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#31
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Sun noise
Jim Lux wrote in
: .... Indeed, this would be a very challenging measurement, because you also have to take into account the match of that load, and if it's just a Jim, an important point, and more generally on the mismatch issue... It seems that many measuring sun noise rise prefer to measure the rise by attenuator substitution. Though it seems a simple and sound method of measurement, the effects of mismatch need to be considered, not only on the power delivered to the receiver chain, but also the noise figure of the device with the changing input or output loads. The effects are not necessarily easy to quantify, which makes the apparently simple method a bit of a trap. Owen |
#32
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Sun noise
On Mon, 27 Aug 2007 23:02:06 GMT, Owen Duffy wrote:
Indeed, this would be a very challenging measurement, because you also have to take into account the match of that load, and if it's just a Jim, an important point, and more generally on the mismatch issue... Hi All, Given the notoriety that follows discussion about the Real component of the transmitter's source Z.... Let's see, How do I measure thee, let me count the ways. Anyone want to venture a guess on the value of the Real component of the receivers load Z? (And then we game this into the S-9 50µV across those myriad resistors.) 73's Richard Clark, KB7QHC |
#33
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Sun noise
Owen Duffy wrote in news:Xns999955EE72868nonenowhere@
61.9.191.5: Dave Oldridge wrote in 9: Near as I could measure it, the NF of the receiver after my mod was 1.2db. I had to resort to boiling and freezing water and a tiny dummy load to measure it at all. I haven't tried hot/cold tests using ice and boiling water, I didn't think it was practical. Only just and you need a good 4-digit or better AC voltmeter to do it at all. I wasn't after accuracy, just a ball-park estimate and I know I got it fairly close because the receiver did show a marked increase in noise when any decent antenna was connected. You finally measured a receiver noise temperature of 50K with hot and cold loads of 270 and 370. That means a Y factor of 1.059dB. If Y were just 0.1dB greater, NF would be 0.78dB, 0.1dB lower and, NF would be 1.66dB. Yep...the most I'd be willing to commit to with that measurement would be that it was below around 2.5 and PROBABLY fairly close to my measurement. I measured the voltages alternately 25 times and took a mean to try to smooth out the errors. With this configuration the sensitivity of NF to changes in Y are extreme, 0.4dB change in NF per 0.1dB change in Y around that point. If you made the Y measurements using the audio output of a narrow band receiver, it is very hard to make high resolution measurements (eg to 0.01dB resolution) with say, a multimeter. It is. You need a good AC voltmeter with decent digital accuracy and resolution and you have to average a bunch of readings. I have done these tests with a liquid nitrogen cooled load and room temperature load, and that gives more practical Y ratios, 3.7dB for a 1.2dBNF, and the sensitivity in NF is 0.08dB per 0.1dB change in Y. This still demands high resolution measurement of noise power. Yes, anything less than 4 digits is just about useless. -- Dave Oldridge+ ICQ 1800667 |
#34
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Sun noise
Dave Oldridge wrote in
9: Owen Duffy wrote in news:Xns999955EE72868nonenowhere@ 61.9.191.5: .... If you made the Y measurements using the audio output of a narrow band receiver, it is very hard to make high resolution measurements (eg to 0.01dB resolution) with say, a multimeter. It is. You need a good AC voltmeter with decent digital accuracy and resolution and you have to average a bunch of readings. I put some notes together on a perspective of the noise measurement (sampling) process and its statistical uncertainty, they are at http://www.vk1od.net/fsm/nmu.htm . It is my experience that a digital voltmeter probably samples for something around 100ms, and with a 2kHz wide noise bandwidth, you might expect an uncertainty of near 0.5dB at the 90% confidence level. Just watch the readings bounce around. Sure, if you average 100 of those measurements (actually, you should get the root of the sum of the squares... because it is power you average, not voltage), you might reduce that uncertainty to around 0.05dB... but it is not a very practical manual method, if recording accuracy (ie writing down the wrong number) doesn't get you, environmental drift will. Owen |
#35
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Sun noise
Dave Oldridge wrote:
