HR: 09:30h
AN: V51H-07 [Abstracts]
TI: Monitoring Changing Eruption Styles of Kilauea Volcano Over the Summer of 2007 With Spaceborne Infrared Data
AU: * Ramsey, M
EM: mramsey@pitt.edu
AF: University of Pittsburgh, Department of Geology and Planetary Science, Pittsburgh, PA
15260, United States
AU: Wessels, R
EM: rwessels@usgs.gov
AF: Alaska Volcano Observatory, U.S. Geological Survey Alaska Science Center, Anchorage, AK
99508, United States
AB:
On June 19, 2007 episode 56 (the Father's Day intrusion) of the ongoing eruption at Kilauea Volcano culminated
with a small eruption of lava from a 250 m long fissure approximately 6 km west of Pu'u 'O'o. The event was
preceded by an earthquake swarm and attributed to the intrusion of magma. This intrusion was also associated
with cessation of activity at Pu'u 'O'o and deflation of its summit region. On July 21, 2007 new lava then erupted
along a set of fissures that extended eastward from Pu'u 'O'o toward the old Kupaianaha vent. By early
September, this eruption continued to supply a lava channel approximately 1 km long, which has fed two 'a'a flow
lobes advancing to the northeast and southeast. We describe the application of spaceborne imaging data from
the visible to the thermal infrared (TIR) wavelengths for monitoring activity throughout this period. Satellite thermal
infrared (TIR) data with low spatial resolution (i.e., kms/pixel) have been used for years to monitor changes in
surface thermal features such as volcanic flows. However, the use of higher spatial resolution data allows for the
extraction of physical parameters at meter to sub-meter scales. The Advanced Spaceborne Thermal Emission
and Reflection Radiometer (ASTER) provides TIR, shortwave infrared (SWIR), and visible-near infrared (VNIR)
data ideal for this type of analysis, hazard assessment, and smaller-scale monitoring of active lava flows. From
June-August of 2007, ASTER was scheduled 23 times and collected 11 independent scenes of the new flow
activity at Kilauea. Of these, 7 were clear to partly-cloudy and show excellent coverage of the activity following the
Father's Day intrusion. TIR and SWIR data, converted to atmospherically corrected emitted
surface radiance, have been used to extract flow extent, areal coverage, flow advance rate, and maximum
brightness temperature. These data correlate well with descriptions of the flow activity documented by Hawaiian
Volcano Observatory field crews. For example, the ASTER night time image collected on July 19 (22:42:56 HST)
had a maximum SWIR-derived temperature of 305 C, and a total thermally-elevated area of 0.19 sq. km. Within
that region, 3 distinctly hotter zones were identified as most likely the West Gap pit craters, which were described
as intermittently overflowing to form a small lava lake at the time. Following the July 21 fissure eruption, ASTER
observations were augmented with non-standard approaches such as collecting visible night time data in order
to accurately extract the higher temperature of the open lava channel. Although clouds partially obscure the
August 30 night image, a maximum pixel-integrated temperature of 750 C was detected using the VNIR night-
time data for the first time. Such a monitoring program coordinated between NASA and a USGS volcano
observatory can provide important data on hot spot detection, eruption rate, and flow advance at times where it
may be too costly or risky to send scientists into the field.
DE: 8414 Eruption mechanisms and flow emplacement
DE: 8419 Volcano monitoring (7280)
DE: 8425 Effusive volcanism
DE: 8429 Lava rheology and morphology
DE: 8485 Remote sensing of volcanoes
SC: Volcanology, Geochemistry, Petrology [V]
MN: 2007 Fall Meeting