Fermi 2 had minor fuel failure in the late 1990s; however Cm-242 is not at a 
low ratio in all our smear samples.  For example in refuel floor samples and 
Chem sample sink samples, Cm-242 is as much as half of total alpha activity, 
whereas in more "legacy" type samples (not exposed to fresh reactor water) such 
as drywell basement, drywell sump, inside MSIVs, etc., Cm-242 has the lowest 
alpha activity or is not detected.  This is despite our having negligible fuel 
leakage in recent years.    

 
Tom VanderMey, CHP
Principal Radiological Engineer
DTE Energy, Fermi 2
734-586-1539



[email protected] wrote: -----


To: [email protected]
From: [email protected]
Sent by: [email protected]
Date: 11/13/2012 04:12PM
Subject: Re: Powernet: alpha scaling factor

Zusanne,

San Onofre's mixture has been aging since the mid 1980's.    Our aged 
distributions show >50% Am-241, which grows in from the decay of Pu-241. 
The other major component is Cm244 (T1/2=18 years).   Fresh failed fuel 
has ~50% Cm-242 (T1/2=163 day), which at San Onofre is now <1%.

Mike Russell
949.368.7638




From:   "Ziegler, Susanne E." <[email protected]>
To:     "'[email protected]'" <[email protected]>
Date:   11/13/2012 09:47 AM
Subject:        Powernet: alpha scaling factor
Sent by:        [email protected]



I am interested in typically what alpha isotopes you are seeing during 
your characterizations.  I realize each plant has a different history of 
fuel damage, and cleanup.  I'm am wondering if a typical ratio of Cm-242 
to Pu-138 can be determined.  sue
 
Susanne Ziegler
PSEG Radiation Protection
Hope Creek Generating Station
PO Box 236, MC H05
Hancocks Bridge, NJ 08038
856-339-5143
FAX 856-339-3336
 
Gadugi-working together for a common good
 
 
 
 

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