SDO HMI 2014-02-28 03:00:27 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 19.40 | 59.85 | 9.63 | 29.72 | -6.63 | 147.52 | 3.44 | 216.91 | 0.0699 | 196.2 | 277.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.47 | 0.00 | 0.73 | -7.32 | 150.24 | 6.15 | 268.61 | 0.1068 | -671.0 | -550.9 | |
| 2.76 | 9.57 | 1.37 | 4.77 | -7.00 | 149.90 | 5.81 | 271.78 | 0.1010 | 988.6 | 757.9 | |
| 1.21 | 23.97 | 0.60 | 11.92 | -6.92 | 149.33 | 5.24 | 272.96 | 0.0912 | 1006.4 | 741.1 | |
| 1.72 | -3.00 | 0.86 | -3.00 | -6.74 | 149.18 | 5.09 | 275.06 | 0.0889 | 1005.9 | 999999 | |
| 4.14 | -3.00 | 2.06 | -3.00 | -7.01 | 149.12 | 5.03 | 272.06 | 0.0875 | 1092.8 | 999999 | |
| 0.95 | -3.00 | 0.47 | -3.00 | -7.04 | 148.82 | 4.73 | 271.84 | 0.0823 | 1027.7 | 999999 | |
| 1.03 | -3.00 | 0.51 | -3.00 | -7.19 | 148.70 | 4.61 | 270.03 | 0.0802 | 1055.0 | 999999 | |
| 0.00 | 1.29 | 0.00 | 0.64 | -7.37 | 148.52 | 4.44 | 267.71 | 0.0771 | 768.0 | 484.5 | |
| 0.00 | 1.47 | 0.00 | 0.73 | -8.00 | 148.26 | 4.17 | 259.04 | 0.0737 | 1002.0 | 836.3 | |
| 0.00 | 0.95 | 0.00 | 0.47 | -6.51 | 148.25 | 4.16 | 279.43 | 0.0734 | 598.0 | 367.7 | |
| 0.00 | 1.29 | 0.00 | 0.64 | -5.24 | 147.97 | 3.88 | 296.93 | 0.0760 | -911.0 | -765.4 | |
| 0.00 | 2.59 | 0.00 | 1.28 | -6.07 | 146.93 | 2.84 | 291.86 | 0.0533 | 882.0 | 774.4 | |
| 0.00 | 2.93 | 0.00 | 1.45 | -6.02 | 145.37 | 1.29 | 313.02 | 0.0307 | -1043.0 | -861.4 | |
| 7.59 | 14.32 | 3.76 | 7.09 | -5.87 | 143.37 | -0.71 | 27.83 | 0.0267 | -1140.8 | -728.6 | |
| 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. | |