BUBBLE-SIZE DISTRIBUTION IN MAGMA CHAMBERS AND DYNAMICS OF BASALTIC ERUPTIONS

Authors
Citation
S. Vergniolle, BUBBLE-SIZE DISTRIBUTION IN MAGMA CHAMBERS AND DYNAMICS OF BASALTIC ERUPTIONS, Earth and planetary science letters, 140(1-4), 1996, pp. 269-279
Citations number
36
Categorie Soggetti
Geochemitry & Geophysics
ISSN journal
0012821X
Volume
140
Issue
1-4
Year of publication
1996
Pages
269 - 279
Database
ISI
SICI code
0012-821X(1996)140:1-4<269:BDIMCA>2.0.ZU;2-G
Abstract
In the shallow magma chambers of volcanoes, the CO2 content of most ba saltic melts is above the solubility limit. This implies that the cham ber contains gas bubbles, which rise through the magma and expand. Thu s, the volume of the chamber, its gas volume fraction and the gas flux into the conduit change with time in a systematic manner as a functio n of the size and number of gas bubbles. Changes in gas flux and gas v olume are calculated for a bubble size distribution and related to cha nges in eruption regimes. Fire fountain activity, only present during the first quarter of the eruption, requires that the bubbles are large r than a certain size, which depends on the gas flux and on the bubble content [1]. As the chamber degasses, it loses its largest gas bubble s and the gas flux decreases, eventually suppressing the fire fountain ing activity. Ultimately, an eruption stops when the chamber contains only a few tiny bubbles. More generally, the evolution of basaltic eru ptions is governed by a dimensionless number, tau = tau g Delta rho a (o)(2)/(18 mu h(c)), where tau = a characteristic time for degassing; a(o) = the initial bubble diameter; mu = the magma viscosity; and h(c) = the thickness of the degassing layer. Two eruptions of the Kilauea volcano, Mauna Ulu (1969-1971) and Puu O'o (1983-present), provide dat a on erupted gas volume and the inflation rate of the edifice, which h elp constrain the spatial distribution of bubbles in the magma chamber : bubbles come mainly from the bottom of the reservoir, either by in s itu nucleation long before the eruption or within a vesiculated liquid . Although the gas flux at the roof of the chamber takes similar value s for both eruptions, the duration of both the fire fountaining activi ty and the entire eruption was 6 times shorter at Mauna Ulu than durin g the Puu O'o eruption. The dimensionless analysis explains the differ ence by a degassing layer 6 times thinner in the former than the latte r, due to a 2 year delay in starting the Mauna Ulu eruption compared t o the Puu O'o eruption.