Aloha!
AGU fall meeting is next week! Are you ready!? We are excited to be able to share some of the work we have been doing at the lab this year. The following is a guide to not only what we will be presenting, but other interesting talks and sessions for those interested in infrasound.
Our Infrasound Team Talks, Posters, and Sessions:
Tuesday
8:00 AM - 10:00 AM 2022 Moscone West - NH21D. The Chelyabinsk Meteor Event I
1:40 PM - 6:00 PM Poster NH23D-1554 - Infrasonic Tracking of the Chelyabinsk Meteor in NH23D. The Chelyabinsk Meteor Event II Posters
4:30 PM - 4:45 PM 307 (Moscone South) - Assessing Infrasound Network Performance Using the Ambient Ocean Noise in S24B. Advances in Nuclear Test Monitoring From Multiple Technologies III
Friday
12:05 PM - 12:20 PM 308 (Moscone South) - Regional Localization with the Hawaii Island Infrasound Network in V52C. Assessing Volcanic Processes Through Novel Monitoring Approaches II (cosponsored by EGU-GMPV)
All Sessions of Interest:
Monday
4:00 PM - 6:00 PM 305 Moscone South - S14A. Infrasound and Seismoacoustics I
Tuesday
8:00 AM - 10:00 AM 2022 Moscone West - NH21D. The Chelyabinsk Meteor Event I
1:40 PM - 6:00 PM Poster - A23F Weather, Dynamics and Climate Posters
1:40 PM - 6:00 PM Poster - NH23D The Chelyabinsk Meteor Event II Posters
1:40 PM - 6:00 PM Poster - S23B Infrasound and Seismoacoustics II Posters
4:00 PM - 6:00 PM 307 Moscone South - S24B Advances in Nuclear Test Monitoring From Multiple Technologies III [SWIRL_CU]
Wednesday
1:40 PM - 6:00 PM Poster - S33B Characterization and Modeling for Nuclear Test Monitoring and Verification II Posters
Thursday
8:00 AM - 12:20 PM Poster - V41B Magma Plumbing, Transport and Eruption at Basaltic Volcanoes III Posters (cosponsored by EGU-GMPV and MSA)
1:40 PM - 6:00 PM Poster - NG43A Pattern Formation and Nonlinear and Scaling Geoprocesses: From Microscale to the Climate II Posters [SWIRL_CM.CU]
Friday
10:20 AM - 12:20 PM 308 Moscone South - V52C Assessing Volcanic Processes Through Novel Monitoring Approaches II (cosponsored by EGU-GMPV)
1:40 PM - 3:40 PM 104 Moscone South - U53A Comprehensive Test Ban Treaty Organization
Now you know where we will be hanging out! Don't forget you can always follow along with the fun on twitter with hasgtags #AGU13 #infrasound and just in case you are not already... you can follow our team members at @isoundhunter and @isoundhuntress
Friday, December 6, 2013
Thursday, November 7, 2013
Super Typhoon Haiyan
Aloha! It has sure been busy at the lab this year, but something like Haiyan doesn't happen every day, so here I am! I have just a quick post today with a few figures and a new track. Enjoy!
The CTBTO IMS station I39PW is located on the island of Babeldaob in Palau. Super Typhoon Haiyan ran over the northern most state of Palau, Kayangel island on 06 November 2013 UTC. The infrasound station I39PW recorded the approach, and part of the typhoon before losing power late in the day UTC.
I recommend also listening to the infrasound data sped up ~ 2000x so it is in the audio range while viewing the figures. The following track is around 10 hrs of data covering the ramp up of the storm as well as the storm passing over, up until the station lost power.
Super Typhoon Haiyan was a category 5 when it slammed into Palau. According to an article on gizmodo the storm has broken the intensity scale by 0.1 when it registered 8.1 out of 8. It is beautiful and dangerous. The lab's thoughts are with the people of the Philippines.
The CTBTO IMS station I39PW is located on the island of Babeldaob in Palau. Super Typhoon Haiyan ran over the northern most state of Palau, Kayangel island on 06 November 2013 UTC. The infrasound station I39PW recorded the approach, and part of the typhoon before losing power late in the day UTC.
Spectrogram and array processing results from I39PW created by ISLA.
