1. Funkhouser, John G. and Naughton, John J., 1968, Radiogenic helium and argon in ultramafic inclusions from Hawaii: Journal of Geophysical Research: v. 73, no. 14: p. 4601-4607.
BibTeX
@article{funkhouser1968radiogenic,
author = "Funkhouser, John G. and Naughton, John J.",
title = "Radiogenic helium and argon in ultramafic inclusions from Hawaii",
year = "1968",
journal = "Journal of Geophysical Research",
url = "https://doi.org/10.1029/jb073i014p04601",
doi = "10.1029/jb073i014p04601",
number = "14",
openalex = "W2111713749",
pages = "4601-4607",
volume = "73",
references = "doi101007bf00518082, doi101007bf02597182, doi1010160032063363901132, doi101029jz066i001p00277, doi101029jz070i002p00509, doi101038202526a0, doi101086200619, openalexw184644159, openalexw2020861622, openalexw2952019671"
}
2. Funkhouser, J. G. and Naughton, J. J, 1968, Radiogenic helium and argon in ultramafic inclusions in Hawaii: Journal of Geophysical Research, v. 73, p. 4601-4607.
BibTeX
@article{funkhouser1968radiogenic1,
author = "Funkhouser, J. G. and Naughton, J. J",
title = "Radiogenic helium and argon in ultramafic inclusions in Hawaii",
year = "1968",
journal = "Journal of Geophysical Research, v. 73, p. 4601-4607",
note = "talkorigins\_source = {true}; raw\_reference = {Funkhouser, J. G., and Naughton, J. J., 1968, Radiogenic helium and argon in ultramafic inclusions in Hawaii: Journal of Geophysical Research, v. 73, p. 4601-4607.}"
}
3. Spera, F, 1980, Thermal evolution of plutons.
BibTeX
@misc{spera1980thermal2,
author = "Spera, F",
title = "Thermal evolution of plutons",
year = "1980",
howpublished = "a parameterized approach: Science, v. 207, p. 299-301",
note = "talkorigins\_source = {true}; raw\_reference = {Spera, F., 1980, Thermal evolution of plutons: a parameterized approach: Science, v. 207, p. 299-301.}"
}
4. 1982, Igneous Petrology: Developments in Petrology.
BibTeX
@misc{crossref1982igneous,
title = "Igneous Petrology",
year = "1982",
booktitle = "Developments in Petrology",
url = "https://doi.org/10.1016/c2009-0-09603-2",
doi = "10.1016/c2009-0-09603-2",
openalex = "W4232304061"
}
5. Burley, Brian J., 1988, Igneous petrology: Geochimica et Cosmochimica Acta: v. 52, no. 3: p. 798.
DOI: 10.1016/0016-7037(88)90345-6
BibTeX
@article{burley1988igneous,
author = "Burley, Brian J.",
title = "Igneous petrology",
year = "1988",
journal = "Geochimica et Cosmochimica Acta",
url = "https://doi.org/10.1016/0016-7037(88)90345-6",
doi = "10.1016/0016-7037(88)90345-6",
number = "3",
openalex = "W1488095665",
pages = "798",
volume = "52"
}
6. 1989, Igneous Petrology: Geologiska Föreningen i Stockholm Förhandlingar: v. 111, no. 3: p. 304-304.
DOI: 10.1080/11035898909452720
BibTeX
@article{crossref1989igneous,
title = "Igneous Petrology",
year = "1989",
journal = "Geologiska Föreningen i Stockholm Förhandlingar",
url = "https://doi.org/10.1080/11035898909452720",
doi = "10.1080/11035898909452720",
number = "3",
openalex = "W4254782226",
pages = "304-304",
volume = "111"
}
7. Dunai, Tibor J. and Baur, H., 1995, Helium, neon, and argon systematics of the European subcontinental mantle: Implications for its geochemical evolution: Geochimica et Cosmochimica Acta.
DOI: 10.1016/0016-7037(95)00172-v
BibTeX
@article{doi101016001670379500172v,
author = "Dunai, Tibor J. and Baur, H.",
title = "Helium, neon, and argon systematics of the European subcontinental mantle: Implications for its geochemical evolution",
year = "1995",
journal = "Geochimica et Cosmochimica Acta",
url = "https://doi.org/10.1016/0016-7037(95)00172-v",
doi = "10.1016/0016-7037(95)00172-v",
openalex = "W2042660273",
references = "doi1010160009254186901397"
}
8. 2002, Igneous Petrology: Geology Today: v. 18, no. 3: p. 116-117.
DOI: 10.1046/j.1365-2451.2002.03434.x
BibTeX
@article{crossref2002igneous,
title = "Igneous Petrology",
year = "2002",
journal = "Geology Today",
url = "https://doi.org/10.1046/j.1365-2451.2002.03434.x",
doi = "10.1046/j.1365-2451.2002.03434.x",
number = "3",
openalex = "W4239442782",
pages = "116-117",
volume = "18"
}
9. 2014, igneous petrology: Dictionary Geotechnical Engineering/Wörterbuch GeoTechnik: p. 714-714.
DOI: 10.1007/978-3-642-41714-6_90246
BibTeX
@incollection{crossref2014igneous,
title = "igneous petrology",
year = "2014",
booktitle = "Dictionary Geotechnical Engineering/Wörterbuch GeoTechnik",
url = "https://doi.org/10.1007/978-3-642-41714-6\_90246",
doi = "10.1007/978-3-642-41714-6\_90246",
openalex = "W4249142906",
pages = "714-714"
}
10. Giesting, Paul A. and Schwenzer, S. P. and Filiberto, J. and Starkey, N. A. and Franchi, I. A. and Treiman, A. H. and Tindle, Andy and Grady, M. M., 2015, Igneous and shock processes affecting chassignite amphibole evaluated using chlorine/water partitioning and hydrogen isotopes: Meteoritics and Planetary Science.
