A simple explanation for the space-based calculation of lava eruption rates
- 15 October 2001
- journal article
- Published by Elsevier BV in Earth and Planetary Science Letters
- Vol. 192 (2), 223-233
- https://doi.org/10.1016/s0012-821x(01)00443-5
Abstract
No abstract availableKeywords
This publication has 22 references indexed in Scilit:
- Effusion rate trends at Etna and Krafla and their implications for eruptive mechanismsJournal of Volcanology and Geothermal Research, 2000
- Low-cost volcano surveillance from space: case studies from Etna, Krafla, Cerro Negro, Fogo, Lascar and ErebusBulletin of Volcanology, 1997
- A chronology of the 1991 to 1993 Mount Etna eruption using advanced very high resolution radiometer data: Implications for real‐time thermal volcano monitoringJournal of Geophysical Research, 1997
- Factors controlling the lengths of channel-fed lava flowsBulletin of Volcanology, 1994
- Emplacement of the 75-km-long Carrizozo lava flow field, south-central New MexicoJournal of Volcanology and Geothermal Research, 1993
- Lava flows are fractalsGeophysical Research Letters, 1992
- Eruption rate, area, and length relationships for some Hawaiian lava flowsJournal of Volcanology and Geothermal Research, 1986
- Lengths of Hawaiian lava flowsGeology, 1980
- Effusion rate and the shape of aa lava flow-fields on Mount EtnaGeology, 1978
- Mount Etna and the 1971 eruption - Lengths of lava flowsPhilosophical Transactions of the Royal Society of London. Series A, Mathematical and Physical Sciences, 1973