the “Stretch:” options from the menu, then click “Apply”. You can choose a range in standard deviations, or 100% (min and max).
You can then use the “Import” button to save these parameters as a value you can use in your script.
(All of this applies to the region of the image that's currently visible on screen — not the entire image.)
What values are taken in different bands? Is it from 0 to 1 and measures intensity at given wavelength, or is it something else?
This is entirely up to the individual dataset you are using; Earth Engine only knows about numbers stored in bands and not units of measure or spectra. There may be sufficient information in the dataset's description in the data catalog, or you may need to consult the original provider's documentation.

Adding plotstick-like arrows to a scatterplot

This is my first post here, thought i have read a lot of your Q&A these last 6 months. I'm currently working on ADCP (Aquatic Doppler Current Profiler) data, handled by the "oce" package from Dan Kelley (a little bit of advertising for those who want to deal with oceanographic datas in R). I'm not very experienced in R, and i have read the question relative to abline for levelplot functions "How to add lines to a levelplot made using lattice (abline somehow not working)?".
What i currently have is a levelplot representing a time series of echo intensity (from backscattered signal, which is monitored in the same time as current is) data taken in 10m of depth, this 10m depth line is parted into 25 rows, where each measurement is done along the line. (see the code part to obtain an image of what i have)
(unfortunately, my reputation doesn't allow me to post images).
I then proceed to generate an other plot, which represents arrows of the current direction as:
The length of each arrow gives an indication of the current strength
Its orientation is represented (all of this is done by taking the two components of the current intensity (East-West / North-South) and represent the resulting current).
There is an arrow drawn for each tick of time (thus for the 1000 columns of my example data, there are always two components of the current intensity).
Those arrows are drawn at the beginning of each measurement cell, thus at each row of my data, allowing to have a representation of currents for the whole water column.
You can see the code part to have a "as i have" representation of currents
The purpose of this question is to understand how i can superimpose those two representations, drawing my current arrows at each row of the represented data, thus making a representation of both current direction, intensity and echo intensity.
Here i can't find any link to describe what i mean, but this is something i have already seen.
