Volcanic hazard from San Martin Tuxtla Volcano, Tuxtla Volcanic Field, Veracruz, México: probability maps of ashfall deposition from possible future eruption

Abstract San Martin Tuxtla Volcano, the largest and highest edifice in the Tuxtla Volcanic Field, had explosive eruptions in 1664 and 1793. This volcano poses the highest hazard for the growing population centers surrounding it. The impacts and deposits of the 1793 eruption have been studied recentl...
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Autor*in:	Espíndola, J. M. [verfasserIn] Godinez, M. L. [verfasserIn] Zamora-Camacho, A. [verfasserIn]

Format:	E-Artikel
Sprache:	Englisch

Erschienen:	2011

Schlagwörter:	San Martin Tuxtla Volcano Tuxtla Volcanic Field Basaltic explosive eruptions Basaltic Volcanic Fields Ash distribution Volcanic risk

Übergeordnetes Werk:	Enthalten in: Natural hazards - Dordrecht [u.a.] : Springer Science + Business Media B.V., 1988, 61(2011), 2 vom: 22. Dez., Seite 771-784
Übergeordnetes Werk:	volume:61 ; year:2011 ; number:2 ; day:22 ; month:12 ; pages:771-784

Links:	Volltext

DOI / URN:	10.1007/s11069-011-0063-7

Katalog-ID:	SPR016303628

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100	1		\|a Espíndola, J. M. \|e verfasserin \|4 aut
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520			\|a Abstract San Martin Tuxtla Volcano, the largest and highest edifice in the Tuxtla Volcanic Field, had explosive eruptions in 1664 and 1793. This volcano poses the highest hazard for the growing population centers surrounding it. The impacts and deposits of the 1793 eruption have been studied recently, and some of its characteristics, such as eruptive mass, grain-size distribution of the products and plume height, have been estimated. These data, together with daily data on wind velocities taken in the nearby city of Veracruz, have been used to conduct numerical modeling of ash distribution from an eruptive column comparable to that estimated during the 1793 event. Using wind velocities of randomly chosen days, we constructed probability maps of areas likely to receive, at least 1, 5, or 10 cm of ash. Our results indicate that an area about 1.3 × $ 10^{4} $ $ km^{2} $ has a 12% probability of being covered by an ash fall more than 1 cm thick, if a mass of $ 10^{14} $ g was erupted and deposited from a 10-km-high eruptive plume. The results presented in this paper serve as a scientific basis to estimate volcano risk in the area from a possible eruption, consisting of one or several large explosive events, at San Martin Tuxtla volcano.
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matchkey_str	article:15730840:2011----::ocncaadrmamritxlvlaoutaocncilvrcumiorbbltmpoahale
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publishDate	2011
allfields	10.1007/s11069-011-0063-7 doi (DE-627)SPR016303628 (SPR)s11069-011-0063-7-e DE-627 ger DE-627 rakwb eng 550 ASE 31.00 bkl 43.48 bkl Espíndola, J. M. verfasserin aut Volcanic hazard from San Martin Tuxtla Volcano, Tuxtla Volcanic Field, Veracruz, México: probability maps of ashfall deposition from possible future eruption 2011 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract San Martin Tuxtla Volcano, the largest and highest edifice in the Tuxtla Volcanic Field, had explosive eruptions in 1664 and 1793. This volcano poses the highest hazard for the growing population centers surrounding it. The impacts and deposits of the 1793 eruption have been studied recently, and some of its characteristics, such as eruptive mass, grain-size distribution of the products and plume height, have been estimated. These data, together with daily data on wind velocities