SDO HMI 2014-04-17 05:00:34 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 77.86 | 341.44 | 40.41 | 177.31 | -9.37 | 246.96 | 16.95 | 255.45 | 0.2983 | 323.7 | 184.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 38.26 | 206.71 | 20.05 | 108.30 | -9.11 | 248.84 | 18.83 | 257.82 | 0.3275 | 1384.3 | 478.6 | |
| 5.49 | -1.00 | 2.87 | -1.00 | -9.73 | 248.26 | 18.25 | 255.60 | 0.3201 | 1015.5 | 999999 | |
| 4.16 | 10.54 | 2.17 | 5.49 | -8.52 | 248.07 | 18.06 | 259.24 | 0.3135 | 1053.5 | 714.8 | |
| 0.00 | 0.71 | 0.00 | 0.37 | -8.73 | 247.28 | 17.27 | 258.19 | 0.3012 | 767.0 | 563.2 | |
| 0.00 | 5.05 | 0.00 | 2.62 | -10.37 | 246.89 | 16.88 | 252.56 | 0.3007 | -947.0 | -710.4 | |
| 0.00 | 2.04 | 0.00 | 1.06 | -10.52 | 246.70 | 16.69 | 251.89 | 0.2985 | -867.0 | -768.6 | |
| 4.07 | 6.20 | 2.11 | 3.21 | -10.32 | 246.31 | 16.30 | 252.20 | 0.2913 | -1012.6 | -794.0 | |
| 0.00 | 1.15 | 0.00 | 0.59 | -8.61 | 245.97 | 15.97 | 257.81 | 0.2795 | 702.0 | 583.8 | |
| 1.51 | 3.01 | 0.78 | 1.56 | -10.30 | 245.83 | 15.82 | 251.81 | 0.2836 | 894.4 | 728.7 | |
| 0.00 | 1.24 | 0.00 | 0.64 | -7.54 | 245.49 | 15.48 | 261.44 | 0.2688 | -748.0 | -566.7 | |
| 0.00 | 1.95 | 0.00 | 1.00 | -8.36 | 245.20 | 15.20 | 258.24 | 0.2661 | -803.0 | -645.9 | |
| 0.00 | 3.99 | 0.00 | 2.05 | -8.00 | 245.16 | 15.15 | 259.56 | 0.2644 | -959.0 | -791.7 | |
| 0.00 | 0.89 | 0.00 | 0.45 | -8.64 | 244.87 | 14.86 | 256.96 | 0.2615 | 758.0 | 616.9 | |
| 0.00 | 1.06 | 0.00 | 0.54 | -8.76 | 244.72 | 14.71 | 256.38 | 0.2594 | 837.0 | 666.8 | |
| 0.00 | 1.42 | 0.00 | 0.73 | -9.09 | 244.70 | 14.69 | 255.11 | 0.2603 | 594.0 | 476.6 | |
| 0.00 | 1.06 | 0.00 | 0.55 | -11.58 | 244.28 | 14.27 | 245.58 | 0.2664 | -873.0 | -723.7 | |
| 4.34 | 6.20 | 2.22 | 3.17 | -8.44 | 243.98 | 13.97 | 257.03 | 0.2462 | 1090.0 | 736.7 | |
| 0.71 | 6.11 | 0.36 | 3.13 | -10.44 | 244.00 | 13.99 | 249.34 | 0.2553 | -970.0 | -814.2 | |
| 0.00 | 0.97 | 0.00 | 0.50 | -10.08 | 243.76 | 13.76 | 250.40 | 0.2496 | -839.0 | -717.8 | |
| 0.97 | 41.98 | 0.50 | 21.41 | -9.48 | 243.55 | 13.54 | 252.49 | 0.2433 | -824.6 | -589.0 | |
| 0.00 | 4.52 | 0.00 | 2.31 | -10.81 | 243.57 | 13.57 | 247.39 | 0.2507 | -732.0 | -584.3 | |
| 10.19 | -20.00 | 5.19 | -20.00 | -9.67 | 243.15 | 13.14 | 251.27 | 0.2378 | -1061.2 | 999999 | |
| 0.00 | 1.33 | 0.00 | 0.68 | -10.15 | 243.14 | 13.13 | 249.32 | 0.2401 | -641.0 | -455.5 | |
| 0.00 | 4.25 | 0.00 | 2.17 | -11.21 | 243.12 | 13.11 | 245.21 | 0.2462 | -1003.0 | -856.6 | |
| 0.62 | 3.28 | 0.32 | 1.67 | -10.76 | 243.01 | 13.00 | 246.76 | 0.2416 | -1018.4 | -836.0 | |
| 0.00 | 0.97 | 0.00 | 0.50 | -10.22 | 242.86 | 12.85 | 248.67 | 0.2360 | -741.0 | -542.0 | |
| 1.42 | 10.45 | 0.72 | 5.32 | -9.62 | 242.68 | 12.67 | 250.89 | 0.2299 | 1028.8 | 783.1 | |
| 0.80 | 2.13 | 0.41 | 1.08 | -10.07 | 242.70 | 12.69 | 249.04 | 0.2326 | -814.3 | -669.4 | |
| 0.53 | 3.19 | 0.27 | 1.62 | -10.46 | 242.59 | 12.58 | 247.28 | 0.2332 | -1008.3 | -714.5 | |
| 2.75 | -27.00 | 1.40 | -27.00 | -9.41 | 242.51 | 12.51 | 251.55 | 0.2262 | 1079.8 | 999999 | |
| 0.00 | 1.68 | 0.00 | 0.86 | -9.98 | 242.47 | 12.47 | 249.08 | 0.2286 | 703.0 | 532.6 | |
| 2.04 | 3.10 | 1.04 | 1.58 | -10.77 | 242.41 | 12.40 | 245.78 | 0.2324 | -887.9 | -685.5 | |
| 0.00 | 1.51 | 0.00 | 0.76 | -8.87 | 242.34 | 12.33 | 253.67 | 0.2209 | 758.0 | 560.8 | |
| 0.00 | 1.42 | 0.00 | 0.72 | -9.14 | 242.32 | 12.31 | 252.46 | 0.2218 | 873.0 | 674.2 | |
| 0.00 | 1.33 | 0.00 | 0.67 | -8.56 | 240.96 | 10.96 | 253.40 | 0.1970 | 906.0 | 752.0 | |
| 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. | |