SDO HMI 2014-05-29 19:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 28.07 | 189.77 | 14.05 | 95.17 | -9.05 | 24.75 | -2.30 | 165.91 | 0.1513 | 848.0 | 393.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.90 | 0.00 | 0.45 | -6.27 | 26.87 | -0.17 | 178.13 | 0.0929 | 848.0 | 635.3 | |
| 0.00 | 1.26 | 0.00 | 0.63 | -6.76 | 25.80 | -1.24 | 167.93 | 0.1036 | -919.0 | -672.3 | |
| 28.07 | 164.16 | 14.05 | 82.17 | -9.02 | 25.55 | -1.50 | 169.54 | 0.1431 | 1312.7 | 437.3 | |
| 0.00 | 1.90 | 0.00 | 0.95 | -9.30 | 23.30 | -3.75 | 155.97 | 0.1593 | 953.0 | 712.6 | |
| 0.00 | 1.17 | 0.00 | 0.59 | -9.11 | 23.27 | -3.78 | 155.32 | 0.1566 | 886.0 | 647.2 | |
| 0.00 | 0.72 | 0.00 | 0.36 | -9.69 | 23.26 | -3.79 | 156.78 | 0.1658 | 922.0 | 768.0 | |
| 0.00 | 1.17 | 0.00 | 0.59 | -10.16 | 23.22 | -3.82 | 157.65 | 0.1734 | 852.0 | 738.3 | |
| 0.00 | 1.71 | 0.00 | 0.86 | -9.48 | 23.08 | -3.97 | 155.24 | 0.1637 | 1203.0 | 985.8 | |
| 0.00 | 5.14 | 0.00 | 2.59 | -9.94 | 23.01 | -4.04 | 156.03 | 0.1715 | 666.0 | 760.7 | |
| 0.00 | 1.62 | 0.00 | 0.82 | -8.77 | 20.43 | -6.61 | 140.02 | 0.1780 | -960.0 | -691.3 | |
| 0.00 | 0.99 | 0.00 | 0.51 | -14.17 | 20.07 | -6.97 | 152.75 | 0.2582 | 846.0 | 693.8 | |
| 0.00 | 1.62 | 0.00 | 0.82 | -2.07 | 15.37 | -11.68 | 95.53 | 0.2041 | 984.0 | 782.8 | |
| 0.00 | 1.90 | 0.00 | 0.97 | -5.35 | 14.26 | -12.79 | 109.22 | 0.2344 | -814.0 | -671.0 | |
| 0.00 | 5.51 | 0.00 | 2.86 | -11.91 | 13.03 | -14.01 | 128.76 | 0.3052 | -971.0 | -745.6 | |
| 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. | |