taken in the nearby city of Veracruz, have been used to conduct numerical modeling of ash distribution from an eruptive column comparable to that estimated during the 1793 event. Using wind velocities of randomly chosen days, we constructed probability maps of areas likely to receive, at least 1, 5, or 10 cm of ash. Our results indicate that an area about 1.3 × $ 10^{4} $ $ km^{2} $ has a 12% probability of being covered by an ash fall more than 1 cm thick, if a mass of $ 10^{14} $ g was erupted and deposited from a 10-km-high eruptive plume. The results presented in this paper serve as a scientific basis to estimate volcano risk in the area from a possible eruption, consisting of one or several large explosive events, at San Martin Tuxtla volcano. San Martin Tuxtla Volcano (dpeaa)DE-He213 Tuxtla Volcanic Field (dpeaa)DE-He213 Basaltic explosive eruptions (dpeaa)DE-He213 Basaltic Volcanic Fields (dpeaa)DE-He213 Ash distribution (dpeaa)DE-He213 Volcanic risk (dpeaa)DE-He213 Godinez, M. L. verfasserin aut Zamora-Camacho, A. verfasserin aut Enthalten in Natural hazards Dordrecht [u.a.] : Springer Science + Business Media B.V., 1988 61(2011), 2 vom: 22. Dez., Seite 771-784 (DE-627)315621729 (DE-600)2017806-2 1573-0840 nnns volume:61 year:2011 number:2 day:22 month:12 pages:771-784 https://dx.doi.org/10.1007/s11069-011-0063-7 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER SSG-OPC-GGO SSG-OPC-MAT SSG-OPC-ASE GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2070 GBV_ILN_2086 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2116 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 31.00 ASE 43.48 ASE AR 61 2011 2 22 12 771-784
spelling	10.1007/s11069-011-0063-7 doi (DE-627)SPR016303628 (SPR)s11069-011-0063-7-e DE-627 ger DE-627 rakwb eng 550 ASE 31.00 bkl 43.48 bkl Espíndola, J. M. verfasserin aut Volcanic hazard from San Martin Tuxtla Volcano, Tuxtla Volcanic Field, Veracruz, México: probability maps of ashfall deposition from possible future eruption 2011 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract San Martin Tuxtla Volcano, the largest and highest edifice in the Tuxtla Volcanic Field, had explosive eruptions in 1664 and 1793. This volcano poses the highest hazard for the growing population centers surrounding it. The impacts and deposits of the 1793 eruption have been studied recently, and some of its characteristics, such as eruptive mass, grain-size distribution of the products and plume height, have been estimated. These data, together with daily data on wind velocities taken in the nearby city of Veracruz, have been used to conduct numerical modeling of ash distribution from an eruptive column comparable to that estimated during the 1793 event. Using wind velocities of randomly chosen days, we constructed probability maps of areas likely to receive, at least 1, 5, or 10 cm of ash. Our results indicate that an area about 1.3 × $ 10^{4} $ $ km^{2} $ has a 12% probability of being covered by an ash fall more than 1 cm thick, if a mass of $ 10^{14} $ g was erupted and deposited from a 10-km-high eruptive plume. The results presented in this paper serve as a scientific basis to estimate volcano risk in the area from a possible eruption, consisting of one or several large explosive events, at San Martin Tuxtla volcano. San Martin Tuxtla Volcano (dpeaa)DE-He213 Tuxtla Volcanic Field (dpeaa)DE-He213 Basaltic explosive eruptions (dpeaa)DE-He213 Basaltic Volcanic Fields (dpeaa)DE-He213 Ash distribution (dpeaa)DE-He213 Volcanic risk (dpeaa)DE-He213 Godinez, M. L. verfasserin aut Zamora-Camacho, A. verfasserin aut Enthalten in Natural hazards Dordrecht [u.a.] : Springer Science + Business Media B.V., 1988 61(2011), 2 vom: 22. Dez., Seite 771-784 (DE-627)315621729 (DE-600)2017806-2 1573-0840 nnns volume:61 year:2011 number:2 day:22 month:12 pages:771-784 https://dx.doi.org/10.1007/s11069-011-0063-7 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER SSG-OPC-GGO SSG-OPC-MAT SSG-OPC-ASE GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2070 GBV_ILN_2086 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2116 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 31.00 ASE 43.48 ASE AR 61 2011 2 22 12 771-784
