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1 Introduction and History nel, Paris See pp 255 623: Th orie de la Lumii re Quatri me Section Double R fraction [10] Gehrels, T (1960) Measurements of the wavelength dependence of polarization Lowell Observatory Bulletin No105, Vol IV No17, 300 301 [18] Gehrels, T (1974) (Ed) Planets, Stars and Nebulae studied with Photopolarimetry University of Arizona, Tucson, AZ [26] Gehrels, T, Teska, TM (1963) The wavelength dependence of polarization Appl Opt, 2, 67 77 [20] Grant, R (1852) p 313 in History of Physical Astronomy, Henry G Bohn, London [16] Grigoryan, K A (1958) Polarization observations of Cephei Soob Byurakan Obs, 25, 45 48 [21] Haidinger, W (1844) Ueber das directe Erkennen des polarisirten Lichts und der Lage der Polarisationsebene Ann Phys, 139 (9), 29 39 [15] Hall, JS (1948) A photoelectric polarimeter AJ, 54, 39 [18] Hall, JS (1949) Observations of the polarized light from stars Science, 109, 166 167 [18] Hall, JS, Mikesell, AH (1950) Polarization of the light in the galaxy as determined from observations of 551 early-type stars Publications of the US Naval Observatory Second Series Vol XVII Part I, Washington [18, 20] Hall, JS (1958) Polarization of Starlight in the Galaxy Publications of the US Naval Observatory Second Series Vol XVII Part VI, Washington [18] Herschel, JFW (1869) Outlines of Astronomy Longmans, Green, London [15] Hiltner, WA (1947) On the presence of polarization in the continuous radiation of early-type stars ApJ, 106, 231 234 [17] Hiltner, WA (1949a) Polarization of light from distant stars by interstellar medium Science, 109, 165 [18] Hiltner, WA (1949b) On the presence of polarization in the continuous radiation of stars II ApJ, 109, 471 478 [18] Hiltner, WA (1951) Polarization of stellar radiation III The polarization of 841 stars ApJ, 114, 241 271 [18] Hiltner, WA (1954) Interstellar polarization of 405 stars ApJ, 120, 454 463 [18] Hooke, R (1665) Micrographia Some Physiological Descriptions of Minute Bodies Made by Magnifying Glasses with Observations and Inquiries Thereupon Pub under the auspices of The Royal Society, London [11] Huard, S (1997) Polarization of Light John Wiley & Sons Chichester, West Sussex [26] Huyghens, C (1690) Trait de la Lumi re Leyden Relevant excerpts can be found in Swindell (1975) [3] Janssen, EM (1946) On the polarization of the continuous radiation of early-type stars ApJ, 103, 380 [17] Jenkins, FA, White, HE (1965) Fundamentals of Optics 3rd Edition, McGraw-Hill, New York [23] Kahr, B, Claborn, K (2008) The lives of Malus and his bicentennial law ChemPhysChem, 9, 43 58 [4] Kemp, JC (1970a) Quantum magnetic features in the polarized light of Grw C70 8247 ApJ, 162, L69 L72 [22] Kemp, JC (1970b) Circular polarization of thermal radiation in a magnetic eld ApJ, 162, 169 179 [22] Kemp, JC, Barbour, MS (1981) A hotoelectric polarimeter at Pine Mountain Observatory PASP, 93, 521 525 [22] Kemp, JC, Wolstencroft, RD (1972) Interstellar circular polarization: data for six stars and the wavelength dependence ApJ, 176, L115 L118 [22] K nnen, GP (1985) Polarized Light in Nature Cambridge University Press, Cambridge [26] Kopal, Z, Shapley, MB (1946) A study of the extended envelope surrounding the Wolf Rayet component of V444 Cygni ApJ, 104, 160 176 [17] Kuhn, W, Braun, E (1929) Photochemische erzeugung optisch aktiver stoffe Naturwiss, 17, 227 228 [24] Landstreet, JD (1980) The measurement of magnetic elds in stars AJ, 85, 611 620 [22] Leroy, J-L (1995) Linear polarimetry of Ap stars V A general catalogue of measurements A&AS, 114, 79 104 [22] Leroy, J-L (1998) La polarisation de la lumi re et l observation astronomique Gordon & Breach, Amsterdam [26].

All DBMSs except Oracle use similar numeric formats, so look for our Oracle-specific recommendations only if you use Oracle Any number with a scale of zero (no digits after the decimal point) should be in an INTEGER column INTEGER is the default data type of any literal that contains all digits SMALLINT is the only other SQL Standard data type and is usually just half the size of INTEGER TINYINT is the smallest integer data type and is still large enough for most personal information BIGINT is appropriate for numbers larger than two billion though working with compilers that can't handle such large numbers could be problematic Floating-point operations are fast if they go through the computer's FPU When you install a DBMS, the installer should detect the FPU automatically and bring in the right code, whether FPU dependent or emulated, so make sure you rerun the install program after ardware upgrades The primary advantage of DECIMAL is that it is easy to cast to CHAR, because the number isn't stored in binary form The primary disadvantage of DECIMAL is that it must be converted to binary form before some arithmetic operations can be performed on it Serial data types are useful for ensuring each row of a table has a unique identifier The problem with serials is that they can cause trouble with concurrency control Recommendation if you don't use Oracle: Prefer INTEGER for integers unless maximum values including those from arithmetic operations exceed the INTEGER range Prefer DECIMAL for fixeddecimal numbers and for most floats Prefer DOUBLE PRECISION for floats where DECIMAL isn't appropriate Prefer INTEGER for serials and do your own value assignments Recommendation if you use Oracle: Data type doesn't really matter because all numbers are stored the same Avoid multiply and divide because the packed decimal numbers will have to be converted before they can be operated on Allow free space on each page because rows are all variable-length Don't worry about floating-point storage because it's not there.

