V34B:
Origin and Timescales of Magmatic Systems: Discussing Ages, Rates, Transport, and Storage Processes of Magmas from the Source to Emplacement or Eruption II


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Session ID#: 59372

Session Description:
Magmatic systems involve a range of dynamic processes governing magma generation, ascent, emplacement, and eruption. The timescales of these processes are of paramount importance to understand the evolution of magmatic reservoirs and mush zones during crystallization, assimilation, mixing, and volatile exsolution. Depending on the ascent timescales, these processes may operate far from compositional and textural equilibrium, induced by rapidly changing environmental parameters (e.g. P,T,fO2). Rates and mechanisms of crustal emplacement or eruption, together with physical, petrological and rheological investigations of magmas, are also crucial in characterizing volcanic hazard. We welcome analytical, numerical, experimental, geophysical, and field-based studies addressing rates and timescales of magmatic processes, within the Earth and other planetary bodies. These may include radiogenic isotope dating, mineral geospeedometry, crystal size distribution, and fluid dynamics. Also, we welcome interdisciplinary studies probing the mechanisms and timescales of volcanic phenomena like pre-eruptive dynamics, magma and lava rheology, phase equilibria, and volcanic flows.
Primary Convener:  Maurizio Petrelli, University of Perugia, Department of Physics and Geology, Perugia, Italy
Conveners:  Stephan Kolzenburg, Ludwig Maximilians University of Munich, Department of Earth and Environmental Sciences, Munich, Germany and Kendra J Janell Lynn, University of Delaware, Earth Sciences, Newark, DE, United States
Primary Liaison:  Kendra J Janell Lynn, University of Delaware, Earth Sciences, Newark, DE, United States
Chairs:  Stephan Kolzenburg, Ludwig Maximilians University of Munich, Department of Earth and Environmental Sciences, Munich, Germany and Kendra J Janell Lynn, University of Delaware, Earth Sciences, Newark, DE, United States
OSPA Liaison:  Kendra J Janell Lynn, University of Delaware, Earth Sciences, Newark, DE, United States
Co-Organized with:
Volcanology, Geochemistry and Petrology, and Natural Hazards

Cross-Listed:
  • DI - Study of the Earth's Deep Interior
  • MR - Mineral and Rock Physics
  • NH - Natural Hazards
  • P - Planetary Sciences

Proposed Co-Organized Session with:
  • MR - Mineral and Rock Physics
  • NH - Natural Hazards
Index Terms:

1160 Planetary and lunar geochronology [GEOCHRONOLOGY]
3618 Magma chamber processes [MINERALOGY AND PETROLOGY]
3640 Igneous petrology [MINERALOGY AND PETROLOGY]
8439 Physics and chemistry of magma bodies [VOLCANOLOGY]

Abstracts Submitted to this Session:

Meredith Townsend, Brown University, Earth, Environmental and Planetary Sciences, Providence, RI, United States, Wim Degruyter, Cardiff University, School of Earth and Ocean Sciences, Cardiff, United Kingdom and Christian Huber, Brown University, Department of Earth, Environmental and Planetary Sciences, Providence, RI, United States
Corliss Kin I Sio, Lawrence Livermore National Laboratory, Livermore, CA, United States and James Daniel Paul Moore, Earth Observatory of Singapore, Singapore, Singapore
Sumit Chakraborty, Ruhr University Bochum, Institute GMG, Bochum, Germany
Michael Jollands1, Elias Kempf2, Jörg Hermann2 and Othmar Müntener1, (1)University of Lausanne, Institute of Earth Sciences, Lausanne, Switzerland, (2)University of Bern, Institute of Geological Sciences, Bern, Switzerland
Anna Barth, Lamont-Doherty Earth Observatory of Columbia University, Palisades, NY, United States and Terry A Plank, Lamont-Doherty Earth Observatory, Palisades, NY, United States
Dr. W Henry Henry Towbin, PhD, Brooklyn, NY, United States, Terry A Plank, Lamont-Doherty Earth Observatory, Palisades, NY, United States, Erik Hauri, Carnegie Institution for Science, Washington, DC, United States, Simon C Kohn, University of Bristol, School of Earth Sciences, Bristol, United Kingdom and Richard A. Brooker, University of Bristol, Bristol, United Kingdom
Anne H Peslier1, Richard L Hervig2, Shuying Yang3, Munir Humayun3, Barnes Jessica4, Anthony J Irving5 and Alan D Brandon6, (1)NASA Johnson Space Center, ARES, Houston, TX, United States, (2)Arizona State University, School of Earth and Space Exploration, Tempe, United States, (3)Florida State University, Dept. of EOAS & National High Magnetic Field Laboratory, Tallahassee, FL, United States, (4)NASA, Houston, TX, United States, (5)University of Washington, Earth & Space Sciences, Seattle, WA, United States, (6)New Mexico State University Main Campus, Las Cruces, United States