allfields_unstemmed	10.1007/s11069-011-0063-7 doi (DE-627)SPR016303628 (SPR)s11069-011-0063-7-e DE-627 ger DE-627 rakwb eng 550 ASE 31.00 bkl 43.48 bkl Espíndola, J. M. verfasserin aut Volcanic hazard from San Martin Tuxtla Volcano, Tuxtla Volcanic Field, Veracruz, México: probability maps of ashfall deposition from possible future eruption 2011 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract San Martin Tuxtla Volcano, the largest and highest edifice in the Tuxtla Volcanic Field, had explosive eruptions in 1664 and 1793. This volcano poses the highest hazard for the growing population centers surrounding it. The impacts and deposits of the 1793 eruption have been studied recently, and some of its characteristics, such as eruptive mass, grain-size distribution of the products and plume height, have been estimated. These data, together with daily data on wind velocities taken in the nearby city of Veracruz, have been used to conduct numerical modeling of ash distribution from an eruptive column comparable to that estimated during the 1793 event. Using wind velocities of randomly chosen days, we constructed probability maps of areas likely to receive, at least 1, 5, or 10 cm of ash. Our results indicate that an area about 1.3 × $ 10^{4} $ $ km^{2} $ has a 12% probability of being covered by an ash fall more than 1 cm thick, if a mass of $ 10^{14} $ g was erupted and deposited from a 10-km-high eruptive plume. The results presented in this paper serve as a scientific basis to estimate volcano risk in the area from a possible eruption, consisting of one or several large explosive events, at San Martin Tuxtla volcano. San Martin Tuxtla Volcano (dpeaa)DE-He213 Tuxtla Volcanic Field (dpeaa)DE-He213 Basaltic explosive eruptions (dpeaa)DE-He213 Basaltic Volcanic Fields (dpeaa)DE-He213 Ash distribution (dpeaa)DE-He213 Volcanic risk (dpeaa)DE-He213 Godinez, M. L. verfasserin aut Zamora-Camacho, A. verfasserin aut Enthalten in Natural hazards Dordrecht [u.a.] : Springer Science + Business Media B.V., 1988 61(2011), 2 vom: 22. Dez., Seite 771-784 (DE-627)315621729 (DE-600)2017806-2 1573-0840 nnns volume:61 year:2011 number:2 day:22 month:12 pages:771-784 https://dx.doi.org/10.1007/s11069-011-0063-7 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER SSG-OPC-GGO SSG-OPC-MAT SSG-OPC-ASE GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2070 GBV_ILN_2086 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2116 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 31.00 ASE 43.48 ASE AR 61 2011 2 22 12 771-784
allfieldsGer	10.1007/s11069-011-0063-7 doi (DE-627)SPR016303628 (SPR)s11069-011-0063-7-e DE-627 ger DE-627 rakwb eng 550 ASE 31.00 bkl 43.48 bkl Espíndola, J. M. verfasserin aut Volcanic hazard from San Martin Tuxtla Volcano, Tuxtla Volcanic Field, Veracruz, México: probability maps of ashfall deposition from possible future eruption 2011 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract San Martin Tuxtla Volcano, the largest and highest edifice in the Tuxtla Volcanic Field, had explosive eruptions in 1664 and 1793. This volcano poses the highest