Device for concentrating solar radiation with longitudinal mirrors and a longitudinal receiver

摘要

A device for concentrating solar radiation (4) with longitudinal mirrors (7) and a longitudinal receiver (1), has mirrors with a circular cross-section with a radius of curvature that is twice the transverse distance from the center (35) of each mirror to the central point (3) of the receiver. The width of the receiver is 1% of the transverse distance from the central point to the center (89) of the furthest mirror (32). The width of each mirror is determined according to the drift of the rays reflected when the mirror focuses the sun, prescribing an equal width for all mirrors, which is: equal to the width of the active face (2) of the receiver when mounted according to the meridian; and triple the width of the active face (2) of the receiver when mounted according to the parallel of latitude. The mirrors are installed in a contiguous manner and the receiver is installed at a height on columns (8).

主权项

1. Concentrating device for concentrating solar radiation, with longitudinal mirrors and a longitudinal receiver, based on a array of concave mirrors parallel to one another, having a longitudinal geometry, with a greater length than width, which can rotate about a longitudinal axis of symmetry, which in turn is an axis serving as support in bearings, which are placed on at intervals pillars which are buried in the ground and rigidly support the bearings, wherein the securing axis, which is a rotating shaft, is always fixed in a straight line position, each mirror being orientated by rotation for reflecting radiation towards a longitudinal parallelepiped solar receiver, the longitudinal axis of symmetry thereof located at a height H above the height of the axis of the mirror closest to the receiver as a result of columns or pillars supporting the receiver, with an active face where the receiver receives radiation reflected by the mirrors, the active surface having a transverse width R; the receiver containing internal elements absorbing solar radiation, said receiver having a longitudinal geometry and a greatest length parallel to the longitudinal axes of the mirrors, and having a transverse angle of inclination with respect to horizontal, wherein a final mirror is furthest from the receiver, two fields of mirrors being able to be assembled symmetrically with respect to two parallel receivers with active faces arranged opposite one another, each face pointing to a field in assemblies in which the longitudinal axes follow the local meridian, and being assembled both to the north and to the south of the receiver in cases in which the longitudinal axes of the mirrors are parallel to a local astronomical latitude, in which assemblies can also be two parallel receivers with the active faces arranged opposite one another, each face pointing to a field, the positions and angles being expressed in a coordinate system in a working plane used, which is a plane perpendicular to the longitudinal axes, and transversely and perpendicularly intersects the receiver and the mirrors, the position of the sun being projected on said working plane according to astronomical data, and a y-axis of the coordinate system in the working plane being a vertical line passing through a central or mid-point of a segment representing the active face of the receiver in the working plane, and an x-axis being a horizontal line passing through a central point of a segment which, in the working plane, represents the mirror closest to the receiver; selecting the value of the acute angle forming with a horizontal the line joining the central point of the furthest mirror of the field and the central point of the active surface of the receiver in a range of values between 10° and 80°, with a reference value of 45°; and the inclination of the active face of the receiver being determined, wherein the segment marking said surface in the working plane is perpendicular to the bisector of the field, said bisector being an angle formed with lines going, respectively, from the central point of the active face of the receiver to the central point of the closest mirror, and to the central point of the furthest mirror, the transverse width of the active surface or face of the receiver is 1% of the straight line distance between the central point of the furthest mirror of the field and the central point of the active surface of the receiver; and the mirrors are made of two different parts on each side of the central point of each mirror, both parts having a circular concavity, but with different radii of curvature, the latter radius being selected in a range of values between twice the distance from the central point of the mirror to the central point of the active surface of the receiver, and the radius value increased by 20%; the slope of the mirror being zero at a central point measured in an intrinsic coordinate system of each mirror, in which a y-axis is the normal at a central point and the reference position of the mirror coincides with a line joining said central point with the central point of the active face of the receiver; and in each of the mirrors, the central point of the specular surface coincides in the section with a longitudinal securing axis about which the mirror in question is rotated.