SDO HMI 2014-03-01 00:00:27 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 27.07 | 0.00 | 14.01 | 8.34 | 135.39 | 2.83 | 350.16 | 0.2877 | 163.3 | 191.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.81 | 0.00 | 0.95 | 8.13 | 143.19 | 10.62 | 325.20 | 0.3213 | -870.0 | -619.7 | |
| 0.00 | 0.95 | 0.00 | 0.49 | 5.00 | 142.75 | 10.19 | 319.97 | 0.2752 | -863.0 | -652.4 | |
| 0.00 | 1.81 | 0.00 | 0.94 | 6.49 | 142.60 | 10.04 | 323.64 | 0.2934 | -1015.0 | -763.4 | |
| 0.00 | 0.69 | 0.00 | 0.36 | 10.05 | 141.96 | 9.40 | 331.43 | 0.3378 | -555.0 | -570.9 | |
| 0.00 | 2.67 | 0.00 | 1.38 | 6.88 | 140.94 | 8.38 | 329.18 | 0.2836 | -884.0 | -774.6 | |
| 0.00 | 1.90 | 0.00 | 0.99 | 8.71 | 140.04 | 7.48 | 334.82 | 0.3037 | -917.0 | -737.0 | |
| 0.00 | 1.81 | 0.00 | 0.94 | 10.81 | 135.78 | 3.22 | 349.90 | 0.3157 | 894.0 | 540.7 | |
| 0.00 | 0.95 | 0.00 | 0.49 | 8.05 | 134.82 | 2.26 | 351.58 | 0.2674 | 783.0 | 676.2 | |
| 0.00 | 1.03 | 0.00 | 0.53 | 7.89 | 134.67 | 2.11 | 352.05 | 0.2645 | 823.0 | 683.2 | |
| 0.00 | 1.29 | 0.00 | 0.66 | 7.46 | 133.02 | 0.46 | 358.22 | 0.2548 | 873.0 | 677.3 | |
| 0.00 | 2.16 | 0.00 | 1.12 | 9.87 | 132.21 | -0.35 | 1.18 | 0.2954 | 836.0 | 669.4 | |
| 0.00 | 1.03 | 0.00 | 0.53 | 8.35 | 131.88 | -0.68 | 2.51 | 0.2700 | 781.0 | 637.8 | |
| 0.00 | 1.12 | 0.00 | 0.58 | 8.42 | 130.20 | -2.36 | 8.60 | 0.2739 | 782.0 | 617.5 | |
| 0.00 | 6.04 | 0.00 | 3.11 | 8.61 | 129.95 | -2.61 | 9.36 | 0.2777 | 797.0 | 786.9 | |
| 0.00 | 1.81 | 0.00 | 0.94 | 9.07 | 129.80 | -2.76 | 9.61 | 0.2858 | 984.0 | 808.8 | |
| 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. | |