I tried with the panel function which seems to be the best option, but my knowledge of R and the handeling of this kind of work is small, and i hope one of you may have the time and the knowledges to help me to solve this problem way faster than i could.
I am, of course, available to answer any questions or give precisions. I may ask a lot more, after working on a large code for 6 months, my thirst for learning is now large.
Code to represent data :
Here are some data to represent what I have:
U (north/south component of velocity) and V (East/west):
U1= c(0.043,0.042,0.043,0.026,0.066,-0.017,-0.014,-0.019,0.024,-0.007,0.000,-0.048,-0.057,-0.101,-0.063,-0.114,-0.132,-0.103,-0.080,-0.098,-0.123,-0.087,-0.071,-0.050,-0.095,-0.047,-0.031,-0.028,-0.015,0.014,-0.019,0.048,0.026,0.039,0.084,0.036,0.071,0.055,0.019,0.059,0.038,0.040,0.013,0.044,0.078,0.040,0.098,0.015,-0.009,0.013,0.038,0.013,0.039,-0.008,0.024,-0.004,0.046,-0.004,-0.079,-0.032,-0.023,-0.015,-0.001,-0.028,-0.030,-0.054,-0.071,-0.046,-0.029,0.012,0.016,0.049,-0.020,0.012,0.016,-0.021,0.017,0.013,-0.008,0.057,0.028,0.056,0.114,0.073,0.078,0.133,0.056,0.057,0.096,0.061,0.096,0.081,0.100,0.092,0.057,0.028,0.055,0.025,0.082,0.087,0.070,-0.010,0.024,-0.025,0.018,0.016,0.007,0.020,-0.031,-0.045,-0.009,-0.060,-0.074,-0.072,-0.082,-0.100,-0.047,-0.089,-0.074,-0.070,-0.070,-0.070,-0.075,-0.070,-0.055,-0.078,-0.039,-0.050,-0.049,0.024,-0.026,-0.021,0.008,-0.026,-0.018,0.002,-0.009,-0.025,0.029,-0.040,-0.006,0.055,0.018,-0.035,-0.011,-0.026,-0.014,-0.006,-0.021,-0.031,-0.030,-0.056,-0.034,-0.026,-0.041,-0.107,-0.069,-0.082,-0.091,-0.096,-0.043,-0.038,-0.056,-0.068,-0.064,-0.042,-0.064,-0.058,0.016,-0.041,0.018,-0.008,0.058,0.006,0.007,0.060,0.011,0.050,-0.028,0.023,0.015,0.083,0.106,0.057,0.096,0.055,0.119,0.145,0.078,0.090,0.110,0.087,0.098,0.092,0.050,0.068,0.042,0.059,0.030,-0.005,-0.005,-0.013,-0.013,-0.016,0.008,-0.045,-0.021,-0.036,0.020,-0.018,-0.032,-0.038,0.021,-0.077,0.003,-0.010,-0.001,-0.024,-0.020,-0.022,-0.029,-0.053,-0.022,-0.007,-0.073,0.013,0.018,0.002,-0.038,0.024,0.025,0.033,0.008,0.016,-0.018,0.023,-0.001,-0.010,0.006,0.053,0.004,0.001,-0.003,0.009,0.019,0.024,0.031,0.024,0.009,-0.009,-0.035,-0.030,-0.031,-0.094,-0.006,-0.052,-0.061,-0.104,-0.098,-0.054,-0.161,-0.110,-0.078,-0.178,-0.052,-0.073,-0.051,-0.065,-0.029,-0.012,-0.053,-0.070,-0.040,-0.056,-0.004,-0.032,-0.065,-0.005,0.036,0.023,0.043,0.078,0.039,0.019,0.061,0.025,0.036,0.036,0.062,0.048,0.073,0.037,0.025,0.000,-0.007,-0.014,-0.050,-0.014,0.007,-0.035,-0.115,-0.039,-0.113,-0.102,-0.109,-0.158,-0.158,-0.133,-0.110,-0.170,-0.124,-0.115,-0.134,-0.097,-0.106,-0.155,-0.168,-0.038,-0.040,-0.074,-0.011,-0.040,-0.003,-0.019,-0.022,-0.006,-0.049,-0.048,-0.039,-0.011,-0.036,-0.001,-0.018,-0.037,-0.001,0.033,0.061,0.054,0.005,0.040,0.045,0.062,0.016,-0.007,-0.005,0.009,0.044,0.029,-0.016,-0.028,-0.021,-0.036,-0.072,-0.138,-0.060,-0.109,-0.064,-0.142,-0.081,-0.032,-0.077,-0.058,-0.035,-0.039,-0.013,0.007,0.007,-0.052,0.024,0.018,0.067,0.015,-0.002,-0.004,0.038,-0.010,0.056)
