TY - JOUR
T1 - The Fine Structure of Spots in Electron Diffraction Resulting from the Presence of Planar Interfaces and Dislocations. V. Observations on Coherent Domain Boundaries
AU - de Ridder, R.
AU - van Landuyt, J.
AU - Gevers, R.
AU - Amelinckx, S.
PY - 1970
Y1 - 1970
N2 - Observations of the fine structure of electron diffraction spots due to the presence of coherent domain boundaries in ordered Ni4Mo are compared with theoretical results derived in part III of this paper. It is shown that the predicted fine structure consisting of satellites lying in a direction perpendicular to the image fringes can be observed. How‐ever, in general, only one or two out of the four predicted satellites are registered, the intensity of the other ones being too small. Analysis is made of the fine structure and excellent agreement between theory and experiment is found. Identification of the satellites, based among others on intensity considerations is possible and illustrated on an example. Moreover, the orientation parameters such as s, Δs, and the extinction distance can be estimated from the geometry and a method is outlined allowing to calculate the absorption length from the measured intensities of the satellites.
AB - Observations of the fine structure of electron diffraction spots due to the presence of coherent domain boundaries in ordered Ni4Mo are compared with theoretical results derived in part III of this paper. It is shown that the predicted fine structure consisting of satellites lying in a direction perpendicular to the image fringes can be observed. How‐ever, in general, only one or two out of the four predicted satellites are registered, the intensity of the other ones being too small. Analysis is made of the fine structure and excellent agreement between theory and experiment is found. Identification of the satellites, based among others on intensity considerations is possible and illustrated on an example. Moreover, the orientation parameters such as s, Δs, and the extinction distance can be estimated from the geometry and a method is outlined allowing to calculate the absorption length from the measured intensities of the satellites.
UR - http://www.scopus.com/inward/record.url?scp=0014768829&partnerID=8YFLogxK
U2 - 10.1002/pssb.19700380224
DO - 10.1002/pssb.19700380224
M3 - Article
AN - SCOPUS:0014768829
SN - 0370-1972
VL - 38
SP - 747
EP - 756
JO - Physica Status Solidi (B)
JF - Physica Status Solidi (B)
IS - 2
ER -