SDO HMI 2014-01-13 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 |
| 92.05 | 463.91 | 47.35 | 238.70 | -16.49 | 13.12 | -10.12 | 141.49 | 0.2717 | 1021.7 | 396.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.93 | 0.00 | 0.48 | -14.77 | 14.54 | -8.70 | 141.06 | 0.2339 | -802.0 | -579.3 | |
| 54.65 | 286.32 | 28.07 | 146.98 | -16.59 | 13.77 | -9.47 | 143.42 | 0.2658 | 1405.3 | 472.6 | |
| 0.00 | 3.23 | 0.00 | 1.66 | -16.34 | 12.78 | -10.46 | 140.11 | 0.2728 | 916.0 | 755.3 | |
| 0.00 | 1.61 | 0.00 | 0.83 | -15.77 | 12.78 | -10.46 | 138.67 | 0.2656 | 981.0 | 785.8 | |
| 0.00 | 2.89 | 0.00 | 1.48 | -15.40 | 12.68 | -10.56 | 137.43 | 0.2624 | 915.0 | 720.8 | |
| 8.84 | 161.22 | 4.56 | 83.18 | -16.76 | 12.51 | -10.73 | 140.40 | 0.2810 | 1024.8 | 308.6 | |
| 0.00 | 0.76 | 0.00 | 0.39 | -14.83 | 12.40 | -10.84 | 135.12 | 0.2589 | -778.0 | -606.1 | |
| 28.56 | -6.00 | 14.72 | -6.00 | -16.27 | 12.26 | -10.98 | 138.58 | 0.2777 | 1290.9 | 999999 | |
| 0.00 | 1.95 | 0.00 | 1.03 | -15.48 | 6.85 | -16.39 | 125.70 | 0.3363 | -858.0 | -686.9 | |
| 0.00 | 0.76 | 0.00 | 0.40 | -14.94 | 6.80 | -16.44 | 124.24 | 0.3322 | -700.0 | -580.2 | |
| 0.00 | 1.44 | 0.00 | 0.76 | -15.80 | 6.44 | -16.80 | 125.86 | 0.3446 | -834.0 | -713.6 | |
| 0.00 | 1.02 | 0.00 | 0.55 | -19.02 | 4.42 | -18.82 | 130.08 | 0.4002 | -821.0 | -651.3 | |
| 0.00 | 0.93 | 0.00 | 0.49 | -10.09 | 3.73 | -19.51 | 107.51 | 0.3464 | -774.0 | -608.4 | |
| 0.00 | 0.85 | 0.00 | 0.47 | -19.62 | 1.71 | -21.53 | 127.78 | 0.4391 | -749.0 | -589.4 | |
| 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. | |