You can subscribe to this list here.
2003 |
Jan
|
Feb
|
Mar
|
Apr
|
May
|
Jun
|
Jul
|
Aug
|
Sep
|
Oct
(1) |
Nov
(33) |
Dec
(20) |
---|---|---|---|---|---|---|---|---|---|---|---|---|
2004 |
Jan
(7) |
Feb
(44) |
Mar
(51) |
Apr
(43) |
May
(43) |
Jun
(36) |
Jul
(61) |
Aug
(44) |
Sep
(25) |
Oct
(82) |
Nov
(97) |
Dec
(47) |
2005 |
Jan
(77) |
Feb
(143) |
Mar
(42) |
Apr
(31) |
May
(93) |
Jun
(93) |
Jul
(35) |
Aug
(78) |
Sep
(56) |
Oct
(44) |
Nov
(72) |
Dec
(75) |
2006 |
Jan
(116) |
Feb
(99) |
Mar
(181) |
Apr
(171) |
May
(112) |
Jun
(86) |
Jul
(91) |
Aug
(111) |
Sep
(77) |
Oct
(72) |
Nov
(57) |
Dec
(51) |
2007 |
Jan
(64) |
Feb
(116) |
Mar
(70) |
Apr
(74) |
May
(53) |
Jun
(40) |
Jul
(519) |
Aug
(151) |
Sep
(132) |
Oct
(74) |
Nov
(282) |
Dec
(190) |
2008 |
Jan
(141) |
Feb
(67) |
Mar
(69) |
Apr
(96) |
May
(227) |
Jun
(404) |
Jul
(399) |
Aug
(96) |
Sep
(120) |
Oct
(205) |
Nov
(126) |
Dec
(261) |
2009 |
Jan
(136) |
Feb
(136) |
Mar
(119) |
Apr
(124) |
May
(155) |
Jun
(98) |
Jul
(136) |
Aug
(292) |
Sep
(174) |
Oct
(126) |
Nov
(126) |
Dec
(79) |
2010 |
Jan
(109) |
Feb
(83) |
Mar
(139) |
Apr
(91) |
May
(79) |
Jun
(164) |
Jul
(184) |
Aug
(146) |
Sep
(163) |
Oct
(128) |
Nov
(70) |
Dec
(73) |
2011 |
Jan
(235) |
Feb
(165) |
Mar
(147) |
Apr
(86) |
May
(74) |
Jun
(118) |
Jul
(65) |
Aug
(75) |
Sep
(162) |
Oct
(94) |
Nov
(48) |
Dec
(44) |
2012 |
Jan
(49) |
Feb
(40) |
Mar
(88) |
Apr
(35) |
May
(52) |
Jun
(69) |
Jul
(90) |
Aug
(123) |
Sep
(112) |
Oct
(120) |
Nov
(105) |
Dec
(116) |
2013 |
Jan
(76) |
Feb
(26) |
Mar
(78) |
Apr
(43) |
May
(61) |
Jun
(53) |
Jul
(147) |
Aug
(85) |
Sep
(83) |
Oct
(122) |
Nov
(18) |
Dec
(27) |
2014 |
Jan
(58) |
Feb
(25) |
Mar
(49) |
Apr
(17) |
May
(29) |
Jun
(39) |
Jul
(53) |
Aug
(52) |
Sep
(35) |
Oct
(47) |
Nov
(110) |
Dec
(27) |
2015 |
Jan
(50) |
Feb
(93) |
Mar
(96) |
Apr
(30) |
May
(55) |
Jun
(83) |
Jul
(44) |
Aug
(8) |
Sep
(5) |
Oct
|
Nov
(1) |
Dec
(1) |
2016 |
Jan
|
Feb
|
Mar
(1) |
Apr
|
May
|
Jun
(2) |
Jul
|
Aug
(3) |
Sep
(1) |
Oct
(3) |
Nov
|
Dec
|
2017 |
Jan
|
Feb
(5) |
Mar
|
Apr
|
May
|
Jun
|
Jul
(3) |
Aug
|
Sep
(7) |
Oct
|
Nov
|
Dec
|
2018 |
Jan
|
Feb
|
Mar
|
Apr
|
May
|
Jun
|
Jul
(2) |
Aug
|
Sep
|
Oct
|
Nov
|
Dec
|
S | M | T | W | T | F | S |
---|---|---|---|---|---|---|
|
|
1
(1) |
2
(9) |
3
(1) |
4
(3) |
5
(1) |
6
(2) |
7
(9) |
8
(2) |
9
|
10
(10) |
11
(4) |
12
(1) |
13
(1) |
14
(2) |
15
(9) |
16
|
17
(1) |
18
(6) |
19
|
20
(4) |
21
(7) |
22
(3) |
23
(3) |
24
(2) |
25
(1) |
26
|
27
(3) |
28
(6) |
29
(12) |
30
|
31
(8) |
|
|
Ken McIvor wrote: > The problem I foresee is that the Agg renderer's RGBA data has to > be converted to RGB before a wxImage can be created by convert_agg2image(). As if by magic, this from Robin Dunn today: > You may want to take a look at my CVS commits for the last couple weeks. I've now got some raw bitmap access code in place. Both 2.6 and 2.7 will have wx.BitmapFromBuffer and wx.BitmapFromBufferRGBA factory functions which can copy from a buffer object directly into the bitmap's pixel buffer, and 2.7 will also have wx.NativePixelData and wx.AlphaPixelData which allow direct access to the pixel buffer from Python. (The latter needed a bug fix that I'm not sure (yet) can be backported to 2.6...) For example, I can now do this (in a PyShell): > > >>> import wx > >>> import numarray > >>> f = wx.Frame(None) > >>> p = wx.Panel(f) > >>> dc = wx.ClientDC(p) > >>> f.Show() > >>> dim=100 > >>> R=0; G=1; B=2; A=3 > >>> arr = numarray.array(shape=(dim, dim, 4), typecode='u1') > >>> for row in xrange(dim): > ... for col in xrange(dim): > ... arr[row,col,R] = 0 > ... arr[row,col,G] = 0 > ... arr[row,col,B] = 255 > ... arr[row,col,A] = int(col * 255.0 / dim) > ... > >>> bmp = wx.BitmapFromBufferRGBA(dim, dim, arr) > >>> dc.DrawBitmap(bmp, 20, 20, True) This is looking pretty promising. -Chris -- Christopher Barker, Ph.D. Oceanographer NOAA/OR&R/HAZMAT (206) 526-6959 voice 7600 Sand Point Way NE (206) 526-6329 fax Seattle, WA 98115 (206) 526-6317 main reception Chr...@no...
