Welcome
Username or Email:

Password:


Missing Code




[ ]
[ ]
Online
  • Guests: 76
  • Members: 0
  • Newest Member: omjtest
  • Most ever online: 396
    Guests: 396, Members: 0 on 12 Jan : 12:51
Members Birthdays:
All today's birthdays', congrats!
dan (37)
rchydro (64)
CapRack (30)


Next birthdays
11/07 Dave Marshall (40)
11/07 Worms (46)
11/08 Bert (77)
Contact
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.
Forums
4hv.org :: Forums :: General Science and Electronics
« Previous topic | Next topic »   

Geiger counter design and prospects of scintillation spectroscopy

Move Thread LAN_403
Carbon_Rod
Mon Apr 08 2013, 09:02AM Print
Carbon_Rod Registered Member #65 Joined: Thu Feb 09 2006, 06:43AM
Location:
Posts: 1155
Just curious if anyone knows whether its possible to differentiate the emission energy level of Geiger tube spikes.

For example, does the spark gap avalanche event settling-time differ with ionizing sources?

Cheers,
Rod
Back to top
Steve Conner
Mon Apr 08 2013, 09:21AM
Steve Conner Registered Member #30 Joined: Fri Feb 03 2006, 10:52AM
Location: Glasgow, Scotland
Posts: 6706
Short answer: No. Geiger tubes operate in the avalanche region, every discharge is a complete discharge of the tube. Different particles may touch it off in subtly different ways, but the information is lost in the resulting chaos. Essentially you have a flattened ski resort and you're trying to figure out exactly which snowflake started the avalanche. smile

Long answer: Your Geiger tube may show a "proportional region" when it's operated below its rated voltage. Link2
Back to top
Carbon_Rod
Mon Apr 08 2013, 10:07AM
Carbon_Rod Registered Member #65 Joined: Thu Feb 09 2006, 06:43AM
Location:
Posts: 1155
Are they sampling a ramp generator (~80v to 400v) to garner “trigger” thresholds?

Would the method generalize to an alpha "spark detector"?
Link2


The Neon indicator tube in series with the Geiger tube tends to vary in intensity under background events, and it is operating at a well regulated 400v. Hypothetically, if it were completely discharged every event than when a Geiger tube enters into the saturation “glow” condition it would remain discharged. Which wouldn't make sense.... confused I am... wink

Cheers,
Back to top
Uspring
Mon Apr 08 2013, 03:46PM
Uspring Registered Member #3988 Joined: Thu Jul 07 2011, 03:25PM
Location:
Posts: 711
CR wrote:
Are they sampling a ramp generator (~80v to 400v) to garner “trigger” thresholds?
No you would stay with a voltage just below the point of a continuous discharge. If you want to do spectroscopy you need to pick up the pulse height. Alphas typically produce a few thousand ion/electron pairs, which are multiplied somewhat in the proportional regime. You need low noise amps to do that.

Back to top
Proud Mary
Mon Apr 08 2013, 10:13PM
Proud Mary Registered Member #543 Joined: Tue Feb 20 2007, 04:26PM
Location: UK
Posts: 4992
Have a read of this essential GM tube theory manual from Centronics: Link2

Steve is right to say that some GM tubes can be operated in proportional mode. A few of the common Cold War era Russian GM tubes give proportional mode parameters in their data sheets. This is generally a band about 20V wide before the start of the GM plateau region.

Proportional mode requires a low noise linear pre-amp which can accurately amplify the pulses while maintaining their relative pulse amplitude. Discriminators can then sort these out into the number of bins appropriate to the practical resolution of the instrument.
Back to top
Carbon_Rod
Tue Apr 09 2013, 06:36AM
Carbon_Rod Registered Member #65 Joined: Thu Feb 09 2006, 06:43AM
Location:
Posts: 1155
I was looking into the various tubes listed on this site:
Link2

These look like interesting options, but do not seem to disclose proportional operation:
LND7317,LND712,SBT11A

@Steve
Alternately, would it be possible to avoid proportional methods by using a precision Aluminum coated mica filter wheel to selectively retard beta emission. Thus, forming a profile by automatically stepping through 0.001mm to 1.000mm shielding on the tube aperture over several hours, and removing the background profile after each exposure interval. I am curious if anyone has attempted building a similar apparatus. smile

Thanks for the link PM, I will look over the info.
Rod
Back to top
Uspring
Tue Apr 09 2013, 08:52AM
Uspring Registered Member #3988 Joined: Thu Jul 07 2011, 03:25PM
Location:
Posts: 711
Carbon Rod wrote:
Alternately, would it be possible to avoid proportional methods by using a precision Aluminum coated mica filter wheel to selectively retard beta emission.
Alphas have a much shorter range than betas. You can't shield against betas and not block alphas.
In a thin, transmissive type detector, an alpha will leave a higher signal than a beta due to its fatter ionisation track. If you're sensitive to pulse height, you might be able to distinguish between them.
Alternatively you could place a somewhat shielded (alpha insensitive) detector behind a thin alpha detector and use anticoincidence. A signal in both detectors will signal a beta and a signal only in the first one an alpha.

Back to top
Proud Mary
Tue Apr 09 2013, 10:49AM
Proud Mary Registered Member #543 Joined: Tue Feb 20 2007, 04:26PM
Location: UK
Posts: 4992
The use of filtration using filters of known properties - such as a sheet of thin aluminium foil - has been a basic analytic procedure since the invention of the GM tube in 1928. At the risk of over-simplification, if all the radiation from a sample is blocked by aluminium foil, then you have an alpha only emitter. If none of it is stopped measurably by 1 mm Pb, then it is gamma rays, and so on.

A great deal more can be done with GM tubes than simply detecting the presence or absence of radiation. Have a look at this wonderful old classic from the Golden Age of gaseous detector technology:

The use of the Geiger-Müller counter X-ray spectrometer in an X-ray laboratory, with special reference to automatic recording Link2
Back to top

Moderator(s): Chris Russell, Noelle, Alex, Tesladownunder, Dave Marshall, Dave Billington, Bjørn, Steve Conner, Wolfram, Kizmo, Mads Barnkob

Go to:

Powered by e107 Forum System
 
Legal Information
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.