MULTISPECTRAL THERMAL INFRARED MAPPING OF THE 1 OCTOBER 1988 KUPAIANAHA FLOW FIELD, KILAUEA VOLCANO, HAWAII

被引:43
作者
REALMUTO, VJ
HON, K
KAHLE, AB
ABBOTT, EA
PIERI, DC
机构
[1] MS 183-501, Jet Propulsion Laboratory, California Institue of Technology, Pasadena, 91109, CA
[2] United States Geological Survey Hawaiian Volcano Observatory, 96718, HI, Hawaii National Park
关键词
D O I
10.1007/BF00301118
中图分类号
P [天文学、地球科学];
学科分类号
07 ;
摘要
Multispectral thermal infrared radiance measurements of the Kupaianaha flow field were acquired with the NASA airborne Thermal Infrared Multispectral Scanner (TIMS) on the morning of 1 October 1988. The TIMS data were used to map both the temperature and emissivity of the surface of the flow field. The temperature map depicted the underground storage and transport of lava. The presence of molten lava in a tube or tumulus resulted in surface temperatures that were at least 10-degrees-C above ambient. The temperature map also clearly defined the boundaries of hydrothermal plumes which resulted from the entry of lava into the ocean. The emissivity map revealed the boundaries between individual flow units within the Kupaianaha field. In general, the emissivity of the flows varied systematically with age but the relationship between age and emissivity was not unique. Distinct spectral anomalies, indicative of silica-rich surface materials, were mapped near fumaroles and ocean entry sites. This apparent enrichment in silica may have resulted from an acid-induced leaching of cations from the surfaces of glassy flows. Such incipient alteration may have been the cause for virtually all of the emissivity variations observed on the flow field, the spectral anomalies representing areas where the acid attack was most intense.
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页码:33 / 44
页数:12
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