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Misinterpretation of multipass interferograms can also result from misalignment of the stop in the focal plane. If this stop accidentally cuts off low spatial frequencies in the image, strong diffraction effects are observed, as in the Foucault test. Applications where multipass interferometry is useful include measurements of the homogeneity of glass plates and the precise determination of 90 or 45 angles on roof prisms and cube corners, where high accuracy is required (Langenbeck, 1969b). Another interesting application is in grazing incidence interferometry. Grazing incidence interferometry (Linnik, 1941; Saunders and Gross, 1959) makes it possible to test large surfaces with a system of relatively small aperture. In addition, it is possible to test many nonoptical surfaces, such as ne-ground glass and metal, from which a specular re ection of adequate intensity can be obtained at low angles of incidence (Birch, 1973; Hariharan, 1975; Murty, 1976). With incidence at an angle a, a beam of diameter d covers a strip of length L d cos a 7:8

are dropping, and (2) many sponsors are eager to defray the start-up costs in exchange for some tasteful recognition. Online special events and campaigns are natural ways to engage an existing or new corporate sponsor or supportive philanthropist. Online special events and campaigns appeal to sponsors for a variety of reasons, but four reasons stand out in particular: 1. It s a great naming or branding opportunity to put a logo in the header or footer of each Web page since the online special event or campaign site will be touched by hundreds or thousands of people. 2. It appeals to many sponsors desire to help the charity become more efficient in fundraising. 3. It has a unique ability to provide back to the sponsor deep statistics and reports regarding the adoption of the technology (how many visits, when, how long, etc.), which sponsors love! 4. It still has a sizzle factor. For many corporate sponsors their interest goes beyond doing the right thing for their community and presenting a positive public image for their customers: It is their employee base that is their focus. Corporations are searching for ways to motivate and retain talented staff, and have long realized that philanthropy is an important activity for this. Online special events and campaign tools provide greater ability for a corporation to engage and measure the activity of an employee base. (See Exhibit 15.15.) Today s online applications can allow teams of employees from HR to challenge those in finance. Some corporations have a separate point of entry to the online application for employees only. And the reporting produced from the applications can allow senior management to see which employees took on leadership roles within the charitable activity.

The manager soon realizes that this matchLog table is going to be huge after everyone on the team has played an entire season s worth of games. As you can see, the structure of the table is inefficient because each player s details number, name, phone number, and so on are entered every time he plays a match.

For most of history, astronomers have had to rely on light in the visible part of the spectrum in order to study the Universe One of the great astronomical achievements of the 20th century was the exploitation of the full electromagnetic spectrum for astronomical measurements We now have instruments capable of making observations of radio waves, microwaves, infrared light, visible light, ultraviolet light, X-rays and gamma rays, which all correspond to light waves of different (in this case increasing) frequency We are even entering an epoch where we can go beyond the electromagnetic spectrum and receive information of other types A remarkable feature of observations of a nearby supernova in 1987 was that it was also seen through detection of neutrinos, an extraordinarily weakly interacting type of particle normally associated with radioactive decay.

Very high energy cosmic rays, consisting of highly-relativistic elementary particles, are now routinely detected, though as yet there is no clear understanding of their astronomical origin And as I write, experiments are starting up with the aim of detecting gravitational waves, ripples in space-time itself, and ultimately of using them to observe astronomical events such as colliding stars The advent of large ground-based and satellite-based telescopes operating in all parts of the electromagnetic spectrum has revolutionized our picture of the Universe While there are probably gaps in our knowledge, some of which may be important for all we know, we do seem to have a consistent picture, based on the cosmological principle, of how material is distributed in the Universe My discussion here is brief; for a much more detailed discussion of the observed Universe, see Rowan-Robinson's book 'Cosmology' (full reference in the Bibliography).