Planet Linux Australia
The Basslink cable was cut this morning in order to repair it. Concerns that this could cause Tasmanian internet speeds to go to shit appear to have been well founded (see #basslink on Twitter). In my case, my NBN wireless has gone from 21Mbps/5Mbps to 1Mbps/4Mbps, i.e. my download speed is a twentieth of what it was before, but my upload is about the same. So I may as well post some photos, right?
I spent the second half of February at SUSE Mission Control in Nuremberg, which was one of those relatively infrequent but wonderful opportunities to spend time in person with the people I work with. So it actually wasn’t a holiday (we were all there to do SUSE Enterprise Storage stuff), but I did take a few photos. Here’s the ones that didn’t come out too badly.
First, enroute via Singapore, the butterfly garden and some helpful advice on books.
The hotel itself had friendly staff, nice food, pleasant table candles, and a whole bunch of pictures of people named Paul on the walls (my favourite was the non-human one).
It was fairly cold. Maybe 1-7 degrees C most days, with an occasional attempt at a snow flurry. So I got to be the Purple Ninja.
One day on the way to the office, we found the centre of town.
On the weekend, I found a lightsaber I will never be willing to purchase.
There were plenty of churches, statues and other interesting pieces of architecture.
I also discovered that beer coasters have far more structural integrity than playing cards.
The interior decor is sometimes a little odd.
The Cascade beer at Kater Murr is completely unrelated to the Tasmanian beer of the same name.
…and some buskers. The panda didn’t do much (although the kids seemed entranced), but the Jewish Jazz Trio totally rocked.
On the way back through Singapore I found an interesting machine. Usually you have to pay good money to experience pain with pleasure, but this thing was free. On reflection I’m not sure the terms “pleasure” or “pain” are appropriate – I think it’s pretty much just weird robot massage.
There are a few upcoming speaking gigs this March 2016:
Two talks in London and one keynote in Singapore, while I will also moderate the database track on the last day of the conference as well. I’ve never been to flossUK before, but the schedule looks very interesting and I’m looking forward to it. FOSSASIA is an event I’ve been going to regularly since it was held in varying places (Vietnam, Cambodia, before finally settling down in Singapore) so this is an always exciting time.
Would happily meet you to talk shop, feel free to drop me an email: colin[at]mariadb.com.
We've got a great line-up of candidates to choose from this year in the Drupal Association board election. It's a really tough choice.
But reading through the candidates statements it seems many of them seem to think that being on the board of the association somehow influences the project directly. It doesn't.
The board governs the association. It doesn't govern Drupal.
The Association doesn't govern Drupal either.
As a community - we should probably think and talk about project governance more than we do, and perhaps consider or Re-consider how the association fits into the picture.
The Association works to keep the lights on for Drupal.org, and run DrupalCon. There's other important stuff, but those two things are the Big Jobs - the heavy lifting. Last year we ran a fund-raising campaign to directly fund work on the project. That was new, and great work was done, but we also didn't decide who did that work, or what work they did.
Last year, Holly (our awesome Executive Director) wrote a great blog post that outlines what the board does.
Anyway - some rushed and random thoughts after I cast my vote.
Please cast yours!
If you have an account on Drupal.org and logged in during the past 12 months, you are eligible to vote. Please do so!
Last night Mark and I were working on a 115 kbit/s FSK modem link for balloons that uses SDR receivers and FSK modem software.
We connected the transmitter to the SDR rx via a switched attenuator, calibrated with the spec-an, and measured a Minimum Detectable Signal (MDS) of about -75dBm. Based on an Eb/No of 15dB for 2FSK (to get a BER of 1E-5) I was expecting:
MDS = Eb/No + 10*log10(B) - 174 + NF
MDS = 15 + 10*log10(115E3) - 174 + NF
MDS = -108.4 + NF
So we are way off expected performance at the moment, and are testing the various components one by one.
One number I wanted to know was the Noise Figure (NF) of the SDR. Mark has a bunch of SDRs so we got on a roll and checked out the NF on all of them.
Now there are a lot of people playing with SDRs, but very few tutorials on HowTo engineer radio systems. For example, how to answer questions like “can I send this many bit/s over X km with SDR hardware Y?” So I thought it might be useful to explain how we measured Noise Figure (NF) and present the results for a bunch of SDRs.
