SDO HMI 2014-04-05 10:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 27.36 | 155.01 | 14.86 | 84.28 | 17.59 | 30.12 | 4.44 | 349.72 | 0.4140 | -223.5 | -385.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.32 | 128.35 | 0.72 | 69.85 | 17.18 | 31.32 | 5.64 | 346.71 | 0.4105 | -918.3 | -523.5 | |
| 0.26 | -1.00 | 0.14 | -1.00 | 17.51 | 31.27 | 5.59 | 347.02 | 0.4153 | -961.3 | 999999 | |
| 14.52 | -1.00 | 7.90 | -1.00 | 17.70 | 30.90 | 5.22 | 347.96 | 0.4171 | -1239.0 | 999999 | |
| 2.29 | -1.00 | 1.24 | -1.00 | 17.57 | 30.67 | 4.99 | 348.39 | 0.4142 | -1356.2 | 999999 | |
| 0.00 | 1.41 | 0.00 | 0.77 | 17.93 | 30.11 | 4.43 | 349.82 | 0.4182 | -749.0 | -631.9 | |
| 0.00 | 1.06 | 0.00 | 0.57 | 15.90 | 29.28 | 3.60 | 350.90 | 0.3838 | -882.0 | -745.7 | |
| 0.00 | 3.08 | 0.00 | 1.66 | 16.54 | 27.29 | 1.61 | 356.03 | 0.3905 | 717.0 | 611.4 | |
| 0.00 | 1.14 | 0.00 | 0.62 | 17.06 | 26.26 | 0.58 | 358.60 | 0.3981 | 711.0 | 571.2 | |
| 6.33 | 13.72 | 3.43 | 7.42 | 17.39 | 25.66 | -0.02 | 0.04 | 0.4033 | 1071.9 | 813.4 | |
| 0.00 | 2.20 | 0.00 | 1.19 | 17.71 | 25.57 | -0.11 | 0.26 | 0.4085 | 692.0 | 532.6 | |
| 0.00 | 1.32 | 0.00 | 0.72 | 18.08 | 25.51 | -0.17 | 0.40 | 0.4143 | 806.0 | 624.7 | |
| 2.64 | -9.00 | 1.43 | -9.00 | 17.45 | 25.38 | -0.30 | 0.71 | 0.4043 | 964.0 | 999999 | |
| 0.00 | 1.67 | 0.00 | 0.91 | 18.41 | 25.35 | -0.33 | 0.75 | 0.4196 | 775.0 | 649.9 | |
| 0.00 | 1.06 | 0.00 | 0.57 | 16.99 | 25.35 | -0.33 | 0.80 | 0.3970 | 768.0 | 635.2 | |
| 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. | |