| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 155.86 | 732.88 | 79.38 | 373.64 | 4.34 | 245.65 | 9.02 | 318.85 | 0.2348 | -204.6 | -162.6 | |
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back to the solar disc SDO HMI 2014-04-16 17:00:34 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.42 | 0.00 | 0.74 | 5.35 | 250.50 | 13.87 | 307.84 | 0.3035 | -807.0 | -645.3 | |
| 34.41 | 427.61 | 17.69 | 219.48 | 4.79 | 248.22 | 11.60 | 311.38 | 0.2682 | -1482.7 | -445.9 | |
| 2.74 | -2.00 | 1.41 | -2.00 | 4.08 | 248.09 | 11.46 | 309.68 | 0.2587 | -1180.2 | 999999 | |
| 28.13 | -2.00 | 14.43 | -2.00 | 4.41 | 247.88 | 11.25 | 311.18 | 0.2596 | -1566.4 | 999999 | |
| 6.02 | -2.00 | 3.08 | -2.00 | 4.16 | 247.47 | 10.85 | 311.49 | 0.2517 | -1461.9 | 999999 | |
| 0.53 | -2.00 | 0.27 | -2.00 | 4.71 | 247.27 | 10.64 | 313.63 | 0.2554 | -892.7 | 999999 | |
| 0.00 | 1.50 | 0.00 | 0.76 | 2.59 | 246.14 | 9.51 | 310.15 | 0.2170 | -861.0 | -715.4 | |
| 0.00 | 1.06 | 0.00 | 0.54 | 2.92 | 245.81 | 9.18 | 312.31 | 0.2164 | -929.0 | -763.2 | |
| 10.88 | 18.49 | 5.53 | 9.40 | 3.98 | 245.70 | 9.07 | 316.10 | 0.2278 | -1080.6 | -636.7 | |
| 0.00 | 1.50 | 0.00 | 0.76 | 2.37 | 245.59 | 8.96 | 311.06 | 0.2074 | -899.0 | -699.3 | |
| 0.00 | 1.33 | 0.00 | 0.67 | 3.89 | 245.42 | 8.79 | 316.70 | 0.2234 | -930.0 | -765.0 | |
| 0.00 | 1.15 | 0.00 | 0.58 | 3.43 | 245.32 | 8.70 | 315.57 | 0.2166 | -956.0 | -739.0 | |
| 0.00 | 1.24 | 0.00 | 0.63 | 5.17 | 245.26 | 8.63 | 320.91 | 0.2380 | 555.0 | 425.6 | |
| 3.80 | 5.84 | 1.93 | 2.97 | 4.07 | 245.12 | 8.49 | 318.25 | 0.2222 | -1117.7 | -853.9 | |
| 1.42 | 6.10 | 0.72 | 3.09 | 3.48 | 244.93 | 8.30 | 317.09 | 0.2126 | -1068.0 | -851.9 | |
| 5.48 | 22.65 | 2.79 | 11.51 | 4.64 | 244.82 | 8.19 | 320.93 | 0.2264 | -1080.4 | -713.5 | |
| 4.78 | -16.00 | 2.43 | -16.00 | 4.49 | 244.54 | 7.92 | 321.46 | 0.2214 | -1205.0 | 999999 | |
| 0.00 | 3.27 | 0.00 | 1.66 | 4.06 | 244.42 | 7.79 | 320.67 | 0.2143 | -503.0 | -564.9 | |
| 0.00 | 1.50 | 0.00 | 0.76 | 4.48 | 244.09 | 7.46 | 323.09 | 0.2165 | -137.0 | -120.8 | |
| 0.00 | 0.88 | 0.00 | 0.45 | 2.41 | 244.04 | 7.41 | 316.68 | 0.1887 | -762.0 | -600.6 | |
| 0.00 | 1.24 | 0.00 | 0.62 | 2.29 | 243.95 | 7.32 | 316.59 | 0.1861 | -952.0 | -801.1 | |
| 0.00 | 2.74 | 0.00 | 1.39 | 3.75 | 243.93 | 7.30 | 321.56 | 0.2049 | -966.0 | -705.6 | |
