Kilauea Infrasound: MENE Array
DISCLAIMER: The data products displayed in this section are in active development and have not been sufficiently tested for reliable use in operational eruption monitoring.
The following historical plots are generated every hour for the MENE array (map).
Last updated at:
05/09/08-16:05:10 HST (UTC-10hrs)Please click on the image to see the full-size version of the graph.
Image is 21 Minutes, 42 Seconds old.
Fig. 1: Top) Spectrogram for the last 24 hours from station MENE, located ~13 km northwest of Pu`u `O`o crater and ~7 km from Halema`uma`u. Bottom) PMCC detections from station MENE for the last 24 hours. The arrival azimuth of each coherent detection family is on the y-axis, the number of detections in the family scales the marker size, and the color denotes the weighted mean frequency of the family. Pu`u `O`o lies at ~112° from the array while the Halema`uma`u Gas Vent (HGV) is at ~250°.
Image is 21 Minutes, 42 Seconds old.
Fig. 2. PMCC detections from station MENE for the last 24 hours. Arrival azimuths for Pu`u `O`o crater and the 7/21 fissure eruption are highlighted.
Image is 21 Minutes, 42 Seconds old.
Fig. 3. Log polar plot of 0.5-10 Hz PMCC detections for the MENE array for the last 4 hours. The Pu`u `O`o and Kilauea craters are marked in red, while Fissure D is in yellow.
Image is 21 Minutes, 42 Seconds old.
Fig. 4. Power spectral density for the last hour from station MENE.
Image is 21 Minutes, 42 Seconds old.
Fig. 5: Peak power and frequency of the HGV spectral peak. Top) Maximum power of the peak frequency between 0.3-0.8 Hz. Bottom) Peak frequency of the spectral peak between 0.3-0.8 Hz. Both values are taken every hour from the beamformed power spectral density.
Image is 11 Minutes, 45 Seconds old.
Fig. 6. Coherent acoustic power per hour in the 0.3-1.0 Hz band originating from the direction of the Halema`uma`u Crater Gas Vent (HGV). Top) Power values for the past 24 hours. Bottom) Hourly power values since 3/19. The small subplots indicate the very low frequency energy, and is a proxy for the wind speed. Power values are in watts, or joules/hour.
Image is 11 Minutes, 45 Seconds old.
Fig. 7: Acoustic energy calculation for the last hour for the HGV. Infrasound array data is high-pass filtered between 0.3-1.0 Hz and split into 60 sec windows. The top panel shows the correlation value from PMCC between 0.3-1.0 Hz for azimuths within +/-7 degs from HGV. If the correlation value is above 0.5, the data segment is considered coherent. The middle panel shows the filtered waveform. If the section is red, the signal correlation value is too low or its azimuth is off the target beam. If it is black, it is coherent and arriving from the HGV azimuth, and the incident acoustic source energy is estimated.. The bottom panel shows the calculated acoustic source energy for the time window. The sum of the bottom panel values is shown in Fig. 5.