SDO HMI 2014-01-14 02:00:24 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.87 | 21.29 | 1.01 | 11.48 | 16.80 | 27.40 | 10.22 | 334.85 | 0.4022 | 126.5 | -134.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.02 | 2.38 | 0.55 | 1.29 | 15.96 | 30.00 | 12.82 | 328.41 | 0.4090 | -914.4 | -812.2 | |
| 0.00 | 1.79 | 0.00 | 0.97 | 16.05 | 29.75 | 12.57 | 329.02 | 0.4082 | -679.0 | -567.0 | |
| 0.00 | 1.36 | 0.00 | 0.73 | 16.00 | 28.87 | 11.69 | 330.76 | 0.4005 | -758.0 | -622.2 | |
| 0.00 | 2.98 | 0.00 | 1.62 | 17.83 | 28.39 | 11.21 | 333.90 | 0.4225 | -665.0 | -532.0 | |
| 0.85 | 2.13 | 0.46 | 1.15 | 16.81 | 27.98 | 10.80 | 333.60 | 0.4051 | -615.8 | -523.1 | |
| 0.00 | 2.98 | 0.00 | 1.59 | 15.29 | 27.52 | 10.34 | 332.78 | 0.3802 | -930.0 | -783.4 | |
| 0.00 | 0.85 | 0.00 | 0.46 | 16.66 | 26.34 | 9.17 | 336.98 | 0.3921 | 774.0 | 619.7 | |
| 0.00 | 1.53 | 0.00 | 0.84 | 20.18 | 26.19 | 9.01 | 340.53 | 0.4430 | 807.0 | 717.2 | |
| 0.00 | 0.94 | 0.00 | 0.50 | 17.54 | 25.58 | 8.40 | 339.56 | 0.4005 | 823.0 | 664.1 | |
| 0.00 | 1.19 | 0.00 | 0.64 | 16.08 | 25.29 | 8.11 | 338.82 | 0.3770 | 765.0 | 549.3 | |
| 0.00 | 1.02 | 0.00 | 0.55 | 17.25 | 24.60 | 7.42 | 341.53 | 0.3908 | 714.0 | 620.2 | |
| 0.00 | 0.77 | 0.00 | 0.41 | 16.33 | 24.50 | 7.32 | 340.96 | 0.3763 | 827.0 | 673.8 | |
| 0.00 | 0.43 | 0.00 | 0.23 | 20.23 | 24.35 | 7.18 | 344.30 | 0.4350 | 722.0 | 600.8 | |
| 0.00 | 0.94 | 0.00 | 0.50 | 16.03 | 23.47 | 6.29 | 343.24 | 0.3667 | 774.0 | 680.0 | |
| 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. | |