SDO HMI 2014-05-25 05:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 37.49 | 180.26 | 18.95 | 91.18 | -10.58 | 81.58 | -6.10 | 149.76 | 0.1966 | 126.8 | 61.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 22.72 | 65.46 | 11.39 | 32.80 | -9.95 | 85.92 | -1.76 | 168.39 | 0.1507 | 1234.7 | 430.2 | |
| 0.00 | 1.35 | 0.00 | 0.68 | -8.38 | 85.68 | -1.99 | 163.99 | 0.1253 | -566.0 | -479.2 | |
| 0.00 | 2.52 | 0.00 | 1.27 | -11.76 | 84.64 | -3.04 | 163.74 | 0.1865 | 862.0 | 767.1 | |
| 0.00 | 1.89 | 0.00 | 0.95 | -11.17 | 84.52 | -3.16 | 162.17 | 0.1774 | 740.0 | 527.0 | |
| 0.00 | 1.89 | 0.00 | 0.95 | -10.13 | 84.07 | -3.61 | 157.56 | 0.1631 | 1021.0 | 821.0 | |
| 0.00 | 1.35 | 0.00 | 0.68 | -10.46 | 83.23 | -4.45 | 153.92 | 0.1744 | 819.0 | 657.3 | |
| 0.00 | 1.53 | 0.00 | 0.77 | -9.91 | 82.80 | -4.88 | 150.23 | 0.1694 | 681.0 | 520.5 | |
| 0.00 | 1.26 | 0.00 | 0.64 | -12.34 | 82.60 | -5.08 | 155.34 | 0.2080 | 793.0 | 644.4 | |
| 0.00 | 0.90 | 0.00 | 0.46 | -12.71 | 82.47 | -5.21 | 155.53 | 0.2147 | 799.0 | 603.5 | |
| 0.00 | 1.17 | 0.00 | 0.59 | -10.21 | 81.74 | -5.93 | 146.14 | 0.1834 | 1187.0 | 984.6 | |
| 0.00 | 1.08 | 0.00 | 0.55 | -10.64 | 81.49 | -6.19 | 146.32 | 0.1920 | 645.0 | 570.8 | |
| 0.00 | 2.16 | 0.00 | 1.09 | -10.27 | 81.37 | -6.31 | 144.70 | 0.1879 | 849.0 | 635.3 | |
| 0.00 | 1.89 | 0.00 | 0.95 | -10.00 | 81.31 | -6.36 | 143.58 | 0.1847 | 1066.0 | 857.0 | |
| 0.00 | 0.99 | 0.00 | 0.50 | -9.84 | 81.16 | -6.52 | 142.42 | 0.1841 | 793.0 | 641.0 | |
| 1.35 | 23.35 | 0.68 | 11.78 | -10.24 | 80.78 | -6.90 | 142.17 | 0.1935 | 1007.0 | 823.1 | |
| 0.00 | 0.99 | 0.00 | 0.50 | -11.78 | 80.52 | -7.15 | 145.69 | 0.2173 | 659.0 | 446.1 | |
| 0.00 | 1.35 | 0.00 | 0.68 | -10.27 | 80.41 | -7.27 | 140.80 | 0.1979 | 483.0 | 331.9 | |
| 0.00 | 4.96 | 0.00 | 2.51 | -9.31 | 79.31 | -8.37 | 133.50 | 0.1988 | -702.0 | -823.2 | |
| 0.00 | 3.16 | 0.00 | 1.60 | -9.92 | 79.14 | -8.54 | 135.11 | 0.2082 | -989.0 | -771.4 | |
| 1.08 | 2.71 | 0.55 | 1.37 | -10.26 | 79.10 | -8.58 | 136.12 | 0.2127 | -1117.0 | -861.8 | |
| 0.00 | 1.44 | 0.00 | 0.74 | -12.35 | 78.59 | -9.09 | 140.73 | 0.2448 | -877.0 | -718.7 | |
| 0.00 | 1.44 | 0.00 | 0.73 | -10.47 | 78.59 | -9.08 | 135.20 | 0.2213 | -1060.0 | -869.3 | |
| 0.00 | 1.44 | 0.00 | 0.73 | -10.78 | 78.15 | -9.53 | 134.82 | 0.2304 | -824.0 | -609.1 | |
| 2.07 | 10.46 | 1.06 | 5.34 | -11.12 | 77.76 | -9.92 | 134.73 | 0.2390 | -1198.1 | -869.1 | |
| 0.99 | -24.00 | 0.51 | -24.00 | -10.96 | 77.67 | -10.01 | 134.00 | 0.2383 | -1081.1 | 999999 | |
| 0.00 | 1.80 | 0.00 | 0.93 | -12.69 | 77.51 | -10.17 | 138.47 | 0.2610 | -726.0 | -595.2 | |
| 0.00 | 2.52 | 0.00 | 1.28 | -7.77 | 77.48 | -10.19 | 122.03 | 0.2078 | -999.0 | -736.9 | |
| 1.08 | 8.02 | 0.55 | 4.10 | -11.24 | 77.25 | -10.43 | 133.69 | 0.2466 | -1174.6 | -766.0 | |
| 0.00 | 0.90 | 0.00 | 0.46 | -11.85 | 77.19 | -10.48 | 135.33 | 0.2545 | -859.0 | -589.9 | |
| 0.00 | 1.26 | 0.00 | 0.64 | -10.22 | 77.25 | -10.42 | 130.50 | 0.2352 | -944.0 | -744.5 | |
| 0.00 | 1.08 | 0.00 | 0.55 | -10.13 | 77.01 | -10.67 | 129.54 | 0.2374 | -828.0 | -649.6 | |
| 6.76 | 23.80 | 3.47 | 12.23 | -12.25 | 76.83 | -10.85 | 135.48 | 0.2635 | -1220.7 | -580.7 | |
| 0.00 | 0.81 | 0.00 | 0.41 | -9.79 | 76.92 | -10.75 | 128.20 | 0.2350 | -891.0 | -714.9 | |
| 0.00 | 2.07 | 0.00 | 1.06 | -11.85 | 76.78 | -10.89 | 134.25 | 0.2594 | -1092.0 | -898.0 | |
| 1.44 | -32.00 | 0.74 | -32.00 | -12.13 | 76.58 | -11.10 | 134.50 | 0.2650 | -1023.1 | 999999 | |
| 0.00 | 1.26 | 0.00 | 0.66 | -13.62 | 72.31 | -15.37 | 129.30 | 0.3343 | -761.0 | -611.6 | |
| 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. | |