maschmeyer agu2015 compressedseoe.sc.edu/.../maschmeyer_agu2015_compressed.pdf · 2016. 2. 8. ·...

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Detection of high-silica lava flows and lava morphology at the Alarcon Rise, Gulf of California, Mexico using automated classification of the morphological-compositional relationship in AUV multibeam bathymetry and sonar backscatter Christina A. Maschmeyer ([email protected]) 1 , Scott M. White 1 , Brian M. Dreyer 2 , David A. Clague 3 University of South Carolina, Columbia, SC 1 University of California, Santa Cruz, CA 2 Monterey Bay Aquarium Research Institute, Moss Landing, CA 3 Introduction and Objectives e Alarcon Rise is the southernmost spreading ridge in the Gulf of California, Mexico. e Alarcon Rise is an intermediate-rate spreading center with a full spreading rate of 50 cm/yr. Eruption processes of lava effusion rate (which corresponds to spreading rate), underlying topography, and lava viscosity control the formation of submarine lava morphologies for mid-oceanic ridge basalt (MORB) [Gregg and Fink (1995)]. Typical MORB exists at the Alarcon Rise, but researchers from the Monterey Bay Aquarium Research Institute (MBARI) and Scripps Oceanographic Institute collected volcanic samples with elevated silica content [Castillo et al. (2002)]. Because submarine lava morphology depends on eruption processes, we propose to use morphologic signatures to identify evolved lavas. Our three primary questions for this research are: 1. Can lava composition be determined by lava flow morphology? 2. What morphologic signatures are critical to identification of lavas with elevated silica? 3. How much high-silica lava exists at the Alarcon Rise? We built an artificial intelligence classifier to begin to answer these questions at the Alarcon Rise. Expert Classification - Construction of an adaptive neuro-fuzzy inference system (ANFIS) enabled the classification of lava composition - Inputs were local slope and texture datasets from high-resolution bathymetry and sonar backscatter collected by AUV D. Allen B. in 2012. - Training cycle data included of 134 ground-referenced igneous samples collected by MBARI in 2012 and 2015 plus 48 points on MORB domes generated in ArcGIS along ROV track lines - Testing data consisted of 47 expert-picked MORB dome samples and 200 ground-referenced igneous samples collected in 2012 and 2015 - We applied the classification to two regions along the Alarcon Rise: a high-silica region and a MORB region AUV Bathymetry AUV Bathymetry Sidescan Sonar Backscatter Sidescan Sonar Backscatter GLCM Textures GLCM Textures Local Slope Local Slope GLCM Textures GLCM Textures ANFIS ANFIS Classification Classification Accuracy Assessment Accuracy Assessment Ground Referenced Igneous Rock Samples Ground Referenced Igneous Rock Samples Training Data Training Data Testing Data Testing Data Submarine Lava Morphology Typical oceanic ridge lava exhibits three distinct morphologies: sheet flows, lobate flows and small pillow mounds (~150 m diameter). Lava effusion rate, viscosity, and underlying topography determine the morphologic differences between flows [Gregg and Fink (1995)]. Lava effusion rate is the most influential variable at spreading ridges with compositionally uniform lava [White and Klein (2014)]. Spreading ridges with silica-rich lavas do not exhibit submarine lava flow morphologies. Large pillows with extreme radial jointing and corrugated surfaces and asymmetrical lava blocks build large domes. Angular, blocky talus is also common at silica-rich domes [Wanless et al. (2010)]. e high-silica region of interest includes a large (~500 m diameter) dome. MORB Morphology Sheet Lobate Pillow High-Silica Lava Morphology Radial Jointing Lava Blocks Corrugated Pillow High-Silica Dome Distance (m) 550 500 450 400 350 300 250 200 150 100 50 0 Depth (m) -2,340 -2,360 -2,380 -2,400 -2,420 -2,440 -2,460 MORB Dome Depth (m) 550 500 450 400 350 300 250 200 150 100 50 0 Depth (m) -2,330 -2,340 -2,350 -2,360 -2,370 -2,380 Seafloor Mapping and Sampling - February-April 2012 and 2015, MBARI mapped the Alarcon Rise at 1 m horizontal resolution using the AUV (Autonomous Underwater Vehicle) D. Allen B. We created inputs for the expert classifier from bathymetry and sonar backscatter collected during 2012 - MBARI collected 410 rock samples over 19 dives by the ROV (remotely operated vehicle) Doc Ricketts -364 igneous samples collected along the spreading ridge were used during classification Completed Dives Trackline Coverage Basalt Basaltic Andesite Andesite Dacite Rhyolite Total 9 36.3 km 135 7 6 7 35 190 10 38.6 km 97 14 37 16 10 174 Igneous Rock Samples References - Castillo, P.R., Hawkins, J.W., Lonsdale, P.F., Hilton, D.R., and Shaw, A.M., 2002, Petrology of the Alarcon Rise lavas, Gulf of California: Nascent intracontinental ocean crust: Journal of Geophysical Research, v. 107, no.B10, p. 1-15. - Gregg, P.M., Fink, J.H., 1995, Quantification of submarine lava-flow morphology through analog experiments: Geology, v. 23, n.1, p. 73-76. - Wanless, V.D., Perfit, M.R., Ridley, W.L., and Klein, E., 2010, Dacite petrogenesis on mid-ocean ridges: Evidence for oceanic crustal melting and assimilitaion: Journal of Petrology, v. 51, n. 12, p. 2377-2410. -White, W.M., and Klein, E.M., 2014, Composition of the Oceanic Crust, in Saunders, J.A.,Hofstra, A.H., Goldfarb, R.J., and Reed, M.H., eds., Treatise on Geochemistry: Elsevier, v. 4, p. 457-496. 200 Meters KEY Ground-Referenced Samples Classification MORB High-Silica Expert Defined MORB Dome MORB Transitional High-Silica ¯ High-Silica Region MORB Region High-Silica Region MORB Region ¯ Regional Classification - Classification result data distribution determined three classes (red, yellow, blue) majority filtered with a 25 m radius gridded at 2 m2 - Blue represents areas of MORB classified ANFIS with values <1.2 - Yellow represents mixed classification ranging in ANFIS values between 1.2 - 1.7 - Red represents exclusively high-silica lavas with ANFIS values >1.7 Alarcon Rise Bathymetry - AUV bathymetry gridded at 1 m2 collected by AUV D. Allen B. in 2012 overlaying ESRI World-Ocean basemap obtained from multiple contributors -ROV Doc Ricketts dive tracks during 2012 and 2015 -Training and testing data in the high-silica region and MORB region were classified using the 25 m majority filtered ANFIS result -Classification values at high-silica region range between 0.9 and 1.5 for MORB and between 1.2 and 2.0 for high-silica lavas -Classification of MORB region data range from 0.9 to 1.7 Number of Samples MORB Expert Defined MORB Domes High-Silica Lava Expert Defined MORB Domes MORB MORB Region High-Silica Region Ground-Referenced Data Classification -ANFIS classification for the 100 m 2 sampling square on the high-silica dome resulted in a value of 1.3 -Two sampling zones of 100 m 2 were constructed on a MORB dome and flat MORB area -Classification of the MORB dome ranged from 1.3-2.0 -Classification of the flat MORB area ranged from 0.9-1.5 Number of Samples Focus-Area Classification - Of the 0.98 km2 high-silica region, ANFIS classified 20.6% as MORB, 64.9% as transitional, and 14.5% as high-silica lava -Of the 4.45 km 2 MORB region, ANFIS classified 69.8% as MORB, 21.0% as transitional, and 9.2% as high-silica lava Class ANFIS Total Producer's Accuracy User's Accuracy MORB 167.0 80.2% 73.2% Evolved 80.0 38.8% 48.8% Relative Abundance of Lava Composition (%) High-Silica Lava Transitional MORB Conclusions - Because spreading rate remains constant at the Alarcon Rise, differences in lava flow morphology result from differences in lava viscosity and can be used to distinguish high-silica lava flows from MORB flows - Local slope, BPI texture, and sonar backscatter texture do not signficantly distinguish between high-silica lava and MORB domes - e amount of high-silica lava present at the Alarcon Rise cannot be accurately determined by a classifier with 66.8% overall accuracy Future Work - Dome classification may improve classification of compositional differences between high-silica lavas and MORB because high-silica lava flows only form coorugated pillows and blocky domes - e current classifier cannot distinguish between large silica-rich domes and small MORB domes there- fore training and testing data should only be picked at domes rather than on MORB sheet and lobate flows - A shape-recognition parameter may aid in classification because MORB domes form circular outlines and high-silica domes form rectangular outlines Acknowledgements - Science team, AUV team, ROV pilots, and crews of the 2012 and 2015 Alarcon Rise cruises on the R/V Zephyr and Western Flyer - e Monterey Bay Aquarium Reserach Institute - e Department of Earth and Ocean Sciences at the University of South Carolina, Columbia ANFIS Results