Owen Duffy wrote in news:Xns999955EE72868nonenowhere@ 61.9.191.5: Dave Oldridge wrote in . 159: Near as I could measure it, the NF of the receiver after my mod was 1.2db. I had to resort to boiling and freezing water and a tiny dummy load to measure it at all. snip This still demands high resolution measurement of noise power. Yes, anything less than 4 digits is just about useless. That would be necessary but not sufficient. I suspect that other aspects of the measurement introduce greater uncertainty than the voltmeter. For instance, do you know the reflection coefficient of the load to 4 digits? (that would be knowing Z to about 0.1 ohm, at the RF frequency of interest), and is it stable with temperature to that level? For instance, a high quality load from Maury Microwave (a 2610F ) is specified to have a VSWR of 1.005 from DC-1GHz, which is a reflection coefficient of 0.0025. But that's only at 25C. An Agilent metrology grade cal kit with N connectors specifies rho0.00398 for the lowband loads, but only within 1 degree of the specified temperature. See, for example: http://cp.literature.agilent.com/lit...5054-90049.pdf A good thinfilm resistor might have a tempco of 5 ppm, with metal film being around 50 ppm, and thick film more in the 200 ppm area. For a 100 degree change, that's a 500 ppm (for the thin film) or a reflection coefficient change of 0.00025. Clearly one doesn't want to use any old resistor for the calibration load here. Measuring RF power to an accuracy of 1% is challenging. Your system is measuring a change in noise power of 100K out of 300K, roughly, so you've got a 30% change in noise power into the system. The Y-factor method essentially plots two points (one at 273K another at 373K, if you're using ice and boiling water), and then calculates the intercept at 0K. Since zeroK is about 3 times farther away than the measurement's width, errors in the measurement are roughly tripled at the intercept, and then doubled because you're using two measurements, so an error of 1% in the power measurement leads to about 5% error in the NF (if you're around 100K) (and this also applies if you have consistent errors.. say both power measurements are 1% high, the NF will come back as 105K instead of 100K). A 5% measurement uncertainty for power (0.2dB) gets you about 25-30% uncertainty in NF. The best way to improve the accuracy is to push the low temperature lower (e.g. with dry ice (195K) or LN2 (77K)), but that, of course, aggravates the change in reflection coefficient of your load with temperature. |
#36
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Sun noise
Jim Lux wrote in news:46D463CF.1080309
@jpl.nasa.gov: Dave Oldridge wrote: Owen Duffy wrote in news:Xns999955EE72868nonenowhere@ 61.9.191.5: Dave Oldridge wrote in .159: Near as I could measure it, the NF of the receiver after my mod was 1.2db. I had to resort to boiling and freezing water and a tiny dummy load to measure it at all. snip This still demands high resolution measurement of noise power. Yes, anything less than 4 digits is just about useless. That would be necessary but not sufficient. .... Just following through on the '4 digit' issue... I have done two series of 250 measurements of audio noise voltage from a SSB receiver using two different digital multimeters, the 9932 is a modern digital multimeter that is NOT true RMS responding, and the 506 is a modern digital multimeter that is true RMS responding with bandwidth adequate to cover the receiver output response. From observation with a stopwatch, I estimate that the 9932 updates 3 times per second, and the 506 updates 2 times per second. The integration times are probably .33 and .5 seconds respectively. I have measured the receiver equivalent noise bandwidth and it is 1600Hz. 95% of 250 readings were within 0.41dB for the 9932 and 0.31dB for the 506. These observations reconcile well with my Chi-squared based estimate of the uncertainty that I referred to in an earlier post. As for the number of digits, they are both 4 digit multimeters which doesn't mean a lot. They were used to measure 200mV with 1mV resolution, so the representational error is 0.04dB. The error due to the number of digits in this downscale three digit application is insignificant compared to the sampling error of 0.4dB and 0.3dB. Graphically, the distributions are shown at http://www.vk1od.net/nfm/temp.gif . Different meters with different integration times, and different receivers with different noise bandwidth will result in different outcomes, but I argue that the uncertainty is predictable. Owen |
#37
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Sun noise
On Thu, 30 Aug 2007 10:11:22 GMT, Owen Duffy wrote:
they are both 4 digit multimeters which doesn't mean a lot. They were used to measure 200mV with 1mV resolution, Hi Owen, The convention for decades has been to describe them as 3½ Digits, or 2000 count, not 4 digit unless they could represent 9999. Adding digits does not generally add precision, resolution, monotonicity, or accuracy. However, as it costs money to add a digit, the underlying circuitry could usually support "some" of these attributes. Better instruments perform rounding after the last digit. 73's Richard Clark, KB7QHC |
