SDO HMI 2014-05-16 00:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 28.10 | 154.02 | 19.11 | 104.15 | 15.29 | 248.85 | 39.36 | 295.92 | 0.6823 | -321.7 | -252.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 16.52 | 141.52 | 11.27 | 96.23 | 15.44 | 249.41 | 39.92 | 295.83 | 0.6895 | -734.5 | -332.0 | |
| 7.90 | -1.00 | 5.35 | -1.00 | 15.37 | 248.94 | 39.45 | 295.96 | 0.6838 | -949.9 | 999999 | |
| 3.68 | -1.00 | 2.49 | -1.00 | 15.68 | 248.72 | 39.24 | 296.50 | 0.6828 | -843.1 | 999999 | |
| 0.00 | 1.44 | 0.00 | 0.93 | 11.76 | 247.31 | 37.82 | 291.67 | 0.6483 | 688.0 | 529.7 | |
| 0.00 | 0.45 | 0.00 | 0.29 | 11.87 | 246.90 | 37.41 | 292.03 | 0.6436 | 628.0 | 518.4 | |
| 0.00 | 2.42 | 0.00 | 1.56 | 11.61 | 246.62 | 37.14 | 291.79 | 0.6391 | 664.0 | 503.2 | |
| 0.00 | 1.53 | 0.00 | 0.98 | 11.42 | 246.44 | 36.95 | 291.59 | 0.6359 | 579.0 | 604.2 | |
| 0.00 | 1.08 | 0.00 | 0.70 | 13.80 | 246.22 | 36.73 | 295.21 | 0.6442 | 676.0 | 558.3 | |
| 0.00 | 1.26 | 0.00 | 0.81 | 13.64 | 246.00 | 36.51 | 295.10 | 0.6407 | 802.0 | 705.5 | |
| 0.00 | 1.17 | 0.00 | 0.75 | 14.39 | 245.67 | 36.18 | 296.37 | 0.6405 | 288.0 | 341.2 | |
| 0.00 | 0.81 | 0.00 | 0.50 | 16.57 | 241.21 | 31.73 | 302.54 | 0.6001 | 558.0 | 458.3 | |
| 0.00 | 0.99 | 0.00 | 0.59 | 14.19 | 238.85 | 29.36 | 300.77 | 0.5554 | 632.0 | 525.1 | |
| 0.00 | 1.35 | 0.00 | 0.81 | 16.79 | 238.32 | 28.83 | 305.26 | 0.5676 | 578.0 | 451.3 | |
| 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. | |