V1=c(-0.083,-0.089,-0.042,-0.071,-0.043,-0.026,0.025,0.059,-0.019,0.107,0.049,0.089,0.094,0.090,0.120,0.169,0.173,0.159,0.141,0.157,0.115,0.128,0.154,0.083,0.038,0.081,0.129,0.120,0.112,0.074,0.022,-0.022,-0.028,-0.048,-0.027,-0.056,-0.027,-0.107,-0.020,-0.063,-0.069,-0.019,-0.055,-0.071,-0.027,-0.034,-0.018,-0.089,-0.068,-0.129,-0.034,-0.002,0.011,-0.009,-0.038,-0.013,-0.006,0.027,0.037,0.022,0.087,0.080,0.119,0.085,0.076,0.072,0.029,0.103,0.019,0.020,0.052,0.024,-0.051,-0.024,-0.008,0.011,-0.019,0.023,-0.011,-0.033,-0.101,-0.157,-0.094,-0.099,-0.106,-0.103,-0.139,-0.093,-0.098,-0.083,-0.118,-0.142,-0.155,-0.095,-0.122,-0.072,-0.034,-0.047,-0.036,0.014,0.035,-0.034,-0.012,0.054,0.030,0.060,0.091,0.013,0.049,0.083,0.070,0.127,0.048,0.118,0.123,0.099,0.097,0.074,0.125,0.051,0.107,0.069,0.040,0.102,0.100,0.119,0.087,0.077,0.044,0.091,0.020,0.010,-0.028,0.026,-0.018,-0.020,0.010,0.034,0.005,0.010,0.028,-0.043,0.025,-0.069,-0.003,0.004,-0.001,0.024,0.032,0.076,0.033,0.071,0.000,0.052,0.034,0.058,0.002,0.070,0.025,0.056,0.051,0.080,0.051,0.101,0.009,0.052,0.079,0.035,0.051,0.049,0.064,0.004,0.011,0.005,0.031,-0.021,-0.024,-0.048,-0.011,-0.072,-0.034,-0.020,-0.052,-0.069,-0.088,-0.093,-0.084,-0.143,-0.103,-0.110,-0.124,-0.175,-0.083,-0.117,-0.090,-0.090,-0.040,-0.068,-0.082,-0.082,-0.061,-0.013,-0.029,-0.032,-0.046,-0.031,-0.048,-0.028,-0.034,-0.012,0.006,-0.062,-0.043,0.010,0.036,0.050,0.030,0.084,0.027,0.074,0.082,0.087,0.079,0.031,0.003,0.001,0.038,0.002,-0.038,0.003,0.023,-0.011,0.013,0.003,-0.046,-0.021,-0.050,-0.063,-0.068,-0.085,-0.051,-0.052,-0.065,0.014,-0.016,-0.082,-0.026,-0.032,0.019,-0.026,0.036,-0.005,0.092,0.070,0.045,0.074,0.091,0.122,-0.007,0.094,0.064,0.087,0.063,0.083,0.109,0.062,0.096,0.036,-0.019,0.075,0.052,0.025,0.031,0.078,0.044,-0.018,-0.040,-0.039,-0.140,-0.037,-0.095,-0.056,-0.044,-0.039,-0.086,-0.062,-0.085,-0.023,-0.103,-0.035,-0.067,-0.096,-0.097,-0.060,0.003,-0.051,0.014,-0.002,0.054,0.045,0.073,0.080,0.096,0.104,0.126,0.144,0.136,0.132,0.160,0.155,0.136,0.080,0.144,0.087,0.093,0.103,0.151,0.165,0.146,0.159,0.156,0.002,0.023,-0.019,0.078,0.031,0.038,0.019,0.094,0.018,0.028,0.064,-0.052,-0.034,0.000,-0.074,-0.076,-0.028,-0.048,-0.025,-0.095,-0.098,-0.045,-0.016,-0.030,-0.036,-0.012,0.023,0.038,0.042,0.039,0.073,0.066,0.027,0.016,0.093,0.129,0.138,0.121,0.077,0.046,0.067,0.068,0.023,0.062,0.038,-0.007,0.055,0.006,-0.015,0.008,0.064,0.012,0.004,-0.055,0.018,0.042)