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Page 1: Maschmeyer AGU2015 compressedseoe.sc.edu/.../Maschmeyer_AGU2015_compressed.pdf · 2016. 2. 8. · Training Data Testing Data Submarine Lava Morphology Typical oceanic ridge lava exhibits

Detection of high-silica lava �ows and lava morphology at the Alarcon Rise, Gulf of California, Mexico using automated classi�cation of the morphological-compositional relationship in AUV multibeam bathymetry and sonar backscatter

Christina A. Maschmeyer ([email protected])1, Scott M. White1, Brian M. Dreyer2, David A. Clague3

University of South Carolina, Columbia, SC1 University of California, Santa Cruz, CA2 Monterey Bay Aquarium Research Institute, Moss Landing, CA3

Introduction and Objectives�e Alarcon Rise is the southernmost spreading ridge in the Gulf of California, Mexico. �e Alarcon Rise is an intermediate-rate spreading center with a full spreading rate of 50 cm/yr. Eruption processes of lava e�usion rate (which corresponds to spreading rate), underlying topography, and lava viscosity control the formation of submarine lava morphologies for mid-oceanic ridge basalt (MORB) [Gregg and Fink (1995)]. Typical MORB exists at the Alarcon Rise, but researchers from the Monterey Bay Aquarium Research Institute (MBARI) and Scripps Oceanographic Institute collected volcanic samples with elevated silica content [Castillo et al. (2002)].

Because submarine lava morphology depends on eruption processes, we propose to use morphologic signatures to identify evolved lavas. Our three primary questions for this research are:1. Can lava composition be determined by lava �ow morphology? 2. What morphologic signatures are critical to identi�cation of lavas with elevated silica? 3. How much high-silica lava exists at the Alarcon Rise?

We built an arti�cial intelligence classi�er to begin to answer these questions at the Alarcon Rise.

Expert Classi�cation- Construction of an adaptive neuro-fuzzy inference system (ANFIS) enabled the classi�cation of lava composition- Inputs were local slope and texture datasets from high-resolution bathymetry and sonar backscatter collected by AUV D. Allen B. in 2012.- Training cycle data included of 134 ground-referenced igneous samples collected by MBARI in 2012 and 2015 plus 48 points on MORB domes generated in ArcGIS along ROV track lines- Testing data consisted of 47 expert-picked MORB dome samples and 200 ground-referenced igneous samples collected in 2012 and 2015- We applied the classi�cation to two regions along the Alarcon Rise: a high-silica region and a MORB region

AUV BathymetryAUV Bathymetry Sidescan Sonar Backscatter

Sidescan Sonar Backscatter

GLCM TexturesGLCM TexturesLocal SlopeLocal Slope GLCM TexturesGLCM Textures

ANFISANFIS Classi�cationClassi�cation

Accuracy AssessmentAccuracy

Assessment

Ground Referenced Igneous Rock Samples

Ground Referenced Igneous Rock Samples

Training DataTraining Data Testing DataTesting Data

Submarine Lava MorphologyTypical oceanic ridge lava exhibits three distinct morphologies: sheet �ows, lobate �ows and small pillow mounds (~150 m diameter). Lava e�usion rate, viscosity, and underlying topography determine the morphologic di�erences between �ows [Gregg and Fink (1995)]. Lava e�usion rate is the most in�uential variable at spreading ridges with compositionally uniform lava [White and Klein (2014)].

Spreading ridges with silica-rich lavas do not exhibit submarine lava �ow morphologies. Large pillows with extreme radial jointing and corrugated surfaces and asymmetrical lava blocks build large domes. Angular, blocky talus is also common at silica-rich domes [Wanless et al. (2010)]. �e high-silica region of interest includes a large (~500 m diameter) dome.

MORB Morphology

Shee

tLo

bate

Pillo

w

High-Silica Lava Morphology

Rad

ial J

oint

ing

Lava

Blo

cks

Cor

ruga

ted

Pillo

w

High-Silica Dome

Distance (m)550500450400350300250200150100500

Dep

th (m

)

-2,340

-2,360

-2,380

-2,400

-2,420

-2,440

-2,460

MORB Dome

Depth (m)550500450400350300250200150100500

Dep

th (m

)

-2,330

-2,340

-2,350

-2,360

-2,370

-2,380

Sea�oor Mapping and Sampling- February-April 2012 and 2015, MBARI mapped the Alarcon Rise at 1 m horizontal resolution using the AUV (Autonomous Underwater Vehicle) D. Allen B. We created inputs for the expert classi�er from bathymetry and sonar backscatter collected during 2012 - MBARI collected 410 rock samples over 19 dives by the ROV (remotely operated vehicle) Doc Ricketts -364 igneous samples collected along the spreading ridge were used during classi�cation

