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IFM-GEOMAR, Leibniz-Institute for Marine Sciences, Dynamics of the Ocean Floor, D-24148 Kiel, Germany, thansteen@ifm-geomar.de
Fachbereich Geowissenschaften, Universität Bremen, D-28334 Bremen, Germany, akluegel@uni-bremen.de
| The first 20% of the full text of this article appears below. |
| INTRODUCTION |
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Fluid inclusions can provide thermobarometric data on various timescales. During ascent of mafic to intermediate magmas, fluid inclusions may form within hours to days and record transient magma stagnation levels, whereas chemical mineral-melt thermobarometry requires equilibrium mineral growth and thus typically reflects well-defined crystallization events (Roedder and Bodnar 1980; Wanamaker et al. 1990; Hansteen et al. 1998; Klügel et al. 2000; Frezzotti and Peccerillo 2004). Such data has only rarely been combined with melt inclusion investigations in order to depict detailed magma ascent histories (e.g., Bureau et al. 1998). During prolonged crystallization in magma chambers or in the plutonic environment, however, fluid inclusions reflect the equilibrium situation, and data from various thermobarometric methods should overlap.
This chapter focuses on the use of fluid inclusions as thermobarometers to constrain magmatic processes and timescales. After an introduction of basic principles and explanation of the most relevant fluid systems we show in a "cookbook" style how barometric data are derived, and discuss error magnitudes and pitfalls. Thermobarometric information attained from chemical mineral-melt equilibria are compared to that obtained from fluid inclusions in order to provide detailed accounts for magma ascent and crystallization. Although the term "fluid inclusion" is often used in a general way comprising all
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