hazard for the growing population centers surrounding it. The impacts and deposits of the 1793 eruption have been studied recently, and some of its characteristics, such as eruptive mass, grain-size distribution of the products and plume height, have been estimated. These data, together with daily data on wind velocities taken in the nearby city of Veracruz, have been used to conduct numerical modeling of ash distribution from an eruptive column comparable to that estimated during the 1793 event. Using wind velocities of randomly chosen days, we constructed probability maps of areas likely to receive, at least 1, 5, or 10 cm of ash. Our results indicate that an area about 1.3 × $ 10^{4} $ $ km^{2} $ has a 12% probability of being covered by an ash fall more than 1 cm thick, if a mass of $ 10^{14} $ g was erupted and deposited from a 10-km-high eruptive plume. The results presented in this paper serve as a scientific basis to estimate volcano risk in the area from a possible eruption, consisting of one or several large explosive events, at San Martin Tuxtla volcano. San Martin Tuxtla Volcano (dpeaa)DE-He213 Tuxtla Volcanic Field (dpeaa)DE-He213 Basaltic explosive eruptions (dpeaa)DE-He213 Basaltic Volcanic Fields (dpeaa)DE-He213 Ash distribution (dpeaa)DE-He213 Volcanic risk (dpeaa)DE-He213 Godinez, M. L. verfasserin aut Zamora-Camacho, A. verfasserin aut Enthalten in Natural hazards Dordrecht [u.a.] : Springer Science + Business Media B.V., 1988 61(2011), 2 vom: 22. Dez., Seite 771-784 (DE-627)315621729 (DE-600)2017806-2 1573-0840 nnns volume:61 year:2011 number:2 day:22 month:12 pages:771-784 https://dx.doi.org/10.1007/s11069-011-0063-7 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER SSG-OPC-GGO SSG-OPC-MAT SSG-OPC-ASE GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2070 GBV_ILN_2086 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2116 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 31.00 ASE 43.48 ASE AR 61 2011 2 22 12 771-784
allfieldsSound	10.1007/s11069-011-0063-7 doi (DE-627)SPR016303628 (SPR)s11069-011-0063-7-e DE-627 ger DE-627 rakwb eng 550 ASE 31.00 bkl 43.48 bkl Espíndola, J. M. verfasserin aut Volcanic hazard from San Martin Tuxtla Volcano, Tuxtla Volcanic Field, Veracruz, México: probability maps of ashfall deposition from possible future eruption 2011 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract San Martin Tuxtla Volcano, the largest and highest edifice in the Tuxtla Volcanic Field, had explosive eruptions in 1664 and 1793. This volcano poses the highest hazard for the growing population centers surrounding it. The impacts and deposits of the 1793 eruption have been studied recently, and some of its characteristics, such as eruptive mass, grain-size distribution of the products and plume height, have been estimated. These data, together with daily data on wind velocities taken in the nearby city of Veracruz, have been used to conduct numerical modeling of ash distribution from an eruptive column comparable to that estimated during the 1793 event. Using wind velocities of randomly chosen days, we constructed probability maps of areas likely to receive, at least 1, 5, or 10 cm of ash. Our results indicate that an area about 1.3 × $ 10^{4} $ $ km^{2} $ has a 12% probability of being covered by an ash fall more than 1 cm thick, if a mass of $ 10^{14} $ g was erupted and deposited from a 10-km-high eruptive plume. The results presented in this paper serve as a scientific basis to estimate volcano risk in the area from a possible eruption, consisting of one or several large explosive events, at San Martin Tuxtla volcano. San Martin Tuxtla Volcano (dpeaa)DE-He213 