Skip to main content

NOTICE: Due to a lapse in annual appropriations, most of this website is not being updated. Learn more.

Form submissions will still be accepted but will not receive responses at this time. Sections of this site for programs using non-appropriated funds (such as NVLAP) or those that are excepted from the shutdown (such as CHIPS and NVD) will continue to be updated.

U.S. flag

An official website of the United States government

Official websites use .gov
A .gov website belongs to an official government organization in the United States.

Secure .gov websites use HTTPS
A lock ( ) or https:// means you’ve safely connected to the .gov website. Share sensitive information only on official, secure websites.

Explanation of (hhl)f Habit Planes in Ferrous Alloys

Published

Author(s)

H M. Ledbetter, Martin Dunn

Abstract

We give a possible explanation of the remarkable habit-plane measurements reported by Kajiwara for Fe-Ni-Mn alloys. Examining small, thin (early-stage), martensite plates, Kajiwara found that all habit-plane normals fall on the (hhl)f line, spanning about 25 degrees from approximately (114)f to (223)f. Despite numerous suggested modifications, the crystallographic theories of Wechsler-Lieberman-Read and Bowles-Mackenzie fail to predict habit planes on the (hhl)f line, let alone variations along the line. Kajiwara invoked Suzuki's prism-matching theory, which contains an anisotropic interface distortion, an adjustable parameter contrary to more recent measurements. Our explanation arises from another, more general approach: inclusion theory, which includes crystallographic-theory predictions as the zero-elastic-strain-energy limit.
Citation
Explanation of (hhl)<sub>f</sub> Habit Planes in Ferrous Alloys

Keywords

crystallography, ferrous alloys, habit planes, inclusion theory, martensite

Citation

Ledbetter, H. and Dunn, M. (2008), Explanation of (hhl)<sub>f</sub> Habit Planes in Ferrous Alloys, Explanation of (hhl)<sub>f</sub> Habit Planes in Ferrous Alloys (Accessed October 9, 2025)

Issues

If you have any questions about this publication or are having problems accessing it, please contact [email protected].

Created October 16, 2008
Was this page helpful?