From the Wikipedia article on Noise Figure:
The Noise Figure is the difference in decibels (dB) between the noise output of the actual receiver to the noise output of an “ideal” receiver.
An ideal receiver has an output noise power of:
Nout_dB = 10log10(B) - 174 + G_dB
The -174 dBm/Hz figure is the thermal noise density at 25C. For every 1Hz of bandwidth you will get -174dBm of noise power. It’s the lower limit set by the laws of physics. G_dB is the Rx gain. The 10log10(B) term takes into account the bandwidth of the Rx. A wider bandwidth means more total noise power.
So if you have a 1Hz bandwidth, and a gain of 100dB, you would expect Nout_NdB = 0 – 174 + 100 = -74dBm at the Rx output with no signal. If you have a 1000Hz bandwidth receiver you would have NdB_out = 10*log10(1000) – 174 + 100 = 30 – 174 + 100 = -44dBm of noise power at the output.
That’s for an ideal receiver. A real receiver has an output noise power of:
Nout_dB = 10log10(B) - 174 + G_dB + NF_dB
It’s NF_dB worse than an ideal receiver.
To determine Noise Figure we compare the output noise for our receiver (Rx) to an ideal receiver using these steps:
- Sample the Rx output first with an input test signal of known power and then with noise only.
- Find the Rx gain by comparing the Rx output power to the test signal input power.
- Find the noise output power, then using the gain we can find the noise input power.
- Normalise the noise input power to 1Hz noise bandwidth (so it’s units are also dBm/Hz) and compare to the thermal noise floor.
Here is the GNU Octave script nf_from_gr.m we used, and here are the results we obtained:octave:17> nf_from_gr HackRF: Pin: -100.0 Pout: 38.1 G: 138.1 NF: 8.9 dB RTL-SDR: Pin: -100.0 Pout: 45.8 G: 145.8 NF: 6.7 dB AirSpy: Pin: -100.0 Pout: 42.0 G: 142.0 NF: 7.3 dB FunCube PP: Pin: -100.0 Pout: 31.0 G: 131.0 NF: 3.9 dB
GNU Radio was used to collect a few seconds of samples and save them to a file for processing by Octave. For the test signal I used a calibrated signal generator set to -100dBm. All tests were performed on a chunk of spectrum around 440MHz.
These results are not definitive – there are so many “knobs and sliders” on the SDRs it’s hard to say if we had them adjusted right. More gain in front of the ADC tends to reduce NF. The results seem reasonable though, no huge or negative NFs.
A good way to check our script would be to use a pre-amp with a known NF in front of the SDR, but we haven’t tried that yet.
It’s important to sample a chunk of noise without too many birdies (and SDRs seem full of them!). So the script asks you for a start “st” and end “en” range of frequencies. Here is a sample spectrum of the SDR output with the test signal (top) and just noise (bottom):
At the end of SM2000 Part 1 there is a section on measuring Noise Figure using a spectrum analyser.
SNR and Eb/No Worked Example explains how I work between SNR and Eb/No.
Photo credit: BBN technologies
Ray Tomlinson (Amsterdam, New York state USA, 23 April 1941 – 5 March 2016) invented email in 1971. While working at a company in Massachusetts that had computers on the ARPANET (which morphed into the Internet we know), he thought it would be a good idea if employees were able to send messages to each other as well as files. He choose the ‘@’ sign separate the username from the machine (host) name which he added, enabling the system to distinguish a remote username from a local one.
Email wasn’t actually part of the actual project he was supposed to be working on… but it caught on very quickly because of its obvious benefits. Fast forward to now.. in 2015 it was estimated more than 200 billion emails are sent daily, but that number does include spam which actually makes up a large proportion (about half in 2015).
It is also estimated there are currently over 4 billion email addresses – unfortunately that doesn’t quite mean that more than half the planet’s population has email, as quite a few people have more than one email address, and also computer programs can have an email address of their own.
Tomlinson was co-author on an early standards document RFC-561: Standardizing Network Mail Headers (5 Sep 1973), which was one of the predecessors of the current email standard RFC-822: Standard for the format of ARPA Internet Text Messages (13 Aug 1982).
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