Tuxtla Volcanic Field (dpeaa)DE-He213 Basaltic explosive eruptions (dpeaa)DE-He213 Basaltic Volcanic Fields (dpeaa)DE-He213 Ash distribution (dpeaa)DE-He213 Volcanic risk (dpeaa)DE-He213 Godinez, M. L. verfasserin aut Zamora-Camacho, A. verfasserin aut Enthalten in Natural hazards Dordrecht [u.a.] : Springer Science + Business Media B.V., 1988 61(2011), 2 vom: 22. Dez., Seite 771-784 (DE-627)315621729 (DE-600)2017806-2 1573-0840 nnns volume:61 year:2011 number:2 day:22 month:12 pages:771-784 https://dx.doi.org/10.1007/s11069-011-0063-7 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER SSG-OPC-GGO SSG-OPC-MAT SSG-OPC-ASE GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2070 GBV_ILN_2086 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2116 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 31.00 ASE 43.48 ASE AR 61 2011 2 22 12 771-784
language	English
source	Enthalten in Natural hazards 61(2011), 2 vom: 22. Dez., Seite 771-784 volume:61 year:2011 number:2 day:22 month:12 pages:771-784
sourceStr	Enthalten in Natural hazards 61(2011), 2 vom: 22. Dez., Seite 771-784 volume:61 year:2011 number:2 day:22 month:12 pages:771-784
format_phy_str_mv	Article
institution	findex.gbv.de
topic_facet	San Martin Tuxtla Volcano Tuxtla Volcanic Field Basaltic explosive eruptions Basaltic Volcanic Fields Ash distribution Volcanic risk
dewey-raw	550
isfreeaccess_bool	false
container_title	Natural hazards
authorswithroles_txt_mv	Espíndola, J. M. @@aut@@ Godinez, M. L. @@aut@@ Zamora-Camacho, A. @@aut@@
publishDateDaySort_date	2011-12-22T00:00:00Z
hierarchy_top_id	315621729
dewey-sort	3550
id	SPR016303628
language_de	englisch
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author	Espíndola, J. M.
spellingShingle	Espíndola, J. M. ddc 550 bkl 31.00 bkl 43.48 misc San Martin Tuxtla Volcano misc Tuxtla Volcanic Field misc Basaltic explosive eruptions misc Basaltic Volcanic Fields misc Ash distribution misc Volcanic risk Volcanic hazard from San Martin Tuxtla Volcano, Tuxtla Volcanic Field, Veracruz, México: probability maps of ashfall deposition from possible future eruption
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topic_title	550 ASE 31.00 bkl 43.48 bkl Volcanic hazard from San Martin Tuxtla Volcano, Tuxtla Volcanic Field, Veracruz, México: probability maps of ashfall deposition from possible future eruption San Martin Tuxtla Volcano (dpeaa)DE-He213 Tuxtla Volcanic Field (dpeaa)DE-He213 Basaltic explosive eruptions (dpeaa)DE-He213 Basaltic Volcanic Fields (dpeaa)DE-He213 Ash distribution (dpeaa)DE-He213 Volcanic risk (dpeaa)DE-He213
topic	ddc 550 bkl 31.00 bkl 43.48 misc San Martin Tuxtla Volcano misc Tuxtla Volcanic Field misc Basaltic explosive eruptions misc Basaltic Volcanic Fields misc Ash distribution misc Volcanic risk
topic_unstemmed	ddc 550 bkl 31.00 bkl 43.48 misc San Martin Tuxtla Volcano misc Tuxtla Volcanic Field misc Basaltic explosive eruptions misc Basaltic Volcanic Fields misc Ash distribution misc Volcanic risk
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title	Volcanic hazard from San Martin Tuxtla Volcano, Tuxtla Volcanic Field, Veracruz, México: probability maps of ashfall deposition from possible future eruption
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title_full	Volcanic hazard from San Martin Tuxtla Volcano, Tuxtla Volcanic Field, Veracruz, México: probability maps of ashfall deposition from possible future eruption
author_sort	Espíndola, J. M.
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author_browse	Espíndola, J. M. Godinez, M. L. Zamora-Camacho, A.
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author-letter	Espíndola, J. M.
