| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 3.43 | 23.95 | 1.70 | 11.88 | -7.87 | 7.35 | 0.93 | 179.52 | 0.0512 | 42.9 | -80.4 | |
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back to the solar disc SDO HMI 2014-04-06 21:00:32 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.50 | 0.00 | 0.75 | -8.16 | 12.91 | 6.48 | 252.78 | 0.1175 | 788.0 | 596.1 | |
| 0.00 | 0.79 | 0.00 | 0.39 | -7.49 | 10.89 | 4.47 | 253.72 | 0.0808 | 814.0 | 649.6 | |
| 0.00 | 1.50 | 0.00 | 0.74 | -9.24 | 10.43 | 4.00 | 232.45 | 0.0872 | 1177.0 | 965.9 | |
| 0.53 | 1.32 | 0.26 | 0.66 | -9.66 | 10.22 | 3.79 | 227.25 | 0.0891 | 1018.7 | 806.3 | |
| 0.00 | 0.97 | 0.00 | 0.48 | -7.77 | 9.47 | 3.04 | 242.64 | 0.0595 | 810.0 | 630.6 | |
| 0.00 | 2.64 | 0.00 | 1.31 | -7.59 | 9.44 | 3.01 | 245.18 | 0.0577 | 938.0 | 711.1 | |
| 0.00 | 0.70 | 0.00 | 0.35 | -8.10 | 9.05 | 2.62 | 233.94 | 0.0563 | 806.0 | 599.1 | |
| 0.00 | 0.97 | 0.00 | 0.48 | -11.17 | 8.12 | 1.69 | 198.57 | 0.0915 | 751.0 | 560.4 | |
| 0.00 | 1.50 | 0.00 | 0.74 | -6.90 | 5.90 | -0.53 | 142.78 | 0.0151 | -936.0 | -655.6 | |
| 1.32 | 3.87 | 0.65 | 1.92 | -6.93 | 5.69 | -0.74 | 134.40 | 0.0180 | -1017.9 | -751.4 | |
| 0.00 | 0.88 | 0.00 | 0.44 | -7.62 | 5.54 | -0.89 | 147.89 | 0.0291 | -842.0 | -612.4 | |
| 0.88 | 5.37 | 0.44 | 2.66 | -7.65 | 5.14 | -1.28 | 138.45 | 0.0336 | -1174.8 | -958.3 | |
| 0.70 | -12.00 | 0.35 | -12.00 | -7.50 | 5.11 | -1.31 | 134.64 | 0.0321 | -1127.1 | 999999 | |
| 0.00 | 1.94 | 0.00 | 0.96 | -7.74 | 3.78 | -2.65 | 120.17 | 0.0532 | -