#38
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Sun noise
Owen Duffy wrote:
Jim Lux wrote in news:46D463CF.1080309 @jpl.nasa.gov: Dave Oldridge wrote: Owen Duffy wrote in news:Xns999955EE72868nonenowhere@ 61.9.191.5: Dave Oldridge wrote in 5.159: Near as I could measure it, the NF of the receiver after my mod was 1.2db. I had to resort to boiling and freezing water and a tiny dummy load to measure it at all. snip This still demands high resolution measurement of noise power. Yes, anything less than 4 digits is just about useless. That would be necessary but not sufficient. ... Just following through on the '4 digit' issue... I have done two series of 250 measurements of audio noise voltage from a SSB receiver using two different digital multimeters, the 9932 is a modern digital multimeter that is NOT true RMS responding, and the 506 is a modern digital multimeter that is true RMS responding with bandwidth adequate to cover the receiver output response. From observation with a stopwatch, I estimate that the 9932 updates 3 times per second, and the 506 updates 2 times per second. The integration times are probably .33 and .5 seconds respectively. I have measured the receiver equivalent noise bandwidth and it is 1600Hz. 95% of 250 readings were within 0.41dB for the 9932 and 0.31dB for the 506. These observations reconcile well with my Chi-squared based estimate of the uncertainty that I referred to in an earlier post. As for the number of digits, they are both 4 digit multimeters which doesn't mean a lot. They were used to measure 200mV with 1mV resolution, so the representational error is 0.04dB. Gotta be a bit careful there, because quantization error has a uniform distribution, so the variance is 1/12 of the span. This is different than the (presumably) normally distributed actual measurands. When giving an uncertainty (sampling error), one should also say whether it's a one sigma, two sigma, or 3 sigma number. *Standard uncertainty* is 1 sigma... *expanded uncertainty*, often given as a +/- number is usually the 95% percent confidence interval, which, for normal distributions, is 2 sigma given your statistics above, you would be giving the expanded uncertainty as 0.41dB By the way, unless your device actually directly measures dB (e.g. it has a log detector) or the errors are inherently ratios, it's probably better to give the value in a linear scale (milliwatts?) with the uncertainty in the same units. That gets you around the "ratio" problem where log(1+delta) -log(1-delta) http://physics.nist.gov/cuu/Uncertainty/index.html has the simple explanation, and the technical note (TN1297) , and references to the ISO Guide to Expression of Uncertainty in Measurment (aka the GUM) The error due to the number of digits in this downscale three digit application is insignificant compared to the sampling error of 0.4dB and 0.3dB. Graphically, the distributions are shown at http://www.vk1od.net/nfm/temp.gif . Different meters with different integration times, and different receivers with different noise bandwidth will result in different outcomes, but I argue that the uncertainty is predictable. Indeed, it is. Owen |
#39
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Sun noise
Jim Lux wrote in
: Owen Duffy wrote: ... Just following through on the '4 digit' issue... I have done two series of 250 measurements of audio noise voltage from a SSB receiver using two different digital multimeters, the 9932 is a modern digital multimeter that is NOT true RMS responding, and the 506 is a modern digital multimeter that is true RMS responding with bandwidth adequate to cover the receiver output response. From observation with a stopwatch, I estimate that the 9932 updates 3 times per second, and the 506 updates 2 times per second. The integration times are probably .33 and .5 seconds respectively. I have measured the receiver equivalent noise bandwidth and it is 1600Hz. 95% of 250 readings were within 0.41dB for the 9932 and 0.31dB for the 506. These observations reconcile well with my Chi-squared based estimate of the uncertainty that I referred to in an earlier post. As for the number of digits, they are both 4 digit multimeters which doesn't mean a lot. They were used to measure 200mV with 1mV resolution, so the representational error is 0.04dB. Gotta be a bit careful there, because quantization error has a uniform distribution, so the variance is 1/12 of the span. This is different than the (presumably) normally distributed actual measurands. Ok, point taken. I think more correctly, the maximum error would be 20 *log(1+1/200/2) or 0.0217dB. The expected error due to representation in three digits does not account for the variation in measurements. When giving an uncertainty (sampling error), one should also say whether it's a one sigma, two sigma, or 3 sigma number. *Standard uncertainty* is 1 sigma... *expanded