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title_sort	volcanic hazard from san martin tuxtla volcano, tuxtla volcanic field, veracruz, méxico: probability maps of ashfall deposition from possible future eruption
title_auth	Volcanic hazard from San Martin Tuxtla Volcano, Tuxtla Volcanic Field, Veracruz, México: probability maps of ashfall deposition from possible future eruption
abstract	Abstract San Martin Tuxtla Volcano, the largest and highest edifice in the Tuxtla Volcanic Field, had explosive eruptions in 1664 and 1793. This volcano poses the highest hazard for the growing population centers surrounding it. The impacts and deposits of the 1793 eruption have been studied recently, and some of its characteristics, such as eruptive mass, grain-size distribution of the products and plume height, have been estimated. These data, together with daily data on wind velocities taken in the nearby city of Veracruz, have been used to conduct numerical modeling of ash distribution from an eruptive column comparable to that estimated during the 1793 event. Using wind velocities of randomly chosen days, we constructed probability maps of areas likely to receive, at least 1, 5, or 10 cm of ash. Our results indicate that an area about 1.3 × $ 10^{4} $ $ km^{2} $ has a 12% probability of being covered by an ash fall more than 1 cm thick, if a mass of $ 10^{14} $ g was erupted and deposited from a 10-km-high eruptive plume. The results presented in this paper serve as a scientific basis to estimate volcano risk in the area from a possible eruption, consisting of one or several large explosive events, at San Martin Tuxtla volcano.
abstractGer	Abstract San Martin Tuxtla Volcano, the largest and highest edifice in the Tuxtla Volcanic Field, had explosive eruptions in 1664 and 1793. This volcano poses the highest hazard for the growing population centers surrounding it. The impacts and deposits of the 1793 eruption have been studied recently, and some of its characteristics, such as eruptive mass, grain-size distribution of the products and plume height, have been estimated. These data, together with daily data on wind velocities taken in the nearby city of Veracruz, have been used to conduct numerical modeling of ash distribution from an eruptive column comparable to that estimated during the 1793 event. Using wind velocities of randomly chosen days, we constructed probability maps of areas likely to receive, at least 1, 5, or 10 cm of ash. Our results indicate that an area about 1.3 × $ 10^{4} $ $ km^{2} $ has a 12% probability of being covered by an ash fall more than 1 cm thick, if a mass of $ 10^{14} $ g was erupted and deposited from a 10-km-high eruptive plume. The results presented in this paper serve as a scientific basis to estimate volcano risk in the area from a possible eruption, consisting of one or several large explosive events, at San Martin Tuxtla volcano.
abstract_unstemmed	Abstract San Martin Tuxtla Volcano, the largest and highest edifice in the Tuxtla Volcanic Field, had explosive eruptions in 1664 and 1793. This volcano poses the highest hazard for the growing population centers surrounding it. The impacts and deposits of the 1793 eruption have been studied recently, and some of its characteristics, such as eruptive mass, grain-size distribution of the products and plume height, have been estimated. These data, together with daily data on wind velocities taken in the nearby city of Veracruz, have been used to conduct numerical modeling of ash distribution from an eruptive column comparable to that estimated during the 1793 event. Using wind velocities of randomly chosen days, we constructed probability maps of areas likely to receive, at least 1, 5, or 10 cm of ash. Our results indicate that an area about 1.3 × $ 10^{4} $ $ km^{2} $ has a 12% probability of being covered by an ash fall more than 1 cm thick, if a mass of $ 10^{14} $ g was erupted and deposited from a 10-km-high eruptive plume. The results presented in this paper serve as a scientific basis to estimate volcano risk in the area from a possible eruption, consisting of one or several large explosive events, at San Martin Tuxtla volcano.
