Solar control coated glass
AssigneeAtofina Chemicals, Inc.
InventorsDavid A. Russo, Clem S. McKown, Christophe Roger, Jeffrey L. Stricker
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AssigneeAtofina Chemicals, Inc.
InventorsDavid A. Russo, Clem S. McKown, Christophe Roger, Jeffrey L. Stricker
Estimating the term…
A solar-control glass that has acceptable visible light transmission, absorbs near infrared wavelength light (NIR) and reflects midrange infrared light (low emissivity mid IR) along with a preselected color within the visible light spectrum for reflected light is provided. Also provided is a method of producing the improved, coated, solar-controlled glass. The improved glass has a solar energy (NIR) absorbing layer comprising tin oxide having a dopant such as antimony and a low emissivity control layer (low emissivity) capable of reflecting midrange infrared light and comprising tin oxide having fluorine and/or phosphorus dopant. A separate iridescence color suppressing layer as described in the prior art is generally not needed to achieve a neutral (colorless) appearance for the coated glass, however an iridescence suppressing layer or other layers may be combined with the two layer assemblage provided by the present invention. If desired, multiple solar control and/or multiple low emissivity layers can be utilized. The NIR layer and the low emissivity layer can be separate portions of a single tin oxide film since both layers are composed of doped tin oxide. A method of producing the coated solar control glass is also provided.
A method of producing a tin oxide coated, solar control glass having low haze of less than about 2.0% and having a NIR solar absorbing layer and a low emissivity layer within said tin oxide coating, comprising a glass substrate and a doped tin oxide coating having at least two layers with one layer being a solar absorbing layer comprising SnO2 containing a dopant selected from the group consisting of antimony, tungsten, vanadium, iron, chromium, molybdenum, niobium, cobalt, nickel and mixtures thereof and another layer being a low emissivity layer comprising SnO2 containing a dopant of fluorine or phosphorus and, wherein a portion of said solar absorbing layer contains fluorine in sufficient quantity to reduce the rugosity and haze for said tin oxide coating and wherein the thickness of the NIR solar absorbing layer is from 200 to 320 nanometers (nm) and the thickness of the low emissivity layer is from 200 to 450 nm and the portion of said solar absorbing layer containing fluorine to reduce the rugosity comprises from 300 Angstroms (Å) to 600 Å of the thickness of the solar absorbing layer and is located either adjacent to the interface between the solar absorbing layer and the low emissivity layer, or is the portion of the solar absorbing layer that is closest to the glass substrate, comprising sequentially treating glass at a temperature above 400° C. with:
A method of producing a tin oxide coated, solar control glass having low haze of less than about 2.0% and having a NIR solar absorbing layer and a low emissivity layer within said tin oxide coating, comprising a glass substrate and a doped tin oxide coating having at least two layers with one layer being a solar absorbing layer comprising SnO2 containing a dopant selected from the group consisting of antimony, tungsten, vanadium, iron, chromium, molybdenum, niobium, cobalt, nickel and mixtures thereof and another layer being a low emissivity layer comprising SnO2 containing a dopant of fluorine or phosphorus and, wherein a portion of said solar absorbing layer contains fluorine in sufficient quantity to reduce the rugosity and haze for said tin oxide coating and wherein the thickness of the NIR solar absorbing layer is from 200 to 320 nanometers (nm) and the thickness of the low emissivity layer is from 200 to 450 nm and the portion of said solar absorbing layer containing fluorine to reduce the rugosity comprises from 300 Angstroms (Å) to 600 Å of the thickness of the solar absorbing layer and is located either adjacent to the interface between the solar absorbing layer and the low emissivity layer, or is the portion of the solar absorbing layer that is closest to the glass substrate, comprising sequentially treating glass at a temperature above 400° C. with:
Dependencies are inferred from the claim text.