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116

J

anuary

2012

www.read-tpt.com

A

rticle

Improving standard methods of grain

size determination in high-alloy steel

and alloy products

D.Yu. Klyuev, Ye.Ya. Lezinskaya, V.V. Perchanik (National Metallurgical Academy of Ukraine)

N.A. Koryaka (ITA Representative in CIS, Ukraine)

Austenite or ferrite grain size is the major parameter of steel and

alloy single-phase structure. Determination of this parameter is

complicated by two reasons:

Opacity of the subject being measured

Imperfection of the methods used for grain size determination

Many methods for determination of metal grain structure parameters

appeared in the 20

th

century. They have made it possible to lay

down basic principles of a new trend in metal science: stereological

metallography. Stereometric Metallography by S.A. Saltykov,

Stereology in Physical Metallurgy by K.S. Cherniavsky, Quantitative

Microscopy by De Goff and Rines and Quantitative Stereology by

Underwood are fundamental works generalising the experience

gained in this direction during the last century.

Nearly a century-old history of existence of standard methods of

determination of grain size in steels and alloys underwent several

stages of its development. At first, methods of austenite and ferrite

grain identification were developed. American Society for Testing

and Materials (ASTM) pioneered creation of such standards.

In the early 1930s, ASTM Committee E4 developed a number of

standards including various methods of grain size determination

which formed the basis for analogous standards adopted in many

industrially developed countries, eg SIS 11 11 01 (Sweden), UNI

3245 (Italia), GOST 5639 (Russia), NF A04-102 (France), and SEP

1510 (Germany) which was transformed later into DIN 50601 and

ISO 643.

Methods in the above standards determine average dimensions

(diameter, area) or the number of the grains visible in a microsections

plane.

These methods are based on the development of reference

photographs with which structures seen in the microsections plane

are compared and the grain size is determined by the number of the

grains seen in one square inch at magnification ×100.

Grain size numbers have appeared much more later on, in standard

E112.

It is significant that evaluation by numbers was called forth by the

needs of metal product producers who had to control grain size in

their finished products. Introduction of conventional units (numbers)

has made much easier the grain size control operations but it

significantly worsened accuracy as compared with the quantitative

methods.

Nevertheless, all present-day standard methods of determination of

grain size in metals and alloys use exactly these conventional units.

All methods come to either visual comparison with photographic

references and expression in conventional units (numbers)

amounting from 18 (in GOST 5639) to 30 (in ASTM Е 112), or

counting the number of grains in a unit of length (chord method),

area or volume.

Chord method is of a lowest accuracy because of imperfect means

of determination of spatial dimensions and shapes of individual

crystallites in opaque materials of metal products. It does not ensure

a realistic view of such important parameters of a spatial structure

as grain anisotropy, shape, etc.

The existing methods developed for the reconstruction of spatial

structures by its flat layout in a metallographic section are rather

laborious and, again, coming to the determination of average

dimensions which does not allow establishment of the cause

of material property irregularities undoubtedly connected with

structural irregularities, ie grain anisotropy.

High-alloy steels and alloys used in high-duty structures (power

equipment, electronics, chemical equipment, space technology,

etc) are the materials the most prone to grain anisotropy. It should

be pointed out that the present-day methods of manufacture of

products form such materials, eg tubes for fuel element cans, allow

formation of a rather homogeneous structure in these products

[1-3]

.

At the same time, the available standard methods for evaluation of

such structures are rather imperfect. What concerns methods for

evaluation of grain anisotropy, they are practically absent.

Domain of above standards, except GOST 5639, spreads just to the

structures in which grain size distribution approaches the normal

one. And at the same time, if the image in the microsections plane is

closest to those in photographic references given in the standards,

the most trustworthy assessment results can be obtained. The

higher grain anisotropy of the structure, the higher is the error of its

assessment.