| 0.00 | 2.74 | 0.00 | 1.39 | 5.36 | 243.79 | 7.17 | 326.49 | 0.2260 | -704.0 | -539.5 | |
| 0.00 | 0.88 | 0.00 | 0.44 | 1.86 | 243.28 | 6.65 | 317.71 | 0.1728 | 618.0 | 491.1 | |
| 0.00 | 1.24 | 0.00 | 0.62 | 2.07 | 243.07 | 6.44 | 319.44 | 0.1731 | 760.0 | 453.5 | |
| 0.00 | 1.42 | 0.00 | 0.72 | 4.81 | 243.09 | 6.46 | 327.81 | 0.2115 | -607.0 | -377.4 | |
| 0.97 | 2.92 | 0.49 | 1.47 | 1.49 | 242.97 | 6.35 | 317.59 | 0.1646 | 959.3 | 726.4 | |
| 0.00 | 3.10 | 0.00 | 1.56 | 3.52 | 242.77 | 6.15 | 325.61 | 0.1901 | -304.0 | -262.9 | |
| 0.00 | 1.42 | 0.00 | 0.72 | 4.37 | 242.78 | 6.15 | 327.97 | 0.2024 | 650.0 | 515.4 | |
| 0.00 | 1.50 | 0.00 | 0.76 | 3.06 | 242.68 | 6.05 | 324.62 | 0.1827 | -707.0 | -681.2 | |
| 0.00 | 1.59 | 0.00 | 0.80 | 3.64 | 242.59 | 5.96 | 326.76 | 0.1900 | 318.0 | 255.2 | |
| 0.00 | 3.45 | 0.00 | 1.74 | 4.37 | 242.45 | 5.82 | 329.38 | 0.1994 | 308.0 | 177.0 | |
| 0.00 | 1.42 | 0.00 | 0.71 | 2.94 | 242.13 | 5.51 | 326.75 | 0.1756 | 835.0 | 578.4 | |
| 0.00 | 0.80 | 0.00 | 0.40 | 5.01 | 242.12 | 5.49 | 332.33 | 0.2063 | 660.0 | 447.3 | |
| 0.71 | 167.01 | 0.36 | 84.24 | 3.88 | 242.08 | 5.45 | 329.73 | 0.1889 | 801.2 | 556.1 | |
| 0.00 | 0.53 | 0.00 | 0.27 | 1.15 | 241.85 | 5.23 | 321.68 | 0.1475 | 404.0 | 548.2 | |
| 2.57 | -35.00 | 1.29 | -35.00 | 3.88 | 241.81 | 5.18 | 330.99 | 0.1866 | 946.3 | 999999 | |
| 2.12 | -35.00 | 1.07 | -35.00 | 4.70 | 241.57 | 4.94 | 334.07 | 0.1973 | 609.3 | 999999 | |
| 0.53 | 10.88 | 0.27 | 5.46 | 2.51 | 241.56 | 4.93 | 328.27 | 0.1640 | 1180.7 | 906.2 | |
| 0.00 | 1.15 | 0.00 | 0.58 | 3.05 | 241.50 | 4.87 | 330.23 | 0.1716 | 908.0 | 675.1 | |
| 0.00 | 1.68 | 0.00 | 0.85 | 5.19 | 241.52 | 4.89 | 335.36 | 0.2045 | 275.0 | 214.6 | |
| 35.56 | -35.00 | 17.95 | -35.00 | 4.39 | 241.45 | 4.82 | 333.95 | 0.1916 | 1171.0 | 999999 | |
| 0.00 | 1.59 | 0.00 | 0.80 | 2.99 | 241.17 | 4.54 | 331.77 | 0.1679 | 1088.0 | 897.2 | |
| 0.00 | 4.51 | 0.00 | 2.27 | 2.72 | 241.14 | 4.51 | 331.15 | 0.1634 | 1081.0 | 808.0 | |
| 15.21 | -35.00 | 7.67 | -35.00 | 4.00 | 241.11 | 4.48 | 334.64 | 0.1829 | 1279.7 | 999999 | |
| 0.00 | 0.97 | 0.00 | 0.49 | 5.40 | 241.03 | 4.40 | 337.94 | 0.2045 | 767.0 | 698.0 | |
| 0.00 | 4.51 | 0.00 | 2.26 | 2.02 | 240.98 | 4.35 | 329.82 | 0.1516 | 490.0 | 845.1 | |
| 0.00 | 2.12 | 0.00 | 1.07 | 2.90 | 240.95 | 4.33 | 332.65 | 0.1648 | 996.0 | 858.2 | |
| 0.00 | 1.42 | 0.00 | 0.71 | 1.74 | 240.89 | 4.26 | 329.42 | 0.1467 | 847.0 | 776.6 | |
