SDO HMI 2014-09-25 00:00:34 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 26.62 | 134.26 | 13.29 | 67.15 | 14.36 | 262.19 | -1.71 | 11.27 | 0.1351 | 62.4 | 79.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.33 | 4.33 | 0.66 | 2.16 | 13.33 | 264.67 | 0.76 | 353.33 | 0.1119 | -993.3 | -694.2 | |
| 0.00 | 2.74 | 0.00 | 1.37 | 14.03 | 264.61 | 0.70 | 354.46 | 0.1238 | -802.0 | -666.5 | |
| 1.68 | 7.51 | 0.84 | 3.75 | 13.73 | 264.55 | 0.64 | 354.72 | 0.1185 | -978.9 | -702.7 | |
| 4.24 | 8.04 | 2.11 | 4.01 | 12.97 | 264.48 | 0.58 | 354.64 | 0.1053 | -1033.0 | -716.1 | |
| 0.00 | 0.88 | 0.00 | 0.44 | 14.21 | 264.42 | 0.52 | 356.02 | 0.1267 | -855.0 | -618.7 | |
| 0.00 | 1.59 | 0.00 | 0.79 | 13.21 | 264.39 | 0.48 | 355.67 | 0.1093 | -345.0 | -267.8 | |
| 0.00 | 1.68 | 0.00 | 0.84 | 12.88 | 264.20 | 0.30 | 357.18 | 0.1033 | -932.0 | -603.7 | |
| 0.00 | 0.71 | 0.00 | 0.35 | 14.94 | 264.12 | 0.21 | 358.54 | 0.1391 | -577.0 | -424.4 | |
| 0.00 | 10.08 | 0.00 | 5.03 | 14.27 | 263.84 | -0.07 | 0.54 | 0.1275 | -1122.0 | -658.7 | |
| 2.30 | 10.34 | 1.15 | 5.17 | 14.70 | 263.68 | -0.23 | 1.63 | 0.1349 | -1079.2 | -747.7 | |
| 0.00 | 0.62 | 0.00 | 0.31 | 15.34 | 263.62 | -0.29 | 1.91 | 0.1460 | -670.0 | -552.4 | |
| 2.30 | -10.00 | 1.15 | -10.00 | 14.94 | 263.56 | -0.35 | 2.44 | 0.1392 | -1052.3 | 999999 | |
| 0.00 | 2.12 | 0.00 | 1.06 | 12.79 | 263.25 | -0.66 | 6.32 | 0.1023 | -913.0 | -590.8 | |
| 0.00 | 1.77 | 0.00 | 0.88 | 13.79 | 262.91 | -1.00 | 8.14 | 0.1203 | 871.0 | 667.8 | |
| 0.00 | 1.68 | 0.00 | 0.84 | 14.79 | 262.56 | -1.35 | 9.49 | 0.1384 | 887.0 | 677.7 | |
| 0.00 | 0.88 | 0.00 | 0.44 | 12.88 | 262.45 | -1.46 | 13.58 | 0.1062 | -926.0 | -786.7 | |
| 2.30 | 9.64 | 1.15 | 4.81 | 14.33 | 262.35 | -1.56 | 11.65 | 0.1313 | 918.1 | 590.0 | |
| 1.86 | 8.75 | 0.92 | 4.36 | 12.73 | 262.11 | -1.80 | 16.99 | 0.1052 | 929.5 | 345.6 | |
| 0.00 | 0.80 | 0.00 | 0.40 | 13.79 | 262.07 | -1.84 | 14.71 | 0.1231 | 575.0 | 368.9 | |
| 0.00 | 1.24 | 0.00 | 0.62 | 15.85 | 261.96 | -1.94 | 11.95 | 0.1583 | -646.0 | -466.9 | |
| 2.21 | 3.71 | 1.11 | 1.86 | 15.58 | 261.75 | -2.16 | 13.66 | 0.1545 | -919.0 | -644.5 | |
| 6.90 | 18.65 | 3.44 | 9.32 | 14.03 | 261.67 | -2.24 | 17.17 | 0.1291 | 1102.6 | 585.3 | |
| 0.00 | 1.77 | 0.00 | 0.88 | 13.73 | 261.64 | -2.27 | 18.12 | 0.1242 | 109.0 | 96.4 | |
| 0.00 | 1.06 | 0.00 | 0.53 | 14.00 | 261.17 | -2.74 | 20.76 | 0.1313 | -750.0 | -552.7 | |
| 0.00 | 0.88 | 0.00 | 0.44 | 14.72 | 260.76 | -3.15 | 21.51 | 0.1456 | 953.0 | 768.9 | |
| 0.35 | 2.83 | 0.18 | 1.42 | 15.60 | 260.68 | -3.22 | 19.85 | 0.1602 | 739.2 | 558.8 | |
| 0.00 | 2.48 | 0.00 | 1.24 | 13.81 | 260.68 | -3.23 | 24.68 | 0.1317 | -876.0 | -662.6 | |
| 0.00 | 0.88 | 0.00 | 0.44 | 13.57 | 260.62 | -3.29 | 25.89 | 0.1283 | 520.0 | 454.1 | |
| 0.00 | 2.03 | 0.00 | 1.02 | 13.48 | 260.40 | -3.50 | 27.68 | 0.1286 | 865.0 | 629.1 | |
| 0.62 | 4.33 | 0.31 | 2.17 | 15.36 | 260.25 | -3.66 | 22.87 | 0.1590 | 1180.9 | 803.5 | |
| 0.00 | 0.88 | 0.00 | 0.44 | 16.27 | 260.08 | -3.83 | 21.64 | 0.1746 | 776.0 | 550.5 | |
| 0.00 | 7.25 | 0.00 | 3.64 | 15.63 | 259.65 | -4.26 | 25.39 | 0.1674 | 1207.0 | 851.9 | |
| 0.53 | 3.18 | 0.27 | 1.60 | 15.62 | 259.21 | -4.69 | 27.62 | 0.1707 | 1124.3 | 890.9 | |
| 0.00 | 2.30 | 0.00 | 1.16 | 15.56 | 258.93 | -4.97 | 29.19 | 0.1721 | 1017.0 | 858.8 | |
| 0.00 | 1.59 | 0.00 | 0.80 | 15.40 | 258.59 | -5.32 | 31.29 | 0.1727 | 894.0 | 729.7 | |
| 0.00 | 5.04 | 0.00 | 2.56 | 17.96 | 258.14 | -5.76 | 26.58 | 0.2146 | 833.0 | 628.8 | |
| 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. | |