uncertainty*, often given as a +/- number is usually the 95% percent confidence interval, which, for normal distributions, is 2 sigma Whilst it might be reasonable to assume that the combined error in measurement of a high S/N sine wave voltage might be normally distributed, and that might also be true of measurement of noise voltage in some circumstances, I propose that measurement of noise power in narrow bandwidth with short integration times is distributed as Chi- squared and the number of samples becomes relevant in determining the number of degrees of freedom for the distribution. For this reason, I have talked about a confidence level rather than sigma (which is more applicable to normally distributed data). Just for interest, in the case of the 9932 measurement set: Average=0.201, sigma=0.0046, 1sigma based uncertainty estimate=0.20dB, 2sigma based uncertainty estimate=0.41dB, 3sigma based uncertainty estimate=0.62dB. given your statistics above, you would be giving the expanded uncertainty as 0.41dB I stated it as 95% of obs within 0.41, I should have said 95% of obs within +/-0.41, I was explicit about the implied confidence, the 95% doesn't equate to either the 1sigma or 3sigma confidence, it is very close to the 2sigma confidence (95.45%), and it is at the high confidence end of the scale. By the way, unless your device actually directly measures dB (e.g. it has a log detector) or the errors are inherently ratios, it's probably better to give the value in a linear scale (milliwatts?) with the uncertainty in the same units. That gets you around the "ratio" problem where log(1+delta) -log(1-delta) I understand what you mean in your last sentence. I did record the voltage, and converted the values to dB for analysis. The interval was calculated by taking the average of the 2.5 percentile and 97.5 percentile, which is an approximation, but as such small values is pretty close. I have converted results to dB to make it easier to see the relevance of the error or uncertainty, but in so doing, another (small in this case) error is introduced. http://physics.nist.gov/cuu/Uncertainty/index.html has the simple explanation, and the technical note (TN1297) , and references to the ISO Guide to Expression of Uncertainty in Measurment (aka the GUM) In terms of the above, I am proposing that measurements of narrowband noise with short integration time is not strictly normally distributed, and an estimate of its uncertainty to a given confidence level can be obtained from the Chi-square distribution. One could not estimate the results of the test from knowledge of the instrument accuracy (inherent and representational error) alone. I think the experiment supports the proposition that digital multimeters with typically short integration times do not deliver high resolution measurement of narrow band (eg SSB telephony) noise. The error due to the number of digits in this downscale three digit application is insignificant compared to the sampling error of 0.4dB and 0.3dB. Graphically, the distributions are shown at http://www.vk1od.net/nfm/temp.gif . Different meters with different integration times, and different receivers with different noise bandwidth will result in different outcomes, but I argue that the uncertainty is predictable. Indeed, it is. Thanks, appreciate the comments. Owen |
#40
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Sun noise
Richard Clark wrote in
: On Thu, 30 Aug 2007 10:11:22 GMT, Owen Duffy wrote: they are both 4 digit multimeters which doesn't mean a lot. They were used to measure 200mV with 1mV resolution, Hi Owen, The convention for decades has been to describe them as 3½ Digits, or 2000 count, not 4 digit unless they could represent 9999. Adding digits does not generally add precision, resolution, monotonicity, or accuracy. However, as it costs money to add a digit, the underlying circuitry could usually support "some" of these attributes. Better instruments perform rounding after the last digit. Hi Richard, It is interesting in marketing hype that reference is made to 2 digit and 3 digit instruments, which implies a log based metric (10*log (MaxReading)) when you assume a 'full count', and the same hype refers to the upper digit if it can only have values of 0 or 1 as half a digit, whereas it probably has a weight of log(0.5) or 0.3... so in utility terms, a 2 1/2 digit instrument is really a 2.3 digit instrument. In my case, I was making the measurements straddling 200mV, so I needed a bit of headroom for outliers, say 1dB or 225mV fsd, so it was effectively 2.35 digit instrument if you followed that argument. Nevertheless, the error introduced by the resolution issue and instrument accuracy does not explain the experimental results... something else is happening, and one needs to look beyond the instrument itself to form a realistic view of measurement uncertainty when measuring narrowband noise. Owen |
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