Powered by OpenAIRE graph
Found an issue? Give us feedback
image/svg+xml Jakob Voss, based on art designer at PLoS, modified by Wikipedia users Nina and Beao Closed Access logo, derived from PLoS Open Access logo. This version with transparent background. http://commons.wikimedia.org/wiki/File:Closed_Access_logo_transparent.svg Jakob Voss, based on art designer at PLoS, modified by Wikipedia users Nina and Beao Journal of Geophysic...arrow_drop_down
image/svg+xml Jakob Voss, based on art designer at PLoS, modified by Wikipedia users Nina and Beao Closed Access logo, derived from PLoS Open Access logo. This version with transparent background. http://commons.wikimedia.org/wiki/File:Closed_Access_logo_transparent.svg Jakob Voss, based on art designer at PLoS, modified by Wikipedia users Nina and Beao
Journal of Geophysical Research Atmospheres
Article . 1993 . Peer-reviewed
License: Wiley Online Library User Agreement
Data sources: Crossref
versions View all 1 versions
addClaim

Chemical remanent magnetization during γFeOOH phase transformations

Authors: Özden Özdemir; David J. Dunlop;

Chemical remanent magnetization during γFeOOH phase transformations

Abstract

We have studied chemical remanent magnetization (CRM) accompanying the phase transformations lepidocrocite (γFeOOH) → maghemite (γFe2O3) → hematite (αFe2O3) in a field of 50 μT at a series of 13 temperatures from 200 to 650°C. CRM intensity peaked after the 250°C run as paramagnetic lepidocrocite transformed to ferrimagnetic maghemite of single‐domain size. After the 275, 300 and 350°C runs, CRM intensity decreased about an order of magnitude, probably because of the formation of antiphase domains with oppositely coupled magnetizations in the maghemite. A second CRM peak after the 400°C run is thought to reflect the growth of hematite on antiphase boundaries, breaking the negative coupling and allowing maghemite antiphase domains to align individually with the field. After runs at 450°C and above, CRM intensities were very low and the CRM consisted of two vectors, sometimes reversed in direction to each other and always at a large angle to the field. The explanation seems to lie in perpendicular coupling of the magnetic sublattices of maghemite and hematite.

  • BIP!
    Impact byBIP!
    selected citations
    These citations are derived from selected sources.
    This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
    39
    popularity
    This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
    Top 10%
    influence
    This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
    Top 10%
    impulse
    This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
    Average
Powered by OpenAIRE graph
Found an issue? Give us feedback
selected citations
These citations are derived from selected sources.
This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Citations provided by BIP!
popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
BIP!Impulse provided by BIP!
39
Top 10%
Top 10%
Average
Upload OA version
Are you the author of this publication? Upload your Open Access version to Zenodo!
It’s fast and easy, just two clicks!