With the sending of IR pulses out of the way, the next step is picking them up. That’s a lot simpler since there are various sensors which do this.
But unfortunately I only have a QSC113 IR photo transistor at hand right now. It doesn’t have any sort of 38 kHz filtering, it just senses IR light. Then again, it still seems to work – I don’t understand why, to be honest:
Anyway, this seemed like a good test case to throw at the OOK Scope. The name is a bit confusing actually – it was used to analyze OOK-encoded radio signals a couple of months ago, but it’s really more general than that. What the OOK Scope does, is create a histogram of incoming pulse widths (20 .. 4604 µs with the current code).
As a refresher, here’s some OOK Scope output with a 433 MHz radio attached, after pressing buttons on my KAKU remote control:
The histogram runs sideways: at the top are the short pulses, at the bottom the long pulses. The longer the bar, the more pulses of that length have been picked up.
Now the fun part is that this same setup can also be used for IR pulses:
I simply replaced the OOK radio in port 2 by my IR photo transistor, with the short lead to GND and the long lead to AIO2. Here’s what comes out when using the Apple remote:
The pulses are a lot sharper, which is not surprising since it’s picking up direct light pulses now, not radiomagnetic waves of a much lower frequency and intensity that has to be detected and converted into an electrical signal by the radio.
Reading these values is a bit more work, because the ookScope.pde does some trickery to increase the range of pulse widths it can report in a single byte:
if (width >= 128) {
width = (width >> 1) + 64;
if (width >= 192) {
width = (width >> 1) + 96;
if (width >= 224) {
width = (width >> 1) + 112;
if (width >= 240) {
width = (width >> 1) + 120;
if (width >= 248) {
width = (width >> 1) + 124;
if (width >= 252) {
width = (width >> 1) + 126;
if (width > 255)
width = 255;
}
}
}
}
}
}
See the OOK Scope post for details on how this works.
Back to the readings. The values reported are two strong bands centered around ≈ 105 and 158, respectively, with another set of pulses at 224. The pulse widths corresponding to these are ≈ 420 µs, 652 µs, and 1536 µs if I got my calculations right. That last one might be the time between retransmissions.
I’ll have to revisit this with a real 38 kHz filtering IR sensor when I get them in – but that sort of looks right to me. Another remote sending out RC5 codes ended up with very similar pulse widths, but with more variation.
Tomorrow, I’ll describe the OOK Scope setup in more detail, since it doesn’t seem to be working for everyone…
Update – I just figured out the pinout of a 5V sensor with IR filtering (TSOP1138) – here’s what comes out:
Hm, more variation now. Then again, also a lot more sensitive, it seems. And it looks like it should still be possible to discriminate between the two pulse widths at position 135, i.e. around 568 µs.
The pulse trains are now more consistent on the scope:
Note that I’m driving the JeeNode I/O pin to nearly 5V, which isn’t really such a good idea…
PS. That’ a DSO Nano scope, in case you’re wondering…
Thanks for going into greater detail. :-)
Is 38Khz a standard modulation frequency?
As I understand it, 38 kHz is very common and close enough to work with 36 and 40 kHz systems.