74 J. FRANĚK ET AL.weak lower <strong>and</strong> ⁄ or subducted HP crust is mechanicallydecoupled from middle-crustal units until thelater stages <strong>of</strong> its ascent. This is potentially indicatedby the discordance <strong>of</strong> early structures in the granuliteswith respect to the Monotonous <strong>and</strong> Varied Grouprocks. In these <strong>numerical</strong> models, rapid emplacement<strong>of</strong> these weak, hot rocks as <strong>structural</strong> domes in themiddle crust drives lateral flow, leading to extension<strong>and</strong> ductile thinning above <strong>and</strong> adjacent to the dome.With these calculations in mind, the fan-like geometry<strong>of</strong> the S3 fabrics could have been due to the ductilethinning. Exhumation <strong>of</strong> the Moldanubian rocksfrom below the Tepla´-Barr<strong>and</strong>ian Unit was suggestedby earlier authors (e.g. Scheuvens & Zulauf, 2000;Do¨ rr & Zulauf, 2008), but without the support <strong>of</strong><strong>structural</strong> or seismic data covering the broaderMoldanubian domain.CONCLUSIONSThe <strong>structural</strong> evolution <strong>of</strong> the South Bohemiangranulites reveals a complexity not seen in the easternpart <strong>of</strong> the Moldanubian domain. The SouthBohemian granulites were exhumed along two distinctfabrics, the S2 <strong>and</strong> S3, instead <strong>of</strong> in a single verticalchannel known from the eastern Moldanubian(Schulmann et al., 2005, 2008). The S2 indicates adistinct older tectonic episode possibly related to anearly subduction period <strong>and</strong> emplacement <strong>of</strong> orogeniclower crust at the bottom <strong>of</strong> the orogenic root (Franeˇket al., 2011). The gravimetry <strong>and</strong> <strong>structural</strong> geologyindicate that the individual South Bohemian granulitemassifs reach several kilometres depth. A reflectionseismic pr<strong>of</strong>ile additionally depicts a region <strong>of</strong> probablesteep fabrics through the crust below granulites.This vertical region <strong>of</strong> low reflectivity represents thetrace <strong>of</strong> the deformed granulite D3 crustal-scale ascentchannel that probably consists <strong>of</strong> additional deepergranulite bodies.Partially molten lower crust dominated by felsicgranulites was incorporated into middle crustal levelsin the form <strong>of</strong> a D3 syn-compressional crustal-scaledome at 342–337 Ma. After emplacement, the dome<strong>of</strong> felsic granulite deformed together with the surroundingmiddle crust. The subhorizontal S4 fabricimmediately reworked the S3 during the interval342–337 Ma, being induced by gravitational spreading<strong>of</strong> the growing dome. During D4, the Tepla´-Barr<strong>and</strong>ianupper crust slid to the NW away from the domeregion <strong>and</strong> allowed ductile thinning <strong>of</strong> the mid-crustallevel in the Moldanubian domain.This two-stage exhumation mechanism from HPconditions through the orogenic crust for felsic granulitesmay be applicable to exhumation <strong>of</strong> other HPfelsic rocks. The initial low viscosity probably enabledthe buoyancy-driven rise, while cooling <strong>and</strong> continuedshearing resulted in development <strong>of</strong> a large-scaleme´lange <strong>of</strong> granulite bodies dismembered withinmid-crustal rocks.The presence <strong>of</strong> low-density felsic granulites at thebottom <strong>of</strong> the crustal root is a key factor controllingexhumation <strong>of</strong> the orogenic lower crust <strong>and</strong> the tectonicstyle, both driven by buoyancy in addition totectonic far-field forces. The Bohemian Massif representsa field laboratory for many conceptual models toexplain the exhumation <strong>of</strong> orogenic lower crust ingeneral.ACKNOWLEDGEMENTSThe work was supported by a grant from the CzechScience Foundation (GACˇR 205 ⁄ 05 ⁄ 2187) <strong>and</strong> aninternal project <strong>of</strong> the Czech Geological Survey(326700). Visits by J. Franeˇk to ULP Strasbourg werefunded by the French Government Foundation(BGF). K. Schulmann <strong>and</strong> O. Lexa acknowledgefinancial support from the French National GrantAgency (no. 06-1148784) <strong>and</strong> from the Ministry <strong>of</strong>Education <strong>of</strong> the Czech Republic (grant MSM-0021620855). Pr<strong>of</strong>. G. Manatschal is acknowledged forinspiring discussions. We are grateful for the constructive<strong>and</strong> inspiring reviews <strong>of</strong> R. Jamieson <strong>and</strong>M. Pierce, <strong>and</strong> we thank M. Brown for careful editorialwork.REFERENCESAftalion, M., Bowes, D.R. & Vrána, S., 1989. Early carboniferousU-Pb Zircon age for Garnetiferous, Perpotassic Granulites,Blanský Les Massif, Czechoslovakia. Neues JahrbuchFur Mineralogie-Monatshefte, 4, 145–152.Beaumont, C., Jamieson, R.A., Nguyen, M.H. & Medvedev, S.,2004. Crustal channel flows: 1. 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ORIGIN OF FELSIC MIGMATITES 35(a)Ty
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ORIGIN OF FELSIC MIGMATITES 37(a)Pl
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ORIGIN OF FELSIC MIGMATITES 39Grain
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ORIGIN OF FELSIC MIGMATITES 41(a)(b
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ORIGIN OF FELSIC MIGMATITES 43(a)(b
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ORIGIN OF FELSIC MIGMATITES 45Fig.
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ORIGIN OF FELSIC MIGMATITES 47produ
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ORIGIN OF FELSIC MIGMATITES 49stron
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ORIGIN OF FELSIC MIGMATITES 51Cmı
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ORIGIN OF FELSIC MIGMATITES 53easte
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104 J. FRANĚK ET AL.in terms of th
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106 J. FRANĚK ET AL.Fig. 2. Struct
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108 J. FRANĚK ET AL.(a)perthite po
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110 J. FRANĚK ET AL.(a)(b)(c) (d)
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112 J. FRANĚK ET AL.Table 1. Repre
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114 J. FRANĚK ET AL.at these P-T c
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116 J. FRANĚK ET AL.(a)(b)Fig. 10.
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118 J. FRANĚK ET AL.(a)(b)Fig. 11.
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120 J. FRANĚK ET AL.Table 2. Quant
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122 J. FRANĚK ET AL.(a)(b)Fig. 15.
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124 J. FRANĚK ET AL.Fig. 16. Inter
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126 J. FRANĚK ET AL.development of
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128 J. FRANĚK ET AL.Behrmann, J.H.
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130 J. FRANĚK ET AL.Southern Bohem