Roles of gas and heat in a mushy magma chamber

The processes that occur in magmatic reservoirs and their surrounding
crustal rocks can modulate the triggering, duration, and style of volcanic
eruptions. Although magmatic reservoirs are typically modeled as cavities
filled with fluid magma, geophysical and petrological observations have
long suggested that they likely contain crystal mush, an ensemble of solid
crystals and fluid (gas/melt) that reside in interstitial pore spaces. The
mushy-and-gassy magma chamber extends previous studies by Liao et al
(2018, 2021) to incorporate two new aspects that are typical for crustal
magmatic systems: gas phase (in the form of disconnected gas bubbles) and
nonuniform temperature. This dataset incorporates the parameters and
numerical codes used for generating results in the submitted manuscript
'Roles of Gas and Heat in a Mushy Magma Chamber. The dataset consists
of a README file detailing the data structure, a matlab .mat file that
contains the parameters assumed in the magma chamber model, and several
matlab program .m files that can be applied to the .mat file to generate
results presented in the manuscript.