1,725,018 research outputs found
Santa Fe (ATSF) 3164
No full textA photograph print showing the Santa Fe (ATSF) 3164, 2-8-2, South Shawnee, OK. (hostler M.L. Reed in cab
Recipes (SC 3164)
Get PDFFinding aid only for Manuscripts Small Collection 3164. Handwritten recipes, mostly for cakes and frosting. Includes typescripted recipes for cookies and pastry using Pan American Mills products
Santa Fe (ATSF) 3164
No full textA photograph print showing Santa Fe (ATSF) 3164, 2-8-2, (BLW) class 3160, So. Shawnee, OK. Back of photo lists loco's specifications
Santa Fe (ATSF) 3164
No full textA photograph postcard (& Negative) showing Santa Fe (ATSF) 3164, 2-8-2, northbound through Big Canyon near Arbuckle, OK. 35 cars
Rowen, J A, 1/3164
No full textThis record was harvested from a previous catalogue system and will be withdrawn in 2025. Information in this record may be superseded or incomplete. Visit this record in UMA's new catalogue at: https://archives.library.unimelb.edu.au/nodes/view/428309Surname: Rowen. Given Name(s) or Initials: J A. Military Service Number or Last Known Location: 1/3164. Prisoner of War Enquiry Card Index Number: M/717. Division Enquiry: Malaya. Rank: CPL. Unit: Malaya327065
Item: [2016.0049.60571] "Rowen, J A, 1/3164
Metamorphic angrite Northwest Africa 3164/5167 compared to magmatic angrites
No full textInternational audienceNorthwest Africa (NWA) 3164 and 5167 are two angrites with a granulitic texture unlike that of other angrites, with avariable, up to millimeter grain size. Besides mineralogical and chemical similarities to other angrites, NWA 3164 and5167 exhibit unique characteristics. Ca-rich olivine dominates (in NWA 3164: 49 vol%, Fo57; NWA 5167: 40 vol%,Fo59). Fassaitic clinopyroxene is the second major phase (in NWA 3164: 29 vol%; in NWA 5167: 36 vol%) with a significantTschermak component. In addition, two Al-rich phases are present: plagioclase An99 and hercynitic spinel (6 and 7 vol%respectively for NWA 3164; 17 and 4 vol% respectively for NWA 5167). Heavily weathered iron sulfide and kamacite, (9 wt%in NWA 3164; 4 wt% in NWA 5167) are the remaining minor phases, a unique feature among angrites. All mineral phases arehomogeneous. Like other angrites, NWA 3164 and 5167 exhibit a superchondritic Ca/Al ratio, with negligible amounts ofalkalis and very low silica content. The presence of metal results from the incorporation of exogenous iron following impact.Subsequent annealing resulted in the observed granulitic texture. Major element composition indicates that both NWA 3164and 5167 are derived from a picritic angrite precursor after incorporation of metal and annealing.After correction for iron and Fo90 olivine incorporation, bulk rock REE abundances of both NWA 3164 and NWA 5167appear lower than those of quenched angrites, showing the lowest absolute abundances among angrites. Laser ablation inductivelycoupled plasma mass spectrometry (LA-ICP-MS) analyses of clinopyroxene, olivine and anorthite indicate that differenceof Rare Earth Element (REE) abundances between NWA 3164 and NWA 5167 can be explained by adding traces ofphosphate to NWA 3164. NWA 3164/5167 trace elements abundances are similar, showing depletion in volatile elementsand enrichment in refractory lithophile elements such as Ca, Ti, and Al. The most incompatible elements are depleted as well,unlike other angrites. This indicates that the source of these younger angrites was more depleted in incompatible elementswhen compared to the older magmatic angrites. The low Hf/W is understood as the result of exogenous iron incorporationand therefore the Hf/W andWisotopic heterogeneity of the angrite parent body (APB) mantle is secondary. Comparison withother angrites suggests that iron incorporation may be necessary to explain their low Hf/W and W isotopic compositions
Block Card 3164 Escott Avenue
No full textThis image was produced by the Auditor's Office in Lucas County, Ohio for tax assessment purposes. Associated dates are approximate. Descriptive terms related to this photograph include: Ranch houses | 3164 Escott Avenue (Toledo, Ohio) | Dwelling | Windy Hill Addition (Toledo, Ohio) | South Toledo Area (Toledo, Ohio
3164. Pour les papes d'Avignon, voir plus loin l'histoire étrangère
No full text3164. Pour les papes d'Avignon, voir plus loin l'histoire étrangère. In: Molinier Auguste. Les Sources de l'histoire de France - Des origines aux guerres d'Italie (1494). IV. Les Valois, 1328-1461. Paris : A. Picard et fils, 1904. p. 39
Classroom Management
No full textAbstract: This paper will cover everything an instructor ever wanted to know about classroom management and will cover a selection of different subjects. Some areas will include building culture, setting guidelines and anticipations, providing outcomes, and controlling classroom trouble. We will begin by identifying the instructor’s role in classroom management.
Keywords: management, instructor, procedures, consequences, disruptions, routines, behaviour.
Title: Classroom Management
Author: NAELA ABDULLAH TAMI
International Journal of Social Science and Humanities Research
ISSN 2348-3156 (Print), ISSN 2348-3164 (online)
Vol. 10, Issue 2, April 2022 - June 2022
Page No: 269-274
Research Publish Journals
Website: www.researchpublish.com
Published Date: 20-May-2022
DOI: https://doi.org/10.5281/zenodo.6567025
Paper Download Link (Source):
https://www.researchpublish.com/papers/classroom-managementInternational Journal of Social Science and Humanities Research, ISSN 2348-3156 (Print), ISSN 2348-3164 (online),
Research Publish Journals, Website: www.researchpublish.co
Comet West (1978a)
No full textpeer reviewedIAUC 3164 available at Central Bureau for Astronomical Telegrams
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