SDO HMI 2014-07-09 08:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 63.87 | 404.20 | 48.16 | 304.63 | -19.18 | 254.43 | 43.98 | 240.42 | 0.7564 | 892.0 | 292.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.82 | 0.00 | 0.74 | -20.82 | 263.00 | 52.55 | 242.16 | 0.8412 | 615.0 | 528.6 | |
| 0.00 | 1.09 | 0.00 | 0.89 | -23.11 | 256.71 | 46.26 | 236.90 | 0.7954 | -628.0 | -478.1 | |
| 0.27 | 388.67 | 0.20 | 292.94 | -18.47 | 254.51 | 44.06 | 241.33 | 0.7541 | 993.0 | 312.3 | |
| 61.51 | -3.00 | 46.40 | -3.00 | -19.09 | 254.49 | 44.04 | 240.56 | 0.7566 | 1174.2 | 999999 | |
| 0.00 | 1.54 | 0.00 | 1.17 | -21.81 | 253.57 | 43.11 | 236.82 | 0.7605 | 396.0 | 353.9 | |
| 1.54 | 3.00 | 1.16 | 2.25 | -21.22 | 253.22 | 42.76 | 237.33 | 0.7542 | 630.1 | 505.1 | |
| 0.00 | 1.64 | 0.00 | 1.23 | -22.24 | 252.78 | 42.33 | 235.88 | 0.7552 | -476.0 | -386.6 | |
| 0.55 | 1.45 | 0.40 | 1.08 | -22.09 | 251.75 | 41.30 | 235.47 | 0.7446 | -629.0 | -499.5 | |
| 0.00 | 1.09 | 0.00 | 0.79 | -20.29 | 251.10 | 40.65 | 237.28 | 0.7285 | -657.0 | -537.9 | |
| 0.00 | 2.27 | 0.00 | 1.64 | -20.52 | 251.13 | 40.68 | 237.01 | 0.7301 | -758.0 | -521.0 | |
| 0.00 | 0.45 | 0.00 | 0.32 | -20.55 | 250.37 | 39.92 | 236.53 | 0.7226 | -536.0 | -577.0 | |
| 0.00 | 1.00 | 0.00 | 0.73 | -23.49 | 249.73 | 39.28 | 232.59 | 0.7333 | -513.0 | -383.2 | |
| 0.00 | 1.18 | 0.00 | 0.85 | -23.75 | 249.35 | 38.90 | 232.04 | 0.7313 | -201.0 | -242.3 | |
| 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. | |