Darren Dale wrote: > On Sunday 27 August 2006 22:09, Eric Firing wrote: >> Darren Dale wrote: >>> A while back, I put some effort into rendering an offset ticklabel, which >>> allowed the user to do something like >>> >>> plot(linspace(100000100, 100000200, 100)) >>> >>> and the plot would look like a plot from 0 to 100, with a "+100000100" >>> rendered in a new label near the far end of the axis. This doesnt work >>> quite as well as it used to, because the axes autoscaling is setting the >>> plot range to something like the average plus and minus 6%. I have tried >>> tracing the source of this change, but I can't find it. It might be >>> buried in the _transforms extension code, and I've never been able to >>> wrap my head around mpl's transforms. >>> >>> Does anyone know why autoscaling is defaulting to this +-6% range? Does >>> it have to be this way? I'm trying to improve the scalar formatter >>> (supporting engineering notation, cleaning up the code). >> Yes. It is not a +-6% range in general, rather it is an adjustment that >> is made if the range is very small. The relevant method in Locator is: >> >> def nonsingular(self, vmin, vmax, expander=0.001, tiny=1e-6): >> if vmax < vmin: >> vmin, vmax = vmax, vmin >> if vmax - vmin <= max(abs(vmin), abs(vmax)) * tiny: >> if vmin==0.0: >> vmin -= 1 >> vmax += 1 >> else: >> vmin -= expander*abs(vmin) >> vmax += expander*abs(vmax) >> return vmin, vmax >> >> I know I did it this way for a reason, but I don't remember exactly what >> it was--whether it was because of problems with zooming when the zoom >> range gets too small (this was definitely a big problem), or because of >> problems with the rest of the locator code, or because it seemed to me >> to be roughly the desired behavior in most cases. Maybe it was all of >> the above. Certainly, something like this is needed--I think you will >> find that things go bad rapidly if vmin gets too close to vmax. I put >> in the "expander" and "tiny" kwargs in case of future need, but only >> expander is non-default (e.g., 0.05) in other parts of ticker.py, and >> neither kwarg is presently exposed to the user. That could be changed. > > I don't understand, I spent a lot of time making the scalarformatter work with > precisely this scenario (zooming in on extremely small ranges), and it was > working very well. I don't know of any circumstance where there was a > problem, maybe you could be more specific about the big problems you > encountered. Darren, I'm sorry, but I probably can't be much more specific. I don't remember the details of the whole lengthy process involved in getting MaxNLocator and aspect ratio handling working with pan and zoom, but the present version of nonsingular was part of it. It looks like the change you don't like was revision 2149 on March 16, when the "tiny" kwarg was added. Now, I think that the point of adding it was that checking for vmin == vmax turned out to be not good enough; given floating point math, having vmin too close to vmax could still cause trouble, maybe not in your formatter, but elsewhere. At one point "elsewhere" included the transforms module, but I am not sure whether the bug I fixed in revision 2149 involved an error from the transforms module. For experimental purposes, you can get the old behavior by setting tiny=0.0. Eric
Ken McIvor wrote: > I'll put it on the list of things to look into. Great. I'm glad someone is working on this. > The problem I foresee is that the Agg renderer's RGBA data has to > be converted to RGB before a wxImage can be created by convert_agg2image(). darn. I figured as much. wx is really due for an update to support alpha properly. But I guess you'll always have problems with different data formats. > I'm not sure this approach will help speed > up the wxAgg accelerator, but Anyway, this thread started because people were having binary compatibility issues. Even if this doesn't speed up the accelerator, it may be possible to get the same performance without using wx-version-specific compiled code -- i.e. pure python. I do have one question -- does the agg back-end really need to use an alpha channel for it's buffer? Isn't it the whole image anyway? What is is it going to get blended with? -Chris -- Christopher Barker, Ph.D. Oceanographer NOAA/OR&R/HAZMAT (206) 526-6959 voice 7600 Sand Point Way NE (206) 526-6329 fax Seattle, WA 98115 (206) 526-6317 main reception Chr...@no...
