If you need assistance, please send an email to forum at 4hv dot org. To ensure your email is not marked as spam, please include the phrase "4hv help" in the subject line. You can also find assistance via IRC, at irc.shadowworld.net, room #hvcomm.
Support 4hv.org!
Donate:
4hv.org is hosted on a dedicated server. Unfortunately, this server costs and we rely on the help of site members to keep 4hv.org running. Please consider donating. We will place your name on the thanks list and you'll be helping to keep 4hv.org alive and free for everyone. Members whose names appear in red bold have donated recently. Green bold denotes those who have recently donated to keep the server carbon neutral.
Special Thanks To:
Aaron Holmes
Aaron Wheeler
Adam Horden
Alan Scrimgeour
Andre
Andrew Haynes
Anonymous000
asabase
Austin Weil
barney
Barry
Bert Hickman
Bill Kukowski
Blitzorn
Brandon Paradelas
Bruce Bowling
BubeeMike
Byong Park
Cesiumsponge
Chris F.
Chris Hooper
Corey Worthington
Derek Woodroffe
Dalus
Dan Strother
Daniel Davis
Daniel Uhrenholt
datasheetarchive
Dave Billington
Dave Marshall
David F.
Dennis Rogers
drelectrix
Dr. John Gudenas
Dr. Spark
E.TexasTesla
eastvoltresearch
Eirik Taylor
Erik Dyakov
Erlend^SE
Finn Hammer
Firebug24k
GalliumMan
Gary Peterson
George Slade
GhostNull
Gordon Mcknight
Graham Armitage
Grant
GreySoul
Henry H
IamSmooth
In memory of Leo Powning
Jacob Cash
James Howells
James Pawson
Jeff Greenfield
Jeff Thomas
Jesse Frost
Jim Mitchell
jlr134
Joe Mastroianni
John Forcina
John Oberg
John Willcutt
Jon Newcomb
klugesmith
Leslie Wright
Lutz Hoffman
Mads Barnkob
Martin King
Mats Karlsson
Matt Gibson
Matthew Guidry
mbd
Michael D'Angelo
Mikkel
mileswaldron
mister_rf
Neil Foster
Nick de Smith
Nick Soroka
nicklenorp
Nik
Norman Stanley
Patrick Coleman
Paul Brodie
Paul Jordan
Paul Montgomery
Ped
Peter Krogen
Peter Terren
PhilGood
Richard Feldman
Robert Bush
Royce Bailey
Scott Fusare
Scott Newman
smiffy
Stella
Steven Busic
Steve Conner
Steve Jones
Steve Ward
Sulaiman
Thomas Coyle
Thomas A. Wallace
Thomas W
Timo
Torch
Ulf Jonsson
vasil
Vaxian
vladi mazzilli
wastehl
Weston
William Kim
William N.
William Stehl
Wesley Venis
The aforementioned have contributed financially to the continuing triumph of 4hv.org. They are deserving of my most heartfelt thanks.
Registered Member #1938
Joined: Sun Jan 25 2009, 12:44PM
Location: Romania
Posts: 701
It looks like rain, today! Let's see how good is that case. I don't expect any issues, though.
Maybe some interesting data related to this phenomenon?
A friend working in this field, indicated that the level of radiation detected by the device should stay almost constant. He indicated I should use a ion chamber to better track the Radon variations.
So we'll probably see a new "sensor" added to the device, soon.
Stella, what is your experience with those giga-ohmic resistors that you've purchased earlier? Are they any good? I was looking for something similar, and I found a 1000GOhm glass resistor I'm tempted to purchase.
I also got the DHT-22 sensor, and now I'm thinking about replacing the DHT-11 currently in use. If only the two humidity scales would match ...
Registered Member #543
Joined: Tue Feb 20 2007, 04:26PM
Location: UK
Posts: 4992
radhoo wrote ...
A friend working in this field, indicated that the level of radiation detected by the device should stay almost constant. He indicated I should use a ion chamber to better track the Radon variations.
So we'll probably see a new "sensor" added to the device, soon.
"almost constant" I have been able to track small but distinct diurnal variations over 24 hour periods - a sine wave - which has been known since the early day of cosmic ray research. Google: "On the Interpretation of the Diurnal Variation of Cosmic Rays" which is a pdf I couldn't link to. It is an old one, but nice and clear for all that!