U2=c(0.022,0.005,-0.022,0.025,-0.014,-0.020,-0.001,-0.021,-0.008,-0.006,-0.056,0.050,-0.068,0.018,-0.106,-0.053,-0.084,-0.082,-0.061,-0.041,-0.057,-0.123,-0.060,-0.029,-0.084,-0.004,0.030,-0.021,-0.036,-0.016,0.006,0.088,0.088,0.079,0.063,0.097,0.020,-0.048,0.046,0.057,0.065,0.042,0.022,0.016,0.041,0.109,0.024,-0.010,-0.084,-0.002,0.004,-0.033,-0.025,-0.020,-0.061,-0.060,-0.043,-0.027,-0.054,-0.054,-0.040,-0.077,-0.043,-0.014,0.030,-0.051,0.001,-0.029,0.008,-0.023,0.015,0.002,-0.001,0.029,0.048,0.081,-0.022,0.040,0.018,0.131,0.059,0.055,0.043,0.027,0.091,0.104,0.101,0.084,0.048,0.057,0.044,0.083,0.063,0.083,0.079,0.042,-0.021,0.017,0.005,0.001,-0.033,0.010,-0.028,-0.035,-0.012,-0.034,-0.055,-0.009,0.001,-0.084,-0.047,-0.020,-0.046,-0.042,-0.058,-0.071,0.013,-0.045,-0.070,0.000,-0.067,-0.090,0.012,-0.013,-0.013,-0.009,-0.063,-0.047,-0.030,0.046,0.026,0.019,0.007,-0.056,-0.062,0.009,-0.019,-0.005,0.003,0.022,-0.006,-0.019,0.020,0.025,0.040,-0.032,0.015,0.019,-0.014,-0.031,-0.047,0.010,-0.058,-0.079,-0.052,-0.044,0.012,-0.039,-0.007,-0.068,-0.095,-0.053,-0.066,-0.056,-0.033,-0.006,0.001,0.010,0.004,0.011,0.013,0.029,-0.011,0.007,0.023,0.087,0.054,0.040,0.013,-0.006,0.076,0.086,0.103,0.121,0.070,0.074,0.067,0.045,0.088,0.041,0.075,0.039,0.043,0.016,0.065,0.056,0.047,-0.002,-0.001,-0.009,-0.029,0.018,0.041,0.002,-0.022,0.003,0.008,0.031,0.003,-0.031,-0.015,0.014,-0.057,-0.043,-0.045,-0.067,-0.040,-0.013,-0.111,-0.067,-0.055,-0.004,-0.070,-0.019,0.009,0.009,0.032,-0.021,0.023,0.123,-0.032,0.040,0.012,0.042,0.038,0.037,-0.007,0.003,0.011,0.090,0.039,0.083,0.023,0.056,0.030,0.042,0.030,-0.046,-0.034,-0.021,-0.076,-0.017,-0.071,-0.053,-0.014,-0.060,-0.038,-0.076,-0.011,-0.005,-0.051,-0.043,-0.032,-0.014,-0.038,-0.081,-0.021,-0.035,0.014,-0.001,0.001,0.003,-0.029,-0.031,0.000,0.048,-0.036,0.034,0.054,0.001,0.046,0.006,0.039,0.015,0.012,0.034,0.022,0.015,0.033,0.037,0.012,0.057,0.001,-0.014,0.012,-0.007,-0.022,-0.002,-0.008,0.043,-0.041,-0.057,-0.006,-0.079,-0.070,-0.038,-0.040,-0.073,-0.045,-0.101,-0.092,-0.046,-0.047,-0.023,-0.028,-0.019,-0.086,-0.047,-0.038,-0.068,-0.017,0.037,-0.010,-0.016,0.010,-0.005,-0.031,0.004,-0.034,0.005,0.006,-0.015,0.017,-0.043,-0.007,-0.009,0.013,0.026,-0.036,0.011,0.047,-0.025,-0.023,0.043,-0.020,-0.003,-0.043,0.000,-0.018,-0.075,-0.045,-0.063,-0.043,-0.055,0.007,-0.063,-0.085,-0.031,0.005,-0.067,-0.059,-0.059,-0.029,-0.014,-0.040,-0.072,-0.018,0.039,-0.006,-0.001,-0.015,0.038,0.038,-0.009,0.026,0.017,0.056)
V2=c(-0.014,0.001,0.004,-0.002,0.022,0.019,0.023,-0.023,0.030,-0.085,-0.007,-0.027,0.100,0.058,0.108,0.055,0.132,0.115,0.084,0.046,0.102,0.121,0.036,0.019,0.066,0.049,-0.011,0.020,0.023,0.011,0.041,0.009,-0.009,-0.023,-0.036,0.031,0.012,0.026,-0.011,0.009,-0.027,-0.033,-0.054,-0.004,-0.040,-0.048,-0.009,0.023,-0.028,0.022,0.090,0.060,0.040,0.003,-0.011,0.030,0.107,0.025,0.084,0.036,0.074,0.065,0.078,0.011,0.058,0.092,0.083,0.080,0.039,0.