Completed Dives Trackline Coverage

Basalt Basaltic Andesite Andesite Dacite Rhyolite Total

9 36.3 km 135 7 6 7 35 190

10 38.6 km 97 14 37 16 10 174

Igneous Rock Samples

References- Castillo, P.R., Hawkins, J.W., Lonsdale, P.F., Hilton, D.R., and Shaw, A.M., 2002, Petrology of the Alarcon Rise lavas, Gulf of California: Nascent intracontinental ocean crust: Journal of Geophysical Research, v. 107, no.B10, p. 1-15.- Gregg, P.M., Fink, J.H., 1995, Quanti�cation of submarine lava-�ow morphology through analog experiments: Geology, v. 23, n.1, p. 73-76.- Wanless, V.D., Per�t, M.R., Ridley, W.L., and Klein, E., 2010, Dacite petrogenesis on mid-ocean ridges: Evidence for oceanic crustal melting and assimilitaion: Journal of Petrology, v. 51, n. 12, p. 2377-2410.-White, W.M., and Klein, E.M., 2014, Composition of the Oceanic Crust, in Saunders, J.A.,Hofstra, A.H., Goldfarb, R.J., and Reed, M.H., eds., Treatise on Geochemistry: Elsevier, v. 4, p. 457-496.

200Meters

KEY

Ground-Referenced Samples

Classi�cationMORB

High-Silica

Expert De�ned MORB Dome

MORB

Transitional

High-Silica

¯

High-Silica Region

MORB Region

High-Silica Region

MORB Region

¯

Regional Classi�cation- Classi�cation result data distribution determined three classes (red, yellow, blue) majority �ltered with a 25 m radius gridded at 2 m2- Blue represents areas of MORB classi�ed ANFIS with values <1.2- Yellow represents mixed classi�cation ranging in ANFIS values between 1.2 - 1.7- Red represents exclusively high-silica lavas with ANFIS values >1.7

Alarcon Rise Bathymetry- AUV bathymetry gridded at 1 m2 collected by AUV D. Allen B. in 2012 overlaying ESRI World-Ocean basemap obtained from multiple contributors-ROV Doc Ricketts dive tracks during 2012 and 2015

-Training and testing data in the high-silica region and MORB region were classi�ed using the 25 m majority �ltered ANFIS result-Classi�cation values at high-silica region range between 0.9 and 1.5 for MORB and between 1.2 and 2.0 for high-silica lavas-Classi�cation of MORB region data range from 0.9 to 1.7

Num

ber o

f Sam

ples

MORB

Expert De�nedMORB Domes

High-Silica LavaExpert De�nedMORB Domes

MORB

MORB RegionHigh-Silica Region

Ground-Referenced Data Classi�cation

-ANFIS classi�cation for the 100 m2 sampling square on the high-silica dome resulted in a value of 1.3-Two sampling zones of 100 m2 were constructed on a MORB dome and �at MORB area-Classi�cation of the MORB dome ranged from 1.3-2.0-Classi�cation of the �at MORB area ranged from 0.9-1.5

Num

ber o

f Sam

ples

Focus-Area Classi�cation

- Of the 0.98 km2 high-silica region, ANFIS classi�ed 20.6% as MORB, 64.9% as transitional, and 14.5% as high-silica lava-Of the 4.45 km2 MORB region, ANFIS classi�ed 69.8% as MORB, 21.0% as transitional, and 9.2% as high-silica lava

Class ANFIS Total Producer's Accuracy User's Accuracy

MORB 167.0 80.2% 73.2%

Evolved 80.0 38.8% 48.8%

Rela

tive A

bund

ance

of

Lava

Com

posit

ion

(%) High-Silica Lava

Transitional

MORB

Conclusions- Because spreading rate remains constant at the Alarcon Rise, di�erences in lava �ow morphology result from di�erences in lava viscosity and can be used to distinguish high-silica lava �ows from MORB �ows - Local slope, BPI texture, and sonar backscatter texture do not sign�cantly distinguish between high-silica lava and MORB domes- �e amount of high-silica lava present at the Alarcon Rise cannot be accurately determined by a classi�er with 66.8% overall accuracy

Future Work- Dome classi�cation may improve classi�cation of compositional di�erences between high-silica lavas and MORB because high-silica lava �ows only form coorugated pillows and blocky domes- �e current classi�er cannot distinguish between large silica-rich domes and small MORB domes there-fore training and testing data should only be picked at domes rather than on MORB sheet and lobate �ows- A shape-recognition parameter may aid in classi�cation because MORB domes form circular outlines and high-silica domes form rectangular outlines

Acknowledgements- Science team, AUV team, ROV pilots, and crews of the 2012 and 2015 Alarcon Rise cruises on the R/V Zephyr and Western Flyer- �e Monterey Bay Aquarium Reserach Institute- �e Department of Earth and Ocean Sciences at the University of South Carolina, Columbia

ANFIS Results