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title_short	Volcanic hazard from San Martin Tuxtla Volcano, Tuxtla Volcanic Field, Veracruz, México: probability maps of ashfall deposition from possible future eruption
url	https://dx.doi.org/10.1007/s11069-011-0063-7
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fullrecord_marcxml	<?xml version="1.0" encoding="UTF-8"?><collection xmlns="http://www.loc.gov/MARC21/slim"><record><leader>01000caa a22002652 4500</leader><controlfield tag="001">SPR016303628</controlfield><controlfield tag="003">DE-627</controlfield><controlfield tag="005">20220111030858.0</controlfield><controlfield tag="007">cr uuu---uuuuu</controlfield><controlfield tag="008">201006s2011 xx \|\|\|\|\|o 00\| \|\|eng c</controlfield><datafield tag="024" ind1="7" ind2=" "><subfield code="a">10.1007/s11069-011-0063-7</subfield><subfield code="2">doi</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-627)SPR016303628</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(SPR)s11069-011-0063-7-e</subfield></datafield><datafield tag="040" ind1=" " ind2=" "><subfield code="a">DE-627</subfield><subfield code="b">ger</subfield><subfield code="c">DE-627</subfield><subfield code="e">rakwb</subfield></datafield><datafield tag="041" ind1=" " ind2=" "><subfield code="a">eng</subfield></datafield><datafield tag="082" ind1="0" ind2="4"><subfield code="a">550</subfield><subfield code="q">ASE</subfield></datafield><datafield tag="084" ind1=" " ind2=" "><subfield code="a">31.00</subfield><subfield code="2">bkl</subfield></datafield><datafield tag="084" ind1=" " ind2=" "><subfield code="a">43.48</subfield><subfield code="2">bkl</subfield></datafield><datafield tag="100" ind1="1" ind2=" "><subfield code="a">Espíndola, J. M.</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="245" ind1="1" ind2="0"><subfield code="a">Volcanic hazard from San Martin Tuxtla Volcano, Tuxtla Volcanic Field, Veracruz, México: probability maps of ashfall deposition from possible future eruption</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="c">2011</subfield></datafield><datafield tag="336" ind1=" " ind2=" "><subfield code="a">Text</subfield><subfield code="b">txt</subfield><subfield code="2">rdacontent</subfield></datafield><datafield tag="337" ind1=" " ind2=" "><subfield code="a">Computermedien</subfield><subfield code="b">c</subfield><subfield code="2">rdamedia</subfield></datafield><datafield tag="338" ind1=" " ind2=" "><subfield code="a">Online-Ressource</subfield><subfield code="b">cr</subfield><subfield code="2">rdacarrier</subfield></datafield><datafield tag="520" ind1=" " ind2=" "><subfield code="a">Abstract San Martin Tuxtla Volcano, the largest and highest edifice in the Tuxtla Volcanic Field, had explosive eruptions in 1664 and 1793. This volcano poses the highest hazard for the growing population centers surrounding it. The impacts and deposits of the 1793 eruption have been studied recently, and some of its characteristics, such as eruptive mass, grain-size distribution of the products and plume height, have been estimated. These data, together with daily data on wind velocities taken in the nearby city of Veracruz, have been used to conduct numerical modeling of ash distribution from an eruptive column comparable to that estimated during the 1793 event. Using wind velocities of randomly chosen days, we constructed probability maps of areas likely to receive, at least 1, 5, or 10 cm of ash. Our results indicate that an area about 1.3 × $ 10^{4} $ $ km^{2} $ has a 12% probability of being covered by an ash fall more than 1 cm thick, if a mass of $ 10^{14} $ g was erupted and deposited from a 10-km-high eruptive plume. The results presented in this paper serve as a scientific basis to estimate volcano risk in the area from a possible eruption, consisting of one or several large explosive events, at San Martin Tuxtla volcano.</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">San Martin Tuxtla Volcano</subfield><subfield code="7">(dpeaa)DE-He213</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Tuxtla Volcanic Field</subfield><subfield code="7">(dpeaa)DE-He213</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Basaltic explosive eruptions</subfield><subfield code="7">(dpeaa)DE-He213</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Basaltic Volcanic Fields</subfield><subfield code="7">(dpeaa)DE-He213</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Ash distribution</subfield><subfield code="7">(dpeaa)DE-He213</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Volcanic risk</subfield><subfield code="7">(dpeaa)DE-He213</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Godinez, M. 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Volcanic hazard from San Martin Tuxtla Volcano, Tuxtla Volcanic Field, Veracruz, México: probability maps of ashfall deposition from possible future eruption

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