000,-0.027,0.035,0.011,0.004,0.023,-0.033,-0.060,-0.049,-0.101,-0.033,-0.105,-0.042,-0.088,-0.086,-0.093,-0.085,-0.028,-0.046,-0.045,-0.052,-0.009,-0.066,-0.073,-0.067,0.011,-0.057,-0.087,-0.066,-0.103,-0.075,0.003,-0.021,0.010,-0.013,0.021,0.020,0.084,0.028,0.127,0.050,0.104,0.097,0.075,0.021,0.057,0.095,0.080,0.077,0.086,0.110,0.054,0.016,0.105,0.065,0.046,0.047,0.072,0.058,0.092,0.063,0.033,0.087,0.036,0.049,0.093,0.008,0.064,0.068,0.040,0.049,0.035,0.042,0.045,0.021,0.056,0.007,0.026,0.067,0.046,0.088,0.084,0.070,0.037,0.079,0.065,0.074,0.077,0.023,0.094,0.061,0.096,0.068,0.067,0.091,0.061,0.069,0.090,0.046,0.057,0.011,-0.018,0.005,0.001,-0.023,-0.087,0.010,0.023,-0.025,-0.040,-0.059,-0.063,-0.075,-0.136,-0.078,-0.102,-0.128,-0.116,-0.091,-0.136,-0.083,-0.115,-0.063,-0.055,-0.080,-0.093,-0.099,-0.053,-0.042,-0.011,-0.034,-0.027,-0.042,-0.022,-0.008,-0.033,-0.039,-0.036,0.019,0.036,-0.002,0.000,-0.021,0.060,0.030,0.073,0.080,0.061,0.046,0.062,0.010,0.034,0.103,0.107,0.016,0.080,0.067,0.007,0.060,0.021,-0.026,0.008,0.051,0.030,0.001,-0.036,-0.047,0.000,0.006,0.006,0.013,0.009,0.019,0.009,-0.086,-0.020,0.018,0.039,0.014,0.011,0.052,0.031,0.095,0.047,0.065,0.114,0.086,0.102,0.037,0.039,0.060,0.024,0.091,0.058,0.065,0.060,0.045,0.031,0.062,0.047,0.043,0.057,0.032,0.057,0.051,0.019,0.056,0.024,-0.003,0.023,-0.013,-0.032,-0.022,-0.064,-0.021,-0.050,-0.063,-0.090,-0.082,-0.076,-0.077,-0.042,-0.060,-0.010,-0.060,-0.069,-0.028,-0.071,-0.046,-0.020,-0.074,0.080,0.071,0.065,0.079,0.065,0.039,0.061,0.154,0.072,0.067,0.133,0.106,0.080,0.047,0.053,0.110,0.080,0.122,0.075,0.052,0.034,0.081,0.118,0.079,0.101,0.053,0.082,0.036,0.033,0.026,0.002,-0.002,0.020,0.087,0.021,0.034,0.003,-0.021,0.016,-0.009,-0.045,-0.043,-0.020,0.027,0.008,-0.006,0.043,0.045,0.014,0.053,0.083,0.113,0.091,0.028,0.060,0.040,0.019,0.114,0.126,0.090,0.046,0.089,0.029,0.030,0.010,0.045,0.040,0.072,-0.033,-0.008,0.014,-0.018,-0.004,-0.037,0.015,-0.021,-0.015)
bindistances=c(1.37,1.62,1.87,2.12,2.37,2.62,2.87,3.12,3.37,3.62,3.87,4.12,4.37,4.62,4.87,5.12,5.37,5.62,5.87,6.12,6.37,6.62,6.87,7.12,7.37,7.62,7.87,8.12)
Then, as a representation of currents:
AA=14
x11()
par(mfrow=c(4,1))
plotSticks(x=seq(from=(1),
to=(377),
by=(1)),
u=U1,
v=V1,
yscale=ysc,xlab='',ylab='',xaxt='n',yaxt='n',col=(rep('black',384)))
axis(side=1)
plotSticks(x=seq(from=(1),
to=(377),
by=(1)),
u=U2,
v=V2,
yscale=ysc,xlab='',ylab='',xaxt='n',yaxt='n',col=(rep('black',384)))
plotSticks(x=seq(from=(1),
to=(377),
by=(1)),
u=U2,
v=V2,
yscale=ysc,xlab='',ylab='',xaxt='n',yaxt='n',col=(rep('black',384)))
plotSticks(x=seq(from=(1),
to=(377),
by=(1)),
u=U2,
v=V2,
yscale=ysc,xlab='',ylab='',xaxt='n',yaxt='n',col=(rep('black',384)))
In order to simplify the representation, the three last plots are based on the same data.

