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Milky white knot SMZ 20X.jpg

Why make thin-sections?

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Example #1: "Aluminous stone" in-glass, PLM 100X

Stone is too dense and opaque to see anything of value to help determine crystalline phase(s) composition and its source material.

Mullite brick stone in-glass PLM 100X_edited.jpg

Example #1: "Aluminous stone" after thin-sectioning, PLM 225X

At higher magnifications the Tabular Alumina, secondary a-Al2O3, B-Al2O3 and Nepheline phases are visible.  The stone is from an alumina fortified Mullite or Sillimanite class brick.

Mullite brick stone thin-sectioned 225X_edited.jpg

Example #2: "Silica type stone" in-glass, PLM 100X

Stone is really too thick to be properly identified in-glass even though you can discern some Tridymite laths at the thinner edges or ends of the stone.

Silica brick stone in-glass PLM 100X_edited.jpg

Example #1: "Aluminous stone" after thin-sectioning, PLM 100X

Crystalline morphology and phase(s) can begin to be identified at low magnifications.

Mullite brick stone thin-sectioned PLM 100X_edited.jpg

Example #2: "Silica type stone" in-glass, Stereo-zoom microscope (SMZ) 50X

Stone is translucent white, "lumpy" and includes small outgassing bubbles which serves to indicate it most likely has a siliceous composition

Silica brick stone in-glass SMZ-50X_edited.jpg

Example #2: "Silica type stone" after thin-sectioning, PLM 100X

It is now easy to identify the stone is composed entirely of secondary Tridymite laths and thus originated from silica refractory brick in the colder, front end of the refiner at temperatures < 1470C inversion to Cristobalite.

Silica brick stone thin-sectioned PLM 100Xb_edited.jpg
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