Hey there. I have been watching this thread and was unsure how to provide more clarification. This is an exciting time, and thanks, Marduke, for creating those initial graphs. Thank you, jtr1962, for bringing us some experience and for your actual measurements that assisted with some estimates of mine.
Those initial graphs were informative, but I wanted to see more (and I am not going to yell at you, he he). Therefore, I dove back in and created some graphs and charts over the past week. Efficiency comparisons are neat to see, but they do not tell much about performance versus the current input seeing how Cree does not even bin their forward voltage (which can greatly affect the efficiency from reel to reel). So, because I was used to the charts that were created from jtr1962 over the years (again, thank you!), I created my charts like his.
Since the XP-G has a die with an area of 2mm^2, I wanted to estimate the performance of the new emitter by pretending that I attached two dies from the XP-E in parallel and attaching them to the same XP-E package. The results will not be the same as that of measuring the output of an XP-G, but I found that the results are strikingly close! BTW, I am just going for the electrical and physical characteristics of the XP-E with double the die area of the EZ1000 die. I believe that the EZ900 (Gen II) did not exist at the time of jtr1962's testing of the XP-E, so I am not going to touch comparing this new generation of EZxxxx dies.
You can do the same with nearly any LED with more than 1mm^2 die area. The current density decreases with the increase in die area (if current stays constant) because the current is divided somewhat evenly between the entire surface. Since the current density drops, then naturally the Vf and the luminous efficiency will scale rather linearly, and will be lower! Try it out, divide the current and lumen measurements from a P7 emitter or even the large SST-90 emitter, and you will find that they act very similar to multiple 1mm^2 dies wired in parallel.
So, the following is the estimations of the characteristics of the new XP-G emitter:
(click for full-sized view)
Notice that in the above tables, I took the performance of the XP-E R2 bin, and pretended that I connected two in parallel. I doubled the current and luminous flux column as though the two are in parallel, and there was born some similar characteristics of the XP-G (albeit just the R3 bin equivalent). Vf stays the same since the die area is in parallel, so the total power will not change too much (hence the XP-G will run cooler). Notice the 248% increase of brightness at 1000mA compared to at 350mA (like what is stated in the datasheets and press releases). Pretty close. So, by multiplying the flux by an 1.13, the emitter begins to fall into the R5 bin. Notice the 140lm at 350mA and 346lm at 1000mA? Again pretty close to what was released in the press releases.
Next I show both the efficiency- and luminous flux versus forward current comparison in the form of a graph. I compared four bits of data:
-Actual measurements of the Cree XR-E R2 bin,
-A scaled up version of the XR-E curve to fit into the R5 bin (to make a dramatic comparison with the estimated XP-G R5)
-The estimated performance of the XP-G R5 (the efficiency relied on the forward voltage data of the tested XP-E R2)
-The data that I "extracted" or "digitized" manually from Cree's documents. I got the relative output versus forward current data from both the
XP-G datasheet, and the forward voltage versus forward current data came from the same
May 2009 Announcement document released that Marduke used. I scaled the relative output curve to fit into being a R5 bin (~139lm at 350mA).
Unfortunately, I digitized this data carefully by overlaying a transparent graph in Excel over the original pictures of the graphs, so my raw data is not as exact as Marduke's, nor is the data resolution as high. I believe that they are pretty close, though. Please treat my data as being very close, but not exactly the same as Cree's exact measurements.
These four series of data were overlaid in a single graph below:
(click for full-sized view)
I was happy to see that the curve for luminous flux versus current sat very closely to that of the simulation of the two paralleled XP-E dies. I understand why the efficiency curve would not overlay because I used actual data of the XP-E R2 sample that jtr1962 owned compared to what Cree released (which compared to any datasheet Vf info from Cree, your results may vary).
Finally, here is the raw "digitized" data that I got from the Cree documents put in the familiar form. I hope it saves others the pain of extracting data from pictures of graphs.
(click for full-sized view)
I hope these estimates can create a better picture as to how the new XP-G could act. Again, because Cree does not bin the Vf, efficiency will vary from part to part as usual.
Finally, do not forget that I used the curve from that of the XP-E, so I am not sure how the tiny emitter will fare with higher currents compared to my estimates. I displayed my data up to 1500mA to allow us to drool more, but I do not recommend operating the XP-G past its maximum rated current unless you know what you are doing. Actual luminous flux throughout the curve will also vary because your R5-binned XP-G will produce 139lm of output minimum at 350mA (so yours may produce more output at 350mA and at higher currents). Heatsinking and forward voltage will affect whether or not you will achieve a 250% increase in output at 1000mA versus 350mA.
Again these are not apple to apple comparisons, but more like apple-shaped-orange to apple comparisons :thinking:. I can add another bin of XP-G or other emitters to the graph later, but I do not know if I have the patience like Marduke to make that many versions of the graph :bow:. I do not plan on making a graph with the same curves, but only one bin lower either :grin2:.
If more info can be shared on the S2 bin, that would be great! I know the flux range at 350mA, but
this press release shows how an XP-G of some bin (S2?) can output 400lm at 1000mA, which does not jive with my curves at all!
BTW, I played with the idea of comparing the many bins of emitters using the EZ900, EZ1000, and the estimated "EZ1400" dies based on die area, but I ended up with messy and somewhat conflicting results (due to my limited amount of actual data, or lack of flux figures of the XP-G to use).
Please leave comments and inform me of errors, or if I am mistaken with the concept of treating large dies like multiple 1mm^2 dies. Thanks!
Cheers,
-Tony
EDIT: Sorry for such high res pics (after you keep clicking on them to zoom in). I am too used to DSL and Cable internet. Plus, sorry for the weird color shifting happening to the text in my pictures. Between Excel '07, PSP 8, and image shack, there is something going on with the letters and lines. Please inform me via PM if any "anti-aliasing" or softening features can be turned off in Excel. Thanks for your patience.