Abstract
A number of group IVA iron meteorites show metallographic features suggesting that a shock annealing event intervened during the formation of the Widmanstatten structure. This could complicate the estimation of cooling rates based on diffusion profile methods but would have less influence on methods based upon macroscopic measurements of kamacite band widths.
Sign-in/Register to access full text options 
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a callDisclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.