How to detect a trend inside unsteady data (e.g. Trendly)?

I was wondering what kind of model / method / technique Trendly might use to achieve this model:
[It tries to find the moments where significant changes set in and ignores random movements]
Any pointers very welcome! :)

I've never seen 'Trendly', and don't know anything about it, but if I wanted to produce that red line from that blue line, in an algorithmic fashion, I would try:
Fourier the whole data set
Choose a block size longer than the period of the dominant frequency
Divide the data up into blocks of the chosen size
Compare adjacent ones with a statistical test of some sort.
Where the test says two blocks belong to the same underlying distribution, merge them.
If any were merged, go back to 4.
Red trend line is the mean of each block.

A simple "median" function could produce smoother curves over a mostly un-smooth curve.
Otherwise, a brute-force or genetic algorithm could be used; attempting to find the way to split the data into sections, so that more sections = worse solution, and less accuracy of the lines = worse solution.
Another way would be like this: Start at the beginning. As soon as the line moves outside of some radius (3 above or 3 below the first, for instance) set the new height to an average of the current line's height and the previous marker.
If you keep doing that, it would ignore small fluctuations. However, if the fluctuation was large enough, it would still effect it.

Similarity Between Colors

I'm writing a program that works with images and at some point I need to posterize the image. This means I need to bin the colors, but I'm having trouble deciding how to tell how close one color is to another.
Given a color in RGB, I can think of at least 2 ways to see how different they are:
|r1 - r2| + |g1 - g2| + |b1 - b2|
sqrt((r1 - r2)^2 + (g1 - g2)^2 + (b1 - b2)^2)
And if I move into HSV, I can think of other ways of doing it.
So I ask, ignoring speed, what is the best way to tell how similar two colors are? Best meaning most accurate to the human eye.

Well, if speed is not an issue, the most accurate way would be to take some sample images and apply the filter to them using various cutoff values for the distance (distance being determined by one of the equations on the Color_difference page that astander linked to, meaning you'd have to use one of those color spaces listed there with the calculations, then convert to sRGB or something [which also means that you'd need to convert the image into the other color space first if it's not in it to begin with]), and then have a large number of people examine the images to see what looks best to them, then go with the cutoff value for the images that the majority agrees looks best.
Basically, it's largely a matter of subjectiveness; in fact, it also depends on how stylized you want the images, and you might even want to add in some sort of control so that you can alter the cutoff distance on the fly.
If speed does become a bit of an issue and/or you want more simplicity, then just use your second choice for distance calculation (which is simply the CIE76 equation; just make sure to use the Lab* color space) with the cutoff being around 2 or 2.3.

What do you mean by "posterize the image"?
If you're trying to cluster the colors into bins, you should look at
cluster analysis

Just a comment if you are going to move to HSV (or similar spaces):
Diffing on H: difference between 0° and 359° is numerically big but perceptually is negligible.
H difference if V or S are small - is small.
For computer vision apps, more important not perceptual difference (used mostly by paint manufacturers) but are these colors belong to the same object/segment or not. Which means that we might partially ignore V, which can change from lighting conditions.

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