Abstract
Abstract Amphibole in chassignite melt inclusions provides valuable information about the volatile content of the original interstitial magma, but also shock and postshock processes. We have analyzed amphibole and other phases from NWA 2737 melt inclusions, and we evaluate these data along with published values to constrain the crystallization Cl and H 2 O content of phases in chassignite melt inclusions and the effects of shock on these amphibole grains. Using a model for the Cl/ OH exchange between amphibole and melt, we estimate primary crystallization OH contents of chassignite amphiboles. SIMS analysis shows that amphibole from NWA 2737 currently has 0.15 wt% H 2 O. It has lost ~0.6 wt% H 2 O from an initial 0.7–0.8 wt% H 2 O due to intense shock. Chassigny amphibole had on average 0.3–0.4 wt% H 2 O and suffered little net loss of H 2 O due to shock. NWA 2737 amphibole has δD ≈ +3700‰; it absorbed Martian atmosphere‐derived heavy H in the aftermath of shock. Chassigny amphibole, with δD ≤ +1900‰, incorporated less heavy H. Low H 2 O/Cl ratios are inferred for the primitive chassignite magma, which had significant effects on melting and crystallization. Volatiles released by the degassing of Martian magma were more Cl‐rich than on Earth, resulting in the high Cl content of Martian surface materials.
BibTeX
@article{doi101111maps12430,
author = "Giesting, Paul A. and Schwenzer, S. P. and Filiberto, J. and Starkey, N. A. and Franchi, I. A. and Treiman, A. H. and Tindle, Andy and Grady, M. M.",
title = "Igneous and shock processes affecting chassignite amphibole evaluated using chlorine/water partitioning and hydrogen isotopes",
year = "2015",
journal = "Meteoritics and Planetary Science",
abstract = "Abstract Amphibole in chassignite melt inclusions provides valuable information about the volatile content of the original interstitial magma, but also shock and postshock processes. We have analyzed amphibole and other phases from NWA 2737 melt inclusions, and we evaluate these data along with published values to constrain the crystallization Cl and H 2 O content of phases in chassignite melt inclusions and the effects of shock on these amphibole grains. Using a model for the Cl/ OH exchange between amphibole and melt, we estimate primary crystallization OH contents of chassignite amphiboles. SIMS analysis shows that amphibole from NWA 2737 currently has 0.15 wt\% H 2 O. It has lost \textasciitilde 0.6 wt\% H 2 O from an initial 0.7–0.8 wt\% H 2 O due to intense shock. Chassigny amphibole had on average 0.3–0.4 wt\% H 2 O and suffered little net loss of H 2 O due to shock. NWA 2737 amphibole has δD ≈ +3700‰; it absorbed Martian atmosphere‐derived heavy H in the aftermath of shock. Chassigny amphibole, with δD ≤ +1900‰, incorporated less heavy H. Low H 2 O/Cl ratios are inferred for the primitive chassignite magma, which had significant effects on melting and crystallization. Volatiles released by the degassing of Martian magma were more Cl‐rich than on Earth, resulting in the high Cl content of Martian surface materials.",
url = "https://doi.org/10.1111/maps.12430",
doi = "10.1111/maps.12430",
openalex = "W2099044587",
references = "doi101007bf00306444, doi101007bf00310910, doi101007s0041000600854, doi1010160098300493900332, doi101093oxfordjournalspetrologya037267, doi101127ejm930623, doi101180minmag199706140513, doi102138am20124276, doi105860choice352126, openalexw2780726130"
}
11. Bacon, C., 2018, Presentation of the Dana Medal of the Mineralogical Society of America for 2017 to Thomas W. Sisson: American Mineralogist: v. 103, no. 4: p. 651-652.
DOI: 10.2138/AM-2018-AP10345 Source
BibTeX
@article{doi102138am2018ap10345,
author = "Bacon, C.",
title = "Presentation of the Dana Medal of the Mineralogical Society of America for 2017 to Thomas W. Sisson",
year = "2018",
journal = "American Mineralogist",
url = "https://pubs.geoscienceworld.org/ammin/article-pdf/103/4/651/4110633/am-2018-ap10345.pdf",
doi = "10.2138/AM-2018-AP10345",
is_oa = "true",
number = "4",
pages = "651-652",
semanticscholar_id = "720ed13aef8a51404ba2c6afa83e8975d603bb72",
volume = "103"
}
12. Marshall, C. and Fairbridge, R., 2019, Encyclopedia of Geochemistry: Elements.
DOI: 10.1007/978-3-319-39193-9 Source
BibTeX
@article{doi1010079783319391939,
author = "Marshall, C. and Fairbridge, R.",
title = "Encyclopedia of Geochemistry",
year = "2019",
journal = "Elements",
booktitle = "Encyclopedia of Earth Sciences Series",
url = "https://link.springer.com/content/pdf/bfm:978-1-4020-4496-0/1",
doi = "10.1007/978-3-319-39193-9",
is_oa = "true",
semanticscholar_citation_count = "82",
semanticscholar_id = "0bb66a022e4fec0e87016d124c1d76c1891cc1cd"
}
13. None, Igneous petrology: SpringerReference.
DOI: 10.1007/springerreference_5043
BibTeX
@misc{crossrefNoneigneous,
title = "Igneous petrology",
year = "None",
booktitle = "SpringerReference",
url = "https://doi.org/10.1007/springerreference\_5043",
doi = "10.1007/springerreference\_5043",
openalex = "W4255032728"
}