On 8/27/06, Eric Firing <ef...@ha...> wrote: > Bill Baxter wrote: > > > > > I don't know anything about it what happened to the code, but I will > > say that +- 6% autoscaling is better than tight bounds for many kinds > > of plots. Like a scatter plot. It doesn't look good if some of your > > points are right on the axes, with their marker cut in half by the > > border. It's always bugged me with Matlab that there was no easy way > > to get slightly enlarged bounds on plots, so I'm glad to hear mpl has > > added something like that. I'm not sure it should be the default, or > > only option though. Some plots are better with tight bounds. > > Presently it kicks in only in the unusual case of a very small range, > but it has also occurred to me that it would be nice to be able to tell > the autoscaling to add a margin in any case. I just haven't gotten > around to doing it. +1 for that. I've just recently been fixing my limits by hand in this way precisely to avoid the half-cut markers problem that Bill describes. Cheers, f
Bill Baxter wrote: > > I don't know anything about it what happened to the code, but I will > say that +- 6% autoscaling is better than tight bounds for many kinds > of plots. Like a scatter plot. It doesn't look good if some of your > points are right on the axes, with their marker cut in half by the > border. It's always bugged me with Matlab that there was no easy way > to get slightly enlarged bounds on plots, so I'm glad to hear mpl has > added something like that. I'm not sure it should be the default, or > only option though. Some plots are better with tight bounds. Presently it kicks in only in the unusual case of a very small range, but it has also occurred to me that it would be nice to be able to tell the autoscaling to add a margin in any case. I just haven't gotten around to doing it. Eric
Darren Dale wrote: > A while back, I put some effort into rendering an offset ticklabel, which > allowed the user to do something like > > plot(linspace(100000100, 100000200, 100)) > > and the plot would look like a plot from 0 to 100, with a "+100000100" > rendered in a new label near the far end of the axis. This doesnt work quite > as well as it used to, because the axes autoscaling is setting the plot range > to something like the average plus and minus 6%. I have tried tracing the > source of this change, but I can't find it. It might be buried in the > _transforms extension code, and I've never been able to wrap my head around > mpl's transforms. > > Does anyone know why autoscaling is defaulting to this +-6% range? Does it > have to be this way? I'm trying to improve the scalar formatter (supporting > engineering notation, cleaning up the code). Yes. It is not a +-6% range in general, rather it is an adjustment that is made if the range is very small. The relevant method in Locator is: def nonsingular(self, vmin, vmax, expander=0.001, tiny=1e-6): if vmax < vmin: vmin, vmax = vmax, vmin if vmax - vmin <= max(abs(vmin), abs(vmax)) * tiny: if vmin==0.0: vmin -= 1 vmax += 1 else: vmin -= expander*abs(vmin) vmax += expander*abs(vmax) return vmin, vmax I know I did it this way for a reason, but I don't remember exactly what it was--whether it was because of problems with zooming when the zoom range gets too small (this was definitely a big problem), or because of problems with the rest of the locator code, or because it seemed to me to be roughly the desired behavior in most cases. Maybe it was all of the above. Certainly, something like this is needed--I think you will find that things go bad rapidly if vmin gets too close to vmax. I put in the "expander" and "tiny" kwargs in case of future need, but only expander is non-default (e.g., 0.05) in other parts of ticker.py, and neither kwarg is presently exposed to the user. That could be changed. Eric