SDO HMI 2014-05-20 21:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 28.34 | 143.94 | 35.30 | 173.37 | -11.30 | 79.49 | -65.53 | 101.50 | 0.9117 | -241.0 | 17.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 2.07 | 58.47 | 2.23 | 63.25 | -11.04 | 82.53 | -62.48 | 101.39 | 0.8898 | 741.7 | 251.3 | |
| 4.77 | -1.00 | 5.14 | -1.00 | -10.74 | 82.51 | -62.50 | 101.04 | 0.8898 | 698.4 | 999999 | |
| 0.00 | 0.27 | 0.00 | 0.30 | -12.04 | 81.78 | -63.23 | 102.46 | 0.8960 | 478.0 | 405.3 | |
| 0.00 | 2.16 | 0.00 | 2.59 | -11.54 | 79.47 | -65.54 | 101.75 | 0.9127 | -314.0 | -262.6 | |
| 0.00 | 5.04 | 0.00 | 6.04 | -11.17 | 79.49 | -65.52 | 101.34 | 0.9124 | -662.0 | -501.1 | |
| 0.00 | 1.17 | 0.00 | 1.48 | -13.24 | 78.22 | -66.79 | 103.53 | 0.9218 | 139.0 | 106.6 | |
| 0.00 | 2.34 | 0.00 | 2.86 | -11.15 | 78.96 | -66.05 | 101.30 | 0.9161 | -447.0 | -328.0 | |
| 0.00 | 1.35 | 0.00 | 1.70 | -12.37 | 78.29 | -66.72 | 102.59 | 0.9210 | 244.0 | 180.1 | |
| 0.00 | 0.63 | 0.00 | 0.80 | -12.54 | 77.96 | -67.05 | 102.76 | 0.9233 | 228.0 | 133.3 | |
| 3.87 | 66.21 | 4.90 | 85.95 | -11.21 | 78.07 | -66.94 | 101.32 | 0.9221 | -703.3 | -88.4 | |
| 2.79 | 4.23 | 3.73 | 5.64 | -13.19 | 76.85 | -68.16 | 103.40 | 0.9306 | -424.5 | -348.2 | |
| 2.52 | -10.00 | 3.26 | -10.00 | -11.29 | 77.63 | -67.38 | 101.39 | 0.9250 | -460.8 | 999999 | |
| 12.32 | -10.00 | 16.04 | -10.00 | -11.53 | 77.43 | -67.59 | 101.64 | 0.9264 | -510.3 | 999999 | |
| 0.00 | 2.07 | 0.00 | 2.76 | -12.13 | 76.86 | -68.15 | 102.26 | 0.9302 | -628.0 | -562.1 | |
| 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. | |