SDO HMI 2014-01-12 15:00:24 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 75.80 | 506.88 | 41.56 | 278.56 | -16.44 | 13.39 | -23.02 | 120.02 | 0.4346 | 1043.9 | 374.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.19 | 0.00 | 0.63 | -15.91 | 18.24 | -18.17 | 124.37 | 0.3649 | 846.0 | 651.5 | |
| 3.06 | 4.93 | 1.63 | 2.63 | -14.53 | 16.98 | -19.42 | 119.47 | 0.3714 | 967.2 | 799.1 | |
| 0.00 | 1.36 | 0.00 | 0.73 | -14.89 | 15.84 | -20.56 | 119.06 | 0.3900 | -844.0 | -681.7 | |
| 38.84 | 483.78 | 21.23 | 265.54 | -16.50 | 14.15 | -22.26 | 120.85 | 0.4248 | 1393.9 | 398.3 | |
| 0.00 | 0.93 | 0.00 | 0.52 | -17.63 | 13.47 | -22.94 | 122.48 | 0.4422 | 638.0 | 504.4 | |
| 1.87 | -4.00 | 1.03 | -4.00 | -16.51 | 13.58 | -22.83 | 120.31 | 0.4326 | 1009.5 | 999999 | |
| 1.19 | -4.00 | 0.65 | -4.00 | -16.50 | 13.35 | -23.06 | 120.07 | 0.4358 | 1038.9 | 999999 | |
| 6.03 | -4.00 | 3.32 | -4.00 | -16.59 | 13.07 | -23.34 | 119.97 | 0.4401 | 1173.7 | 999999 | |
| 0.00 | 4.76 | 0.00 | 2.61 | -15.32 | 13.10 | -23.31 | 117.34 | 0.4315 | 754.0 | 499.4 | |
| 24.81 | -4.00 | 13.70 | -4.00 | -16.30 | 12.67 | -23.74 | 119.02 | 0.4437 | 1190.1 | 999999 | |
| 0.00 | 1.27 | 0.00 | 0.74 | -16.13 | 6.57 | -29.84 | 114.19 | 0.5262 | -676.0 | -512.7 | |
| 0.00 | 2.97 | 0.00 | 1.74 | -17.15 | 6.35 | -30.06 | 115.89 | 0.5341 | -781.0 | -525.7 | |
| 0.00 | 3.82 | 0.00 | 2.29 | -18.98 | 4.80 | -31.61 | 118.06 | 0.5638 | -718.0 | -693.8 | |
| 0.00 | 1.87 | 0.00 | 1.13 | -18.10 | 3.48 | -32.93 | 115.84 | 0.5764 | -567.0 | -485.8 | |
| 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. | |