SDO HMI 2014-03-15 04:00:29 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 37.98 | 176.01 | 47.06 | 221.14 | 11.28 | 10.33 | 64.43 | 285.60 | 0.9198 | -34.2 | -112.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 6.87 | 97.78 | 9.23 | 129.27 | 11.74 | 11.98 | 66.08 | 285.70 | 0.9312 | -269.0 | -219.4 | |
| 7.39 | -1.00 | 9.65 | -1.00 | 11.51 | 11.35 | 65.45 | 285.60 | 0.9270 | -604.4 | 999999 | |
| 2.17 | -1.00 | 2.86 | -1.00 | 11.97 | 11.49 | 65.58 | 286.05 | 0.9285 | -410.9 | 999999 | |
| 0.00 | 1.39 | 0.00 | 1.75 | 10.56 | 10.65 | 64.75 | 284.76 | 0.9212 | 29.0 | -66.2 | |
| 2.43 | -1.00 | 3.06 | -1.00 | 11.61 | 10.30 | 64.40 | 285.95 | 0.9205 | -512.6 | 999999 | |
| 0.00 | 0.96 | 0.00 | 1.16 | 10.96 | 9.47 | 63.57 | 285.46 | 0.9139 | -159.0 | -177.1 | |
| 0.00 | 12.52 | 0.00 | 15.29 | 11.47 | 9.61 | 63.71 | 285.97 | 0.9157 | -543.0 | -531.3 | |
| 11.21 | 59.71 | 13.12 | 69.47 | 10.61 | 8.66 | 62.76 | 285.29 | 0.9077 | 349.8 | 252.2 | |
| 1.39 | -8.00 | 1.64 | -8.00 | 11.04 | 8.82 | 62.92 | 285.71 | 0.9096 | -293.2 | 999999 | |
| 0.00 | 1.13 | 0.00 | 1.34 | 11.31 | 8.80 | 62.89 | 286.01 | 0.9099 | -479.0 | -358.1 | |
| 6.52 | -8.00 | 7.50 | -8.00 | 10.32 | 8.22 | 62.32 | 285.08 | 0.9041 | 786.1 | 999999 | |
| 0.00 | 1.30 | 0.00 | 1.52 | 11.27 | 8.44 | 62.54 | 286.06 | 0.9073 | -104.0 | -159.1 | |
| 0.00 | 1.22 | 0.00 | 1.34 | 11.08 | 6.76 | 60.85 | 286.29 | 0.8948 | 496.0 | 444.7 | |
| 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. | |