If you look through the skyshine and 'Background as a Residual Radioactivity Criterion' papers, you'll see that it is these small changes in background that contain almost all the interesting information, and what makes long term observation worthwhile. Once you have a base-line figure from months of obeservation, you'll be able to detect these smaller changes and trends, all of which have a reason behind them which it is our business to understand.
Now as for Rn-222, its daughters, and their alpha emissions, clearly these cannot be detected with a non-window GM tube, and would be much better detected with an ionisation chamber (if there are enough of them) or a scintillation device and MCA. BUT, alpha ranges are but a few cms, as we know, so alpha detection in the open air is a specialised business (as far as I understand it). Most concern about Rn is in the domestic indoors, especially in cellars, where the gas can seep up from rocks below, and accumulate to hazardous levels due to want of ventilation. In Britain, long term alpha dosimetry in high radon areas like Cornwall has been done with photochemical film badges, and more recently Track Etch Detectors, which the householder sends off to a government laboratory every three months or so. I do not think you will get any results worth having if you fix an ionisation chamber to the outisde of your house.
radhoo wrote ...
Stella, what is your experience with those giga-ohmic resistors that you've purchased earlier? Are they any good? I was looking for something similar, and I found a 1000GOhm glass resistor I'm tempted to purchase.
Registered Member #311
Joined: Sun Mar 12 2006, 08:28PM
Location:
Posts: 253
Does having a full-wave rectifier make much difference vs. half-wave? With a single-ended drive like this you get most of the output on one polarity, so you may find you can lose 3 of the diodes with minimal performance loss. Obviously you do then need to make sure the windings are the right way round.
wrote ... Saturation alarm: if the tube becomes paralyzed by high dose rate as in an X-ray beam.
I noticed this when sending a counter through my baggage x-ray (150kVp) - counts increase as it approaches the beam but it then goes silent til it comes out the other side.
Registered Member #1938
Joined: Sun Jan 25 2009, 12:44PM
Location: Romania
Posts: 701
@Ash Small, thanks mate.
@Mike, While not essentially important for the tube itself, you will want to minimize the ripple effect to its maximum extent, to make sure the detector runs undisturbed by various interference factors. Especially the detector/counter part. Let's take a look at the following two photos:
1.The first, shows my version 3.2 inverter output, that uses a NPN oscillating transistor in an Armstrong oscillator, and a feedback mechanism constructed with zenner diodes set for 400V, that triggers an oscillator-blocking second transistor. See the trace for CH1 - yellow, set for 400V
2. The second shows the output in 3.3, fully rectified and produced by a a precisely calculated PWM signal. See the CH2, cyan trace, set for 350V
I have plenty of diodes and do not feel the need to spare any of them, given the nice improvement in the results. But yes, it is possible to only use a single diode to rectify the inverter's output. I just don't see any reason for doing that.
Registered Member #30
Joined: Fri Feb 03 2006, 10:52AM
Location: Glasgow, Scotland
Posts: 6706
I don't understand how these scope traces show an improvement in the results. They are traces of two different things. The first one shows the high voltage AC output before the rectifier and smoothing capacitors, the second one shows the smoothed DC.
Registered Member #1938
Joined: Sun Jan 25 2009, 12:44PM
Location: Romania
Posts: 701
Steve Conner wrote ...
I don't understand how these scope traces show an improvement in the results. They are traces of two different things. The first one shows the high voltage AC output before the rectifier and smoothing capacitors, the second one shows the smoothed DC.
Steve, they both show "DC" , in the same place, right before the 10M resistor connected to the tube's anode.
Remember that for the first trace, there is an oscillator blocker transistor, controlled by the zenners for voltage regularization. This is why we see those huge variations, but also a frequency value is being computed by the scope. Circuit diagram here: . Scope connected before R2.
This site is powered by e107, which is released under the GNU GPL License. All work on this site, except where otherwise noted, is licensed under a Creative Commons Attribution-ShareAlike 2.5 License. By submitting any information to this site, you agree that anything submitted will be so licensed. Please read our Disclaimer and Policies page for information on your rights and responsibilities regarding this site.