The Australasian Institute of Mining and Metallurgy (The AusIMM) has been one of the principal organisations behind the JORC Code, which has been adopted by the Australian Stock Exchange and the Australian Securities commission as the standard for reporting mineral resources and ore reserves. This is now starting to be recognised as the international standard, with the UK, the USA and Canada all examining some form of the JORC Code for their resource and reserve reporting guidelines. The AusIMM has now further taken the initiative to produce a major volume covering all aspects of world’s best practice in Mineral Resource and Ore Reserves estimation. This prestigious volume will be published in the year 2000. <...>

We have been describing and attempting to interpret trace fossils, more or less effectively, for over a century. One could point to several times in the history of paleontology or sedimentary geology when ichnology, as a separate discipline, appears to take shape for the first time. This is largely a matter of when the various early practitioners were active. I will leave it to the historians of our discipline to nail down all the exact dates, key figures and origins of ideas. A concise historical sketch can be found in the introduction to Ekdale et al. (1984). It is clear from this brief account, and from the longer essay by Osgood (1975) and especially the excellent historical chapters that follow, that the origins of ichnology are varied but that the discipline takes on its modern methodologic and conceptual aspects in the 1950s and 1960s. In anglophone countries, this development is usually associated with a ‘founder’ (Dolf Seilacher, signaled especially by a series of extremely influential articles: e.g., 1953, 1962, 1964, 1967a,b) and a ‘founding document’ (Ha¨ntzschel, 1962, 1975)—at least for invertebrate ichnology. Vertebrate and plant trace fossil researchers would tell the story a bit differently (see the essays that follow). But most of the central concepts and methods start to circulate and become widely applied or discussed at about this time.

Of the many techniques that have been applied to the study of crystal defects, probably no single technique has contributed more to our understanding of their nature, properties, and influence on the physical and chemical properties of crystalline materials than transmission electron microscopy (ТЕМ). Although the importance of crystal defects and the use of ТЕМ for their direct observation were recognized by physical metallurgists in the early 1950s, it was at least a decade later that earth scientists responded to many of the new ideas of the defect solid state and to the power of ТЕМ. However, ТЕМ is now used extensively for the direct observation of defect microstructures in minerals and rocks, and there appears to be an increasing number of earth scientists who want to use the technique or to become more familiar with the interpretation of ТЕМ observations. This book is written for such people. However, it makes no attempt to be a practical manual of ТЕМ or a definitive text, but rather an introduction to the basic principles of the technique and of the interpretation of electron micrographs and electron diffraction patterns. As such, I hope the book will also be useful to students of materials science.

The physical-chemical properties of kimberlite melt govern the transport and eruption behaviour of kimberlite magmas. However, the physical properties of kimberlitic melts remain unknown, in part, because the composition of the melt phase is poorly constrained (Price et al. 2000; Kopylova et al. 2006; Sparks et al. 2006). As well, the experimental techniques needed to probe these extreme melts for viscosity (!), glass transition temperatures (Tg), heat capacity (Cp), and volatile solubilities are not yet available. Furthermore, the physical properties of kimberlite melts need not be simple linear extrapolations from the properties of other silicate melts (Russell & Giordano 2005). Computational models, calibrated on high quality experimental data, provide a means of exploring the physical properties of silicate melts for which there are no data.

In this presentation we use the current estimates for the range of kimberlite melt compositions (Table 1 & 2; after Price et al. 2000; Sparks et al. 2006; Kopylova et al. 2006). Secondly, we introduce and apply two multicomponent chemical models for predicting specific physical properties of melts in general. These models are designed to predict the calorimetric glass transition temperature and the viscosity of silicate melts as a function of melt composition and are used to explore the corresponding properties of kimberlite melts.