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the main reflector The overall effect on antenna performance is twofold: first the spill-over loss is reduced and second (and more important) the distribution of the energy on the antenna radiating aperture is made more uniform (as shown in the right-hand part of the figure) This means that the radiation efficiency of the main reflector (aperture efficiency), which is the dominant factor in the overall antenna efficiency, is improved The shape of the main reflector must also be modified in order to maintain a constant total path length (FA + AB + BD) of the rays all over the antenna (see Figure 79 b)), in accordance with the conventional laws of optics In terms of diffraction calculations, this is the condition for uniform phase distribution over the antenna aperture.

NOTE 1 The performance of Cassegrain antennas may be more or less impaired by the partial blockage and scattering caused by the sub-reflector and also by its supporting struts The main effects are: efficiency loss This loss can be reduced to some tenths of a decibel if the sub-reflector diameter is not greater than about 1/10 of the main reflector diameter The blocking effect can be reduced by application of the so-called "shaping technique" This technique allows a reduction of the energy directed from the sub-reflector to the central part of the main reflector (and also to the primary feed) The sub-reflector supporting struts also have the blocking effect, although the loss is lower than that of sub-reflector blockage.

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side lobe effects Direct radiation of the primary feed outside the sub-reflector diameter (so-called "sub-reflector spill-over" radiation) increases the side lobes of the antenna and must, therefore, be kept as small as possible The sub-reflector edge diffraction must also be combined with the spill-over radiation The sub-reflector struts are located in the field of two radiated waves One is the radiated power from the main reflector (plane wave) and the other is the radiated power from the sub-reflector (spherical wave) The both waves are scattered by the struts and degrade the side lobe NOTE 2 Cassegrain and Gregorian antennas exhibit a lower noise temperature than front-fed antennas This is due to the fact that the direct spill-over rays from the primary radiator are directed towards the sky, while they are directed more or less towards the ground in the case of front-fed antennas..

Transmit frequency Transmit polarization Transmit total output back-off Satellite e.i.r.p. in the direction of the receiving ES Transmit cross-polarization isolation Transmit frequency reuse isolation Satellite adjacent transponder isolation Transponder intermodulation C/I

A circular polarizer attaches to the lens, and you rotate it to reduce re ected polarized light. Maximum polarization occurs when the lens is at right angles (45 ) to the sun. With wide-angle lenses, uneven polarization can occur, causing part of the sky to be darker than other areas of the sky. Pass on the polarizer when making panoramic images as the unevenly toned sky it produces may be dif cult for the software to blend easily. Neutral density lters. Neutral density (ND) lters work like sunglasses for your camera. When photographing waterfalls, for example, even at your lowest ISO setting you can t use the slow shutter speed/aperture combination you d like to because there s way too much light. ND lters allow you to still get the shot by cutting the light transmission. They come in various strengths in 1/2 stop increments up to 8 stops to allow you to shoot longer exposures in bright environments.

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