Alkali feldspars: ordering, composition and optical properties

dc.contributor.authorSu, Shu-Chunen
dc.contributor.committeecochairBloss, F. Donalden
dc.contributor.committeecochairRibbe, Paul H.en
dc.contributor.committeememberGibbs, Geralden
dc.contributor.committeememberStewart, David B.en
dc.contributor.committeememberWondratschek, Hansen
dc.contributor.departmentGeologyen
dc.date.accessioned2016-05-23T18:29:17Zen
dc.date.available2016-05-23T18:29:17Zen
dc.date.issued1986en
dc.description.abstractFor the entire alkali feldspar series, Σt₁ (total Al content in the T₁ sites, a quantitative measure of structural state or Al,Si long-range ordering) can be closely estimated from X<sub>Or</sub> (mole fraction of KAlSi₃O₈) and Y<sub>x</sub> (one half of the optic axial angle 2V<sub>x</sub>) by use of a simple determinative diagram based on the model Σt₁ = (b₀ + b₁X<sub>Or</sub> + b₂X<sub>Or</sub>sin²V<sub>x</sub> + b₃sin²V<sub>x</sub>) / (a₀ + a₁X<sub>Or</sub> + a₂X<sub>Or</sub>sin²V<sub>x</sub> + a₃sin²V<sub>x</sub>). Three sets of coefficients for this equation are required to account for three cases: (A) where X<sub>Or</sub> ≤ 0.6; (B) where X<sub>Or</sub> > 0.6 and O.A.P. (optical axial plane) ~ ⊥ (010); and (C) where X<sub>Or</sub> > 0.6 and O.A.P. = (010). They are (multiplied by 1000): <table style =”width:100%”> <tr><th>Case</th><th>a₀</th><th>a₁</th><th>a₂</th><th>a₃</th><th>b₀</th><th>b₁</th><th>b₂</th><th>b₃</th></tr> <tr><td>A</td><td>4.08</td><td>-2.35</td><td>0.95</td><td>-1.28</td><td>1.52</td><td>-0.18</td><td>-1.74</td><td>2.88</td></tr> <tr><td>B</td><td>1.69</td><td>1.63</td><td>-2.33</td><td>0.69</td><td>0.11</td><td>2.17</td><td>-2.70</td><td>3.46</td></tr> <tr><td>C</td><td>-1.69</td><td>-1.63</td><td>-0.70</td><td>2.38</td><td>-0.11</td><td>-2.17</td><td>-0.53</td><td>3.57</td></tr> </table> Tested by the data from 109 alkali feldspars in the literature and the author's experiments, this model estimates Σt₁ (given X<sub>Or</sub> and V<sub>x</sub>) with a standard error of 0.02, which is essentially the same as when Σt₁ is estimated from refined lattice parameters determined by X-ray diffraction methods. The model was developed by assuming that the principal refractive indices for sodium light - symbolized as n<sub>a</sub>, n<sub>b</sub>, and n<sub>c</sub> dependent upon whether the corresponding principal vibration axis was parallel or most nearly parallel to crystallographic axes a, b and c - varied linearly with Σt₁ for the high-sanidine to low-microcline series and for the low albite to high albite (or analbite) series. However, for the high albite to high sanidine solid solution series, as well as the low albite to low microcline series, neither density nor principal refractive indices vary linearly across the entire composition range, but they closely approached linearity between 0.0 ≤ X<sub>Or</sub> < 0.6 and 0.6 < X<sub>Or</sub> ≤ 1.0.en
dc.description.degreePh. D.en
dc.format.extentxi, 128 leavesen
dc.format.mimetypeapplication/pdfen
dc.identifier.urihttp://hdl.handle.net/10919/71274en
dc.language.isoen_USen
dc.publisherVirginia Polytechnic Institute and State Universityen
dc.relation.isformatofOCLC# 15048204en
dc.rightsIn Copyrighten
dc.rights.urihttp://rightsstatements.org/vocab/InC/1.0/en
dc.subject.lccLD5655.V856 1986.S9en
dc.subject.lcshFeldsparen
dc.titleAlkali feldspars: ordering, composition and optical propertiesen
dc.typeDissertationen
dc.type.dcmitypeTexten
thesis.degree.disciplineGeologyen
thesis.degree.grantorVirginia Polytechnic Institute and State Universityen
thesis.degree.leveldoctoralen
thesis.degree.namePh. D.en

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