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Michael Weissman Mills, Andrea Christine 2015-09-25T20:02:49Z 2015-09-25T20:02:49Z 10000-01-01 2004 2004 Finally, returning to pinning field statistics, a comparison of the length-scales involved in avalanche size distributions, temporal Barkhausen power spectra, and spatial pinning field power spectra illustrates that the most recent justification for the statistics of the effective pinning field is incomplete. Made available in DSpace on 2015-09-25T20:02:49Z (GMT). No. of bitstreams: 2 license.txt: 4848 bytes, checksum: 96035ab3f5e1c23cc7138a224ce498bd (MD5) 3160926.pdf: 4105850 bytes, checksum: a902ba433e5d974d4c453c87cbb6c485 (MD5) Previous issue date: 2004 Embargo set by: Seth Robbins for item 81789 Lift date: Forever Reason: Restricted to the U of I community idenfinitely during batch ingest of legacy ETDs Restricted to the U of I community idenfinitely during batch ingest of legacy ETDs U of I Only 95 p. Thesis (Ph.D.)--University of Illinois at Urbana-Champaign, 2004. http://hdl.handle.net/2142/80507 (MiAaPQ)AAI3160926 eng Physics, Condensed Matter Barkhausen Noise Studies: Pinning Field Statistics and Time-Asymmetries text Physics Physics University of Illinois at Urbana-Champaign Dissertation Ph.D.