SDO HMI 2014-04-05 12:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 26.74 | 149.43 | 14.54 | 81.40 | 17.60 | 30.29 | 5.71 | 346.86 | 0.4178 | -302.3 | -395.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.06 | 127.44 | 0.57 | 69.49 | 17.29 | 31.31 | 6.72 | 344.36 | 0.4164 | -1038.6 | -507.1 | |
| 1.32 | -1.00 | 0.72 | -1.00 | 17.52 | 31.29 | 6.70 | 344.56 | 0.4198 | -922.6 | 999999 | |
| 14.69 | -1.00 | 8.01 | -1.00 | 17.68 | 30.91 | 6.33 | 345.48 | 0.4207 | -1285.7 | 999999 | |
| 1.67 | -1.00 | 0.91 | -1.00 | 17.62 | 30.69 | 6.10 | 345.94 | 0.4188 | -1376.2 | 999999 | |
| 1.58 | -1.00 | 0.86 | -1.00 | 17.68 | 30.53 | 5.95 | 346.32 | 0.4192 | -1138.1 | 999999 | |
| 0.00 | 1.50 | 0.00 | 0.82 | 18.17 | 30.17 | 5.58 | 347.39 | 0.4254 | -698.0 | -590.4 | |
| 0.00 | 2.29 | 0.00 | 1.25 | 17.94 | 30.07 | 5.48 | 347.49 | 0.4215 | -805.0 | -664.3 | |
| 0.00 | 1.41 | 0.00 | 0.75 | 15.44 | 27.59 | 3.00 | 352.22 | 0.3750 | 858.0 | 699.2 | |
| 0.00 | 2.11 | 0.00 | 1.14 | 16.45 | 27.48 | 2.90 | 352.85 | 0.3909 | 790.0 | 634.9 | |
| 0.00 | 1.14 | 0.00 | 0.62 | 16.61 | 27.26 | 2.68 | 353.43 | 0.3931 | 765.0 | 638.5 | |
| 5.45 | 7.74 | 2.95 | 4.19 | 17.42 | 25.67 | 1.09 | 357.42 | 0.4041 | 1046.3 | 812.9 | |
| 0.00 | 0.79 | 0.00 | 0.43 | 17.72 | 25.55 | 0.96 | 357.74 | 0.4087 | 736.0 | 655.4 | |
| 0.97 | 2.11 | 0.52 | 1.14 | 17.49 | 25.39 | 0.81 | 358.10 | 0.4050 | 990.6 | 855.9 | |
| 0.00 | 1.76 | 0.00 | 0.96 | 18.44 | 25.33 | 0.75 | 358.31 | 0.4202 | 907.0 | 719.7 | |
| 0.00 | 1.14 | 0.00 | 0.61 | 16.38 | 24.38 | -0.20 | 0.50 | 0.3869 | 817.0 | 572.9 | |
| 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. | |