I recommend also listening to the infrasound data sped up ~ 2000x so it is in the audio range while viewing the figures. The following track is around 10 hrs of data covering the ramp up of the storm as well as the storm passing over, up until the station lost power.
Super Typhoon Haiyan was a category 5 when it slammed into Palau. According to an article on gizmodo the storm has broken the intensity scale by 0.1 when it registered 8.1 out of 8. It is beautiful and dangerous. The lab's thoughts are with the people of the Philippines.
Aqua/MODIS 11/07/2013 04:25 UTC
You can read more:
Friday, May 31, 2013
Aloha Video Friday: Bass edition
Aloha! I have two videos for you this wonderful Friday!
First I am going to warn you that these videos were created to be listened to on a system with a healthy dose of bass. We recommend a subwoofer. If you have a speaker that can dip down into the infrasound range even better!
First we have a video staring Tungurahua Volcano in Ecuador.
First I am going to warn you that these videos were created to be listened to on a system with a healthy dose of bass. We recommend a subwoofer. If you have a speaker that can dip down into the infrasound range even better!
First we have a video staring Tungurahua Volcano in Ecuador.
The second video stars our very own Kilauea Volcano, specifically the Pu'u O'o vent
We hope you enjoyed the bass drop Plinian and Hawaiian style! Have a good weekend!
Friday, February 15, 2013
Feb 15, 2013 Russian Meteor
Aloha, this post will be updated as more information becomes available and more data are processed.
This morning in Russia a meteor exploded over the skies of Chelyabinsk (55.2N, 61.4E). The event occurred around 03:20 UTC today (Feb 15th). We, as members of the infrasound community are very busy and will be releasing bits and pieces as we go (look under @infrasoundhunter on twitter). This post will mostly contain results from our lab, although we retain the right to post anything we find totally awesome.
The CTBTO twitter account released the following image:
Initial results from station I31KZ located ~600 km from the hypercenter, to the south. (source)
More results from I31KZ. "Behold the infrasonic signature of the Russian Meteor, radiating from 8Hz down to 0.004 Hz - the deep end of sound" - isoundhunter (source)
Initial location released for the meteor, and the stations we have been talking about. Plotted in Google Earth.
"The 4mHz (0.004 Hz) low end for the Russian meteor infrasound corresponds to a 250s atmospheric oscillation, a wavelength of 85km. A BIG. Slow. Sound." - isoundhunter (source)
Russian Meteor in Hawaii!?
The CTBT IMS Infrasound site in Hawaii (I59US) seems to have recorded a signal from this event. The station I59US is located approximately 11,000 km from the source, with a travel time of 11 hours and 40 minutes.
There is an article in the Star Advertisor (unfortunetly it is behind a pay wall) but the figures are posted here
This morning in Russia a meteor exploded over the skies of Chelyabinsk (55.2N, 61.4E). The event occurred around 03:20 UTC today (Feb 15th). We, as members of the infrasound community are very busy and will be releasing bits and pieces as we go (look under @infrasoundhunter on twitter). This post will mostly contain results from our lab, although we retain the right to post anything we find totally awesome.
The CTBTO twitter account released the following image:
Results from the CTBTO IMS Infrasound Network. The event was picked up by 11 infrasound stations. (source)
Initial results from station I31KZ located ~600 km from the hypercenter, to the south. (source)
Initial results from I46RU located ~1,500 km from the hypercenter, to the east. (source)
More results from I31KZ. "Behold the infrasonic signature of the Russian Meteor, radiating from 8Hz down to 0.004 Hz - the deep end of sound" - isoundhunter (source)
Initial location released for the meteor, and the stations we have been talking about. Plotted in Google Earth.
"The 4mHz (0.004 Hz) low end for the Russian meteor infrasound corresponds to a 250s atmospheric oscillation, a wavelength of 85km. A BIG. Slow. Sound." - isoundhunter (source)
Russian Meteor in Hawaii!?
The CTBT IMS Infrasound site in Hawaii (I59US) seems to have recorded a signal from this event. The station I59US is located approximately 11,000 km from the source, with a travel time of 11 hours and 40 minutes.
There is an article in the Star Advertisor (unfortunetly it is behind a pay wall) but the figures are posted here
EDIT: We are still working on this amazing data set! I will be posting results as we finalize them.
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