| 0.00 | 1.33 | 0.00 | 0.67 | 3.41 | 240.75 | 4.12 | 335.12 | 0.1712 | 1012.0 | 871.5 | |
| 0.00 | 1.42 | 0.00 | 0.71 | 4.30 | 240.51 | 3.88 | 338.32 | 0.1836 | 923.0 | 749.5 | |
| 0.00 | 1.24 | 0.00 | 0.62 | 1.68 | 240.44 | 3.81 | 331.96 | 0.1419 | 787.0 | 655.3 | |
| 0.00 | 3.45 | 0.00 | 1.74 | 4.60 | 240.36 | 3.73 | 339.66 | 0.1876 | 1123.0 | 939.0 | |
| 0.00 | 2.03 | 0.00 | 1.03 | 5.18 | 239.67 | 3.04 | 344.06 | 0.1933 | 823.0 | 631.3 | |
| 0.00 | 1.42 | 0.00 | 0.71 | 4.17 | 239.27 | 2.64 | 344.67 | 0.1747 | 846.0 | 588.9 | |
| 0.00 | 0.88 | 0.00 | 0.44 | 4.05 | 238.64 | 2.01 | 348.08 | 0.1701 | 1118.0 | 862.0 | |
| 0.00 | 1.59 | 0.00 | 0.80 | 5.73 | 238.40 | 1.77 | 351.00 | 0.1978 | 823.0 | 495.1 | |
| 0.00 | 1.15 | 0.00 | 0.58 | 6.43 | 237.19 | 0.57 | 357.28 | 0.2078 | 811.0 | 563.8 | |
| Proj. U | - Projected umbra area in millionths of solar disc, negative values indicate | |
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that the umbra consists of fragmented regions which cannot be separated without losing umbral area. In this way several spots (intensity minima in the umbra) have a common umbra, e.g. -2 means that the given spot shares an umbra with spot No.2, and the common U value is indicated at spot No.2. |
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| Proj. WS | - Projected whole spot area in millionths of solar disc, negative values indicate | |
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that several umbras have a common penumbra, e.g. -7 means that the given umbra shares a penumbra with umbra No.7, and the WS value is indicated at No.7. |
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| Corr. U | - Corrected umbra area in millionths of solar hemisphere, for negative values see above | |
| Corr. WS | - Corrected whole spot area in millionths of solar hemisphere, for negative values see above | |
| B | - Heliographic latitude B; positive: North, negative: South | |
| L | - Heliographic longitude L | |
| LCM | - Longitudinal distance from the Sun's central meridian | |
| Pos. angle | - Position angle | |
| r | - Distance from the centre of Sun's disc in terms of Sun's radius | |
| MU | - Mean magnetic field within the umbra contour averaged the pixel values with sign. | |
| MP | - Mean magnetic field within the penumbra contour averaged the pixel values with sign. | |