SDO HMI 2014-04-23 10:00:35 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 48.34 | 341.39 | 111.25 | 801.96 | -12.11 | 226.49 | 78.46 | 258.62 | 0.9770 | 84.8 | 195.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 6.75 | 36.96 | 22.83 | 129.40 | -11.04 | 230.39 | 82.36 | 259.54 | 0.9899 | 64.3 | -65.7 | |
| 0.00 | 1.42 | 0.00 | 5.96 | -12.72 | 232.10 | 84.07 | 257.74 | 0.9934 | 21.0 | 20.1 | |
| 12.00 | 118.18 | 30.78 | 296.59 | -10.04 | 227.59 | 79.56 | 260.71 | 0.9821 | 146.1 | 366.9 | |
| 0.00 | 2.40 | 0.00 | 6.88 | -11.53 | 228.89 | 80.87 | 259.12 | 0.9859 | 298.0 | 275.5 | |
| 2.40 | 9.24 | 5.84 | 22.97 | -12.45 | 227.11 | 79.08 | 258.27 | 0.9802 | 256.2 | 395.4 | |
| 0.00 | 1.07 | 0.00 | 2.14 | -10.43 | 224.32 | 76.30 | 260.47 | 0.9700 | 49.0 | 31.9 | |
| 3.91 | 15.02 | 7.57 | 29.47 | -10.68 | 223.86 | 75.84 | 260.22 | 0.9680 | 435.7 | 286.6 | |
| 6.04 | 92.59 | 10.96 | 167.75 | -13.15 | 222.77 | 74.75 | 257.70 | 0.9627 | -527.7 | 211.7 | |
| 8.09 | 57.40 | 18.02 | 130.19 | -16.23 | 226.00 | 77.98 | 254.45 | 0.9758 | 286.5 | -10.7 | |
| 6.93 | -8.00 | 12.12 | -8.00 | -13.57 | 222.19 | 74.17 | 257.28 | 0.9600 | 62.1 | 999999 | |
| 0.00 | 1.16 | 0.00 | 2.09 | -14.50 | 222.92 | 74.90 | 256.29 | 0.9633 | 449.0 | 424.4 | |
| 0.00 | 1.42 | 0.00 | 2.14 | -16.51 | 219.40 | 71.38 | 254.21 | 0.9456 | -265.0 | -132.6 | |
| 2.22 | 3.82 | 3.13 | 5.39 | -16.71 | 218.03 | 70.00 | 253.98 | 0.9379 | -414.8 | -293.3 | |
| 0.00 | 0.71 | 0.00 | 0.99 | -16.60 | 217.84 | 69.82 | 254.09 | 0.9368 | -198.0 | -161.8 | |
| 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. | |