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1 Introduction and History Parsons, W (1878) (The 3rd Earl of Rosse) Preliminary Note on Some Measurements of the Polarization of the Light coming from the Moon and from the Planet Venus Sci Proc R Soc Dublin, 1, 19 20 [16] Pye, D (2001) Polarised Light in Science & Nature Institute of Physics Publishing, Bristol [26] Schwarz, H E (1984) Spectropolarimetry of cool giants and supergiants PhD Thesis, Department of Astronomy, University of Glasgow [20] Secchi, A (1860) Letter from the ev Father Secchi to the Astronomer Royal MNRAS, 20 70 71 [16] Semel, M (2003) Spectropolarimetry and polarization-dependent fringes A&A, 401, 1 14 [11] Serkowski, K (1970) Intrinsic polarization of early-type stars with extended atmospheres ApJ, 160, 1083 1105 [21] Serkowski, K (1971) Polarization of variable stars pp 11 31 in New Directions and New Frontiers in Variable Star Research, IAU Colloquium No 15, Bamberg [20, 21] Serkowski, K (1973) Interstellar polarization pp 145 152 in Interstellar Dust and Related Topics IAU Symp No 52 (eds JM Greenberg and HC van de Hulst) Dordtecht, The Netherlands [20] Shakhovskoi, NM (1963) Polarization observations of Lyrae Sov Astron, 6, 587 589 [21] Shakhovskoi, NM (1965) Polarization in variable stars II Eclipsing binaries Sov Astron, 8, 833 842 [21] Shakhovskoi, NM (1969) The spatial orientation of the orbit planes of close binary stars Sov Astron, 13, 303 305 [21] Shulov, OS (1967) Polarimetric observations of close binary stars Trudy Astron Obs Leningrad, 24, 38 53 [21] Shurcliff, WA (1962) Polarized Light Harvard University Press, Harvard [26] Sten o, JO (1996) Scattering physics Sol Phys, 164, 1 20 [16] Sten o, JO, Keller, CU (1997) The second solar spectrum A new window for diagnostics of the Sun A&A, 321, 927 934 [16] Struve, O, Zebergs, V (1962) pp 368 372 in Astronomy of the 20th Century MacMillan, New York [17] Swindell, W (1975) Polarized Light Benchmark Papers in Optics/1 Dowden, Hutchinson & Ross, Stroudsburg, PA, USA [3, 26] Tapia, S (1977) Discovery of a magnetic compact star in the AM Herculis/3U 1809+50 System ApJ, 212, L125 L129 [22] Thiemann, W (1975) Life and Chirality Beyond The Earth Origins of Life, 6, 475 481 [25] Thiessen, G (1961) ber die Polarisation des Sternlichtes, die Strahlung der Sterne, Sowie Bemerkungen zur Galaktiscehn Struktur Astr Abh Hamburg Stern, Vol V, No 9 [21] Tinbergen, J (1996) Astronomical Polarimetry Cambridge University Press, Cambridge [26] Trujillo-Bueno, J, Moreno-Insertis, F, S nchez, F (2001) Astrophysical Spectropolarimetry Cambridge University Press, Cambridge [26] Turner, G (1957) Nineteenth-century studies of the polarization of light re ected by the Moon JBAS, 67, 185 188 [16] Turner, G (1958) The polarization of light re ected by the lunar surface JBAS, 68, 253 263 [16] Umov, N (1912) Eine spektropolariskopische Methode zur Erforschung der Lichtapsorption und der Natur der Farbstoffe Phys Zeitschr, 13, 962 971 [16] Walker, J (1978) More about polarizers and how to use them particularly for studying polarized sky light Scienti c American, 238, 132 136 [3] Whittaker, E (1958) A History of the Theories of Aether and Electricity Thomas Nelson, London ( rst published 1910, Reprinted 1958) [9, 10] Wolstencroft, RD (1985) The search of extra-terrestrial life: recent developments pp 171 175 in Astronomical Sources of Circularly Polarized Light and Their Role in Determining Chirality on Earth IAU Symp No: 112, Boston 18 21 June 1984 Ed MD Papagiannis, Reidel, Dordrecht [25] Zellner, BH, Serkowski, K (1972) Polarization of light by circumstellar material PASP, 84, 619 626 [21].

Each new version removes a bunch of security holes, bugs, and other possible exploits that can make your install vulnerable, and ot updating regularly means you won t get these fixes. This brings us to the first tip. Check your theme s header.php file to see if the following code is there (it almost always is):. Barcode Printer In Java Using Barcode drawer for Java Control to generate, create .Related: Generate EAN-13 VB.NET , VB.NET ISBN Generating , Print UPC-A .NET WinForms

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