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Choose a precision (the number of decimal points or the fraction denominator) from the Precision drop-down list. Choose a fraction format from the Fraction Format drop-down list. This option is available only if the format that you chose uses fractions. Horizontal places a horizontal line between stacked numerators and denominators. Diagonal uses a diagonal slash between the stacked numerator and denominator. Not Stacked uses a diagonal line between the numerator and denominator, which are not stacked. You can see the effect of each choice in the preview box. Choose a decimal separator. This option is available only if the format that you chose uses decimals. You can choose from a period, a comma, and a space. Use the Round Off text box to round off linear dimension distances. For example, you can round to the nearest 0.1 unit or 1 2 inch.

However the LSP is not the only option for particle dark matter, and other proposed particles include an ultra-light particle known as the axion, ultra-heavy dark matter particles which might for instance be formed at the end of inflation, or particles from a 'shadow Universe' which interacts with our own Universe only gravitationally.

, 57 (1947); reprinted in Amateur Telescope Making, vol 3, A E Ingalls, Ed, Scienti c American, New York, 1953 Fienup J R and C C Wackermann, Phase-retrieval Stagnation Problems and Solutions, J Opt Soc Am A, 3, 1897-1907 (1986) Gershberg R W and W O Saxton, A Practical Algorithm for the Determination of Phase from Image and Diffraction Plane Pictures, Optik, 35, 237 (1972) Gershberg R W, Super-Resolution Through Error Energy Reduction, Optica Acta, 21, 709 720 (1974) Hardy J W, J E Lefevre and C L Koliopoulos, Real-time Atmospheric Compensation, J Opt Soc Am, 67, 360-369 (1977) Hudgin R H, Wave-front Reconstruction of Phase Values from Phase Differences, J Opt Soc Am, 67, 375-378, 1977 Ichikawa K, A W Lohmann, and M Takeda, Phase Retrieval Based on the Irradiance Transport Equation and the Fourier Transport Method: Experiments, Appl Opt.

To add a new scale, click Add. In the Add Scale dialog box, name the scale. The name is what will show on the list. You can use existing scales as a guide. Then define the scale by completing the Paper Units and Drawing Units text boxes. For example, to add a 1:12 scale, you would name the scale 1:12, set the Paper Units to 1 and the Drawing Units to 12. To delete scales that you don t use, select the scale and click Delete. You can also edit existing scales (select the scale and click Edit), move them up or down in the order of the list, and reset the list (click Reset) to its original status. Click OK when you re done.

There will be more expertise available in managing the data warehouse volumes of data. Hardware costs will have dropped to some extent. More powerful software tools will be available. The end user will be more sophisticated.

Figure 1.1: Maximum emission in the UNII band LANs (IEEE 802.11) introduces mobility and flexibility to a LAN environment by allowing computers and other devices to communicate with one another wirelessly (URL: H t t p : //grouper.ieee. org/groups/802/11/). This technology is beneficial for improved access to fixed LAN and inter-network infrastructure (including access to other wireless LANs) via a network of access points, as well as creation of higher performance ad hoc networks. The two wireless LAN solutions that utilize OFDM are the 802.11g and the 802.11a. The IEEE s 802.11g standard is designed as a higher-bandwidth (54 Mbps) successor to the popular 802.11b, or the Wi-Fi standard (11 Mbps). While 802.11g is backwards compatible with 802.11b at the 2.4GHz ISM (industrial, scientific & medical) band, the 802.11a operates in the newly allocated UNII band (Unlicensed National Information Infrastructure). Figure 1.1 shows the channel plan and the associated maximum emission of the UNII band. Because of the power limitation, most applications of wireless LAN are limited to homes and office buildings. The basic requirements of wireless LAN include

, 27, 3433 3436 (1988) Kingslake R, A New Bench for Testing Photographic Lenses, J Opt Soc Am, 22, 207 222 (1932) Kogelnik H and T Li, Laser Beams and Resonators, Appl Opt, 5, 1550 1567 (1966) Leistner K, B Marcus, and B W Wheeler, Lens Testing Bench, J Opt Soc Am, 43, 44 (1953) Li Y and E Wolf, Three-Dimensional Intensity Distribution Near Focus in Systems of Different Fresnel Numbers, J Opt Soc Am A, l, 801 808 (1984) Linfoot E H and E Wolf, On Telescopic Star Images, Mon Not Ry Astron Soc, 112, 452 (1952)..