SDO HMI 2014-05-24 18:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 4.05 | 20.88 | 2.74 | 14.10 | -18.86 | 133.57 | 39.81 | 243.39 | 0.6799 | 3.9 | 30.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.17 | 0.00 | 0.81 | -18.71 | 135.26 | 41.50 | 244.37 | 0.6985 | 330.0 | 348.2 | |
| 1.26 | 2.43 | 0.87 | 1.67 | -18.52 | 135.03 | 41.28 | 244.53 | 0.6952 | 814.2 | 628.8 | |
| 0.00 | 1.35 | 0.00 | 0.93 | -18.80 | 135.08 | 41.32 | 244.16 | 0.6968 | 717.0 | 580.7 | |
| 0.00 | 1.17 | 0.00 | 0.80 | -18.90 | 134.81 | 41.05 | 243.90 | 0.6941 | 715.0 | 527.6 | |
| 0.00 | 1.26 | 0.00 | 0.87 | -19.06 | 134.73 | 40.97 | 243.65 | 0.6938 | 509.0 | 486.1 | |
| 1.98 | 3.24 | 1.34 | 2.19 | -18.03 | 133.88 | 40.12 | 244.72 | 0.6800 | 685.1 | 456.3 | |
| 0.00 | 2.07 | 0.00 | 1.38 | -18.17 | 133.13 | 39.37 | 244.18 | 0.6718 | 241.0 | 302.2 | |
| 0.00 | 1.89 | 0.00 | 1.28 | -20.08 | 133.51 | 39.75 | 241.70 | 0.6844 | -544.0 | -492.2 | |
| 0.00 | 1.08 | 0.00 | 0.71 | -17.55 | 132.18 | 38.43 | 244.64 | 0.6581 | -652.0 | -488.6 | |
| 0.00 | 0.72 | 0.00 | 0.49 | -20.57 | 132.86 | 39.10 | 240.70 | 0.6793 | -583.0 | -501.4 | |
| 0.81 | 1.98 | 0.53 | 1.30 | -17.97 | 131.72 | 37.96 | 243.81 | 0.6544 | -780.8 | -707.5 | |
| 0.00 | 0.90 | 0.00 | 0.60 | -19.62 | 131.92 | 38.16 | 241.55 | 0.6642 | -640.0 | -544.0 | |
| 0.00 | 0.90 | 0.00 | 0.60 | -21.26 | 131.86 | 38.10 | 239.23 | 0.6716 | -564.0 | -448.0 | |
| 0.00 | 0.72 | 0.00 | 0.47 | -21.28 | 130.47 | 36.71 | 238.42 | 0.6561 | -688.0 | -585.1 | |
| 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. | |