SDO HMI 2014-04-25 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 |
| 9.43 | 36.72 | 5.17 | 19.98 | -20.27 | 140.72 | 19.12 | 228.24 | 0.4130 | 465.9 | 272.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.33 | 0.00 | 0.73 | -18.85 | 143.76 | 22.16 | 235.02 | 0.4376 | 834.0 | 669.5 | |
| 0.00 | 1.33 | 0.00 | 0.74 | -20.95 | 143.41 | 21.81 | 230.59 | 0.4509 | 548.0 | 479.9 | |
| 0.00 | 2.40 | 0.00 | 1.33 | -20.87 | 142.98 | 21.38 | 230.23 | 0.4450 | 609.0 | 611.6 | |
| 0.00 | 1.16 | 0.00 | 0.63 | -18.29 | 142.49 | 20.89 | 234.70 | 0.4166 | 789.0 | 630.8 | |
| 9.07 | 12.10 | 4.98 | 6.64 | -20.32 | 142.28 | 20.68 | 230.40 | 0.4316 | 1054.1 | 757.7 | |
| 0.00 | 1.33 | 0.00 | 0.73 | -19.87 | 141.88 | 20.28 | 230.77 | 0.4225 | 941.0 | 807.5 | |
| 0.00 | 1.07 | 0.00 | 0.58 | -20.14 | 140.89 | 19.29 | 228.93 | 0.4131 | 835.0 | 715.6 | |
| 0.36 | 1.87 | 0.19 | 1.02 | -21.18 | 140.92 | 19.32 | 227.01 | 0.4236 | 833.0 | 711.6 | |
| 0.00 | 4.36 | 0.00 | 2.36 | -20.42 | 139.80 | 18.20 | 226.85 | 0.4030 | 502.0 | 465.3 | |
| 0.00 | 3.20 | 0.00 | 1.70 | -18.74 | 138.17 | 16.57 | 227.74 | 0.3666 | 448.0 | 351.1 | |
| 0.00 | 1.42 | 0.00 | 0.76 | -20.22 | 137.23 | 15.62 | 223.09 | 0.3715 | -836.0 | -782.4 | |
| 0.00 | 1.42 | 0.00 | 0.76 | -21.07 | 137.21 | 15.61 | 221.45 | 0.3810 | -848.0 | -708.4 | |
| 0.00 | 2.22 | 0.00 | 1.19 | -20.85 | 137.09 | 15.49 | 221.64 | 0.3772 | -817.0 | -788.0 | |
| 0.00 | 1.51 | 0.00 | 0.81 | -21.50 | 136.15 | 14.55 | 218.75 | 0.3750 | -780.0 | -613.3 | |
| 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. | |