SDO HMI 2014-01-13 17:00:24 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.10 | 27.92 | 0.59 | 14.84 | 16.24 | 25.98 | 3.84 | 349.71 | 0.3620 | 240.6 | 102.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 4.16 | 0.00 | 2.22 | 15.78 | 29.53 | 7.39 | 340.22 | 0.3675 | -1118.0 | -930.5 | |
| 0.00 | 2.97 | 0.00 | 1.58 | 15.94 | 29.17 | 7.03 | 341.26 | 0.3679 | -539.0 | -531.7 | |
| 0.00 | 0.85 | 0.00 | 0.45 | 14.96 | 29.01 | 6.87 | 340.74 | 0.3521 | -854.0 | -745.2 | |
| 0.00 | 1.19 | 0.00 | 0.63 | 16.68 | 27.89 | 5.76 | 345.03 | 0.3735 | -703.0 | -558.6 | |
| 0.34 | 2.29 | 0.18 | 1.21 | 15.51 | 26.38 | 4.25 | 348.15 | 0.3492 | -948.8 | -739.5 | |
| 0.76 | 3.31 | 0.41 | 1.77 | 17.43 | 25.62 | 3.49 | 351.12 | 0.3778 | 931.7 | 711.4 | |
| 0.00 | 2.89 | 0.00 | 1.53 | 16.04 | 25.53 | 3.40 | 350.73 | 0.3552 | 1007.0 | 813.1 | |
| 0.00 | 1.10 | 0.00 | 0.59 | 16.95 | 24.60 | 2.46 | 353.56 | 0.3679 | 829.0 | 661.4 | |
| 0.00 | 1.78 | 0.00 | 0.95 | 16.26 | 24.55 | 2.42 | 353.44 | 0.3565 | 794.0 | 680.0 | |
| 0.00 | 0.85 | 0.00 | 0.45 | 17.27 | 23.70 | 1.57 | 355.95 | 0.3717 | 569.0 | 419.4 | |
| 0.00 | 0.93 | 0.00 | 0.49 | 15.91 | 22.96 | 0.82 | 357.73 | 0.3488 | 807.0 | 685.2 | |
| 0.00 | 2.04 | 0.00 | 1.08 | 15.91 | 22.77 | 0.64 | 358.24 | 0.3487 | 908.0 | 713.2 | |
| 0.00 | 1.78 | 0.00 | 0.94 | 15.78 | 22.59 | 0.45 | 358.74 | 0.3466 | 898.0 | 673.3 | |
| 0.00 | 1.78 | 0.00 | 0.95 | 17.17 | 22.47 | 0.33 | 359.13 | 0.3692 | 718.0 | 682.3 | |
| 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. | |