A better understanding of the invention will be had with reference to the accompanying drawings wherein;
This invention can be configured in several ways depending on the deployment environment. The basic system as shown in
Antennas are typically mounted on some type of adjustable bracket 14, see
Each of the brackets 14 shown includes a pair of clamp members 20 and 21 that are mounted in opposing relationship to one another on opposite sides of one of the pole segments 24 and are secured to one another by adjustable bolts 27. The number of brackets for mounting each antenna may vary from one to any number, however, as shown, two brackets are used to mount the antennas to the pole segments. Each bracket also includes a generally u-shaped member 28 that is secured to the backplane 29 of one of the antennas and which is pivotally connected at spaced points 30 to upper portions of a frame member 31 that is pivotally connected at 33 to spaced lower portions of a second frame member 34 that is pivotally adjustable at points 35 to the clamp member 21. Appropriate fasteners, not shown, are used at each of the pivot points to lock the two frame members in an adjusted position relative to one another in order to retain the mounted antenna in a predetermined and properly aligned position relative to the service area surrounding the tower. By adjusting the angled relationship between the frame portions of each bracket and the clamping members, an appropriate tilt angle may be obtained.
The sensors 10 are also mounted to the backplanes 29 of the antennas by generally L-shaped brackets 36. As shown in
Collection of data can be done at each sensor or at a remote central location. The preferred method is to have one data collection unit 13 for each site having multiple antennas, with the data collection unit accessible at the base of the tower or in an easily accessible control cabinet or room (not shown). Cables 17 or wireless data transmission devices (not shown) connect the sensors to the data collection unit 13. Data reduction and processing can also be done at each sensor 10 as opposed to a remote location of the data collection unit shown in the drawing figures. It is also possible to have the data processing unit include a portable device, such as a standard computer 15, as shown in
As shown, the alignment sensors are designed to be permanently installed atop of, or otherwise secured relative to, the directional antennas. The sensors can be made using one or a combination of the several ways described herein. The first category of alignment monitoring sensor 10A uses the sun to determine both azimuth and inclination. This is accomplished in one of two main ways. The first way, as shown in
The sensor coded aperture mask 19 and CCD 18 can be arranged in several ways, the preferred orientation is with the coded aperture mask 19 in a cylindrical arrangement with a vertical axis “A” and the CCD 18 centered on this axis in a horizontal plane below the shadow mask. The CCD 18 and mask 19 will be arranged to view the sun from about 10 to 60 degrees above the horizontal, and 360 degrees around in azimuth. Alternate versions of this sensor can use the same cylindrical mask with one or more CCD's 18 arranged either vertically as shown in
Another variation on the all solar permanently installed alignment monitoring sensor 10B uses a phototransistors or group of phototransistors 42 as solar sensors mounted within a housing 43, see
One phototransistor per slit can be used, or multiple slits can illuminate the same phototransistors, as the times each slit will be illuminated are spaced far enough to not be mistaken. Also, several phototransistors can be aligned below each slit, as is shown in
The housing 43 is mounted atop each antenna to be monitored to be adjustable around the vertical axis, by being secured to an L-shaped bracket, such as 36, as previously described. For this type of sensor, a method of relating the view position of the sensor back to the azimuth direction of the antenna is required. The preferred method is to mount the sensor 10B on the leg 37 of the bracket 36 with the surface of the leg being exactly horizontal when the antenna is correctly leveled, with a central bolt or pin, not shown, about which the sensor can rotate about the vertical axis “B”. To retain the housing in a proper position, a set of equally spaced holes, not shown, are provided on the leg 37 of the sensor mounting bracket 36 into which one or more pins, not shown, on the bottom of the sensor can selectively engage. This forces the sensor to be in one of a number of accepted clocking positions with respect to the antenna. A magnet carried by the mounting bracket 36 may be sensed by one of a circular array of hall effect switches, or reed switches, not shown, arranged around the base of the sensor. Alternately, a fixed pin, not shown, on the mounting bracket 36 can be configured to penetrate one of an array of equally spaced holes, not shown, in the sensor housing 43 base where is it sensed by one of a circular array of optical switches or inductive proximity switches, not shown.
These arrayed sensors relate the azimuth position of the sensor to the position of the antenna. In some instances an engraved degree wheel, not shown, on the bracket 36 can be used as an indicator by a pointer fixed to the sensor housing 43 and the position noted and inputted to the central data collection and processing unit 13. The sensor body is aligned in azimuth to point the slits 44 toward the intended solar track or transverse. For example, a sensor using both morning and afternoon slits would have the slits aligned so that a plane midway between the slits views or faces exactly south. Morning alone slits 44 must be pointed roughly south east, and afternoon alone slits 44′ pointed roughly southwest, depending on latitude. These view directions are to allow installation where the structure of the antenna tower 16 or other support may block some views of the sun. The sensor 10B will not work in a location that is shaded from a direct view of the sun. Measuring of the time of the solar transverse of each slit relative to the known direction of the slits and date, time and location gives precise pointing information of the sensor, in tilt (2 axes) and heading. This is done by comparison of the actual solar transverse time to the expected time from a solar transverse equation and converting the vector to the correct position in the central data collection and processing unit 13.
A third embodiment of a permanently installed solar alignment monitoring sensor 10C is shown in
The sun will cast a shadow of the post 56 across the ring of sensors or phototransistors, allowing them to sense the sun azimuth position. This can be done using wide acceptance angle sensors directly, or by placing a cover 60 over the ring of sensors 54 with the cover including a refracting lens 62 positioned above the sensors which accepts sunlight at lower sun angles and refracts the lower incidence sun rays downward into the sensors at a proper acceptance angle. Also, the upward angle can be increased by the same method.
An example of a combination sealed cover and refracting lens 60 is shown in
Level sensing in the current embodiment may be handled instantly by either a pair of electronic level sensors using a pendulum (not shown) or by a pair of solid state accelerometers 52. In either case, the instruments are placed orthogonally with one axis aligned with down tilt angle of the antenna. It should be noted that the electronic lever sensors 52 may be of any convention structure such that level readings may be transmitted directly or indirectly to the data collection and processing unit 13.
The sensor 10C has two distinct advantages to the sensor 10B discussed above. First, it can be installed in any azimuth orientation, making alignment to the antenna much simpler, as it will be fixed to the antenna in one orientation regardless of the antenna's installed direction (N, S, E or W). Second, the level information is available to the installed real time, and may be used to assist with antenna alignment during installation regardless of weather conditions. Level information from all the sensors gives information in two axes, down tilt, along the antenna's preferential radiation direction, and roll, perpendicular to the antenna's preferential radiation direction. Down tilt is the most important parameter to an antenna's performance, but roll information is also important, because the antenna's mapped radiation pattern assumes that the antenna is mounted level in roll.
It should be noted that the sensors 10A and 10B describe herein could also be fitted with electronic level sensors to gain the advantages stated above. It should also be noted that other solar sensing devices may be used with or in place of the CCD devices and phototransistors mentioned in the described embodiments.
The foregoing description of the present invention has been presented to illustrate the principles of the invention and not to limit the invention to the particular embodiments illustrated. It is intended that the scope of the invention be defined by all of the embodiments encompassed within the following claims and their equivalents.
Number | Date | Country | |
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60817415 | Jun 2006 | US |