I have several instruments and software packages that can create screen captures, and the capture files commonly need some mix of image processing including for example:
- brightness, contrast, gamma adjustment;
- transparency change;
- format conversion; and
- file copy / archive / cleanup.
Above is an example. Though WordPress presents a small image inline, if you click on it, there is a 640×480 image that was created from a QVGA (320×240) screen capture file scaled and gamma adjusted.
Continue reading Standardised processing of instrument screen captures
I mentioned elsewhere that I dowloaded the WSPR archive for 1/08/2017, and particularly analysed 40m spots.
There were close to 1,000,000 spots for the day, about 340,000 on 40m, and about 20,000 individual transmissions reported during the day (40m).
Tx / Rx mix
Above is a pie chart of the mix of Tx Only, Rx ONLY and Tx/Rx stations. The largest group is Tx Only, 44% of stations do not contribute reception records. Nextly, 30% are Rx Only, and 27% Tx and Rx. Continue reading WSPR – data mining 40m 01/08/2017
On the back of A WSPR experiment for station evaluation I thought I would try a similar experiment on 30m in the quest for some meaningful results.
Given the lack of activity from credible stations on 40m, it seemed worth a checkout on 30m befor committing to the trial run, large download and data analysis.
So, I ran WSPR for a half hour just before 0000Z and observed the activity on WSPRnet map. I should note that my tx power was 0.1W and rx performance was impaired as there was a 20dB attenuator in line to achieve the tx power.
Above, the map after of the half hour of activity.
The encouraging this was that there were 12 stations active. Continue reading WSPR checkout on 30m
An experiment was conducted on 40m using WSPR to compare my own station transmit performance with others relatively close by.
The experiment was conducted around sunset on 01/08/2017, data was collected for the period 0600Z to 0900Z, sunset was at 07:17Z.
The experiment was unannounced as previous experience has been that if the WSPR community becomes aware of activity that does not accord with individual’s opinion of acceptable, the activity can be disrupted.
Data for analysis was fetched by downloading the archive which contained nearly 1,000,000 records for the day, and about 340,000 of those were 40m spots.
Factors shaping experiment design
The following is a discussion of various factors that weighed into experiment design.
Transmitters tend to cluster around the centre of the 200Hz WSPR band.
Above is a frequency distribution of tx frequency, and it is evident that the risk of interference is reduced by choosing a frequency near the upper or lower limit of the band segment. There was some activity just outside the designated band segment which might indicate care and competence of operators.
One wonders if randomising the tx frequency might not reduce collisions and improve decode rates. Continue reading A WSPR experiment for station evaluation
I was working recently on an antenna and a visitor was intrigued by a device I was using.
Above, the device is for tensioning a wire span, commonly called a come-along though that term gets applied to all manner for appliances for broadly similar purpose. A significant difference is that this was designed for smooth hard drawn copper wires, and has smooth flat jaws (70x6mm) and does not put a kink in the wire (as do most wire grips for more general fencing and FSWR use). This one has had the strap replaced, it came with a 1.25″ canvas reinforced rubber transmission belt which became hard over time. Continue reading Come-along from the past
On 5/10/2016 we cut over to a new broadband Internet access service, switching from Telstra 8Mb/s ADSL to iiNet NBN 12Mb/s.
Over some years, I have run an automated file transfer to measure the speed of our access service. The tests are done between 6:00 and 22:00, I am interested in performance during the times I want to use the service, and less interested in times when I would usually be sleeping.
One of the performance measures is speed, it seems simple enough especially when it is talked about by politicians and promoted by RSPs and NBN’s advertisements.
So, how does one characterise the speed. People like to think of simple concepts like ‘average’, but let us look at the distribution of speeds.
Above is a chart of the frequency distribution of speed observations for a week in March 2017. It is not in the form of the Normal Distribution, the classic bell-shaped curve for which common parametric statistics like Mean (average) and Standard Distribution are meaningful, but it is a skewed distribution. Without knowing the characteristics of the distribution, it is a misuse of parametric statistics to apply parametric statistics like Mean (average) and Standard Distribution. Continue reading Review of 10 months of iiNet broadband Internet access
On the back of failure to buy decent BN-V11U batteries for my theodolite (Chinese BN-V11U NiMH replacement battery), A fall back was to fabricate a battery that would fit in the battery compartment.
Above is a battery pack made from 5 x 2/3A 1.6Ah NiMH cells. Continue reading Chinese batteries – 5 x 2/3A 1.6Ah NiMH cells
My theodolite uses the once common BN-V11U NiMH camcorder battery.
I purchased a replacement on eBay, they are getting harder to find since changes to regulations about transport of batteries, but there are still quite a few sellers. Continue reading Chinese BN-V11U NiMH replacement battery
This article is a brief review of some issues that were found with initial testing of a Hantek DSO8102E two channel 100MHz hand held oscilloscope.
The DSO8102E is a member of the DSO8000 series (DSO8060, DSO8070E, DSO8100E, DSO8150E, DSO8200E), and shares most specifications across the series.
The specifications are very impressive, and price at just under $1000 for a Chinese brand seemed reasonable (hand held oscilloscopes are expensive compared to bench oscilloscopes).
The test scenario was a practical application, observation of the data traffic to/from a DHT22 temperature and humidity sensor in the project ESP8266 IoT DHT22 temperature and humidity – evolution 2. Continue reading Review of Hantek DSO8102E hand held oscilloscope
This article documents a first project with the Espressif ESP8266 in its third evolution (based on ESP8266 IoT DHT22 temperature and humidity – evolution 2).
The objective is a module that will take periodic temperature and humidity measurements, and in this evolution publish them using a RESTful API.
The example platform used in this article is a Wemos D1Pro. In this case, the D1Pro is configured for an external antenna, and a modification is made to the board to add a 1N34A diode for the deep sleep reset circuit (NodeMCU devkit V1 deep sleep). A three pin right angle header to the top of the board (as seen) and another on the underside on the opposite edge to get GND, +5, +3, and D4 for the DHT22 data wire. There is less than $20 in parts in the pic above. Continue reading ESP8266 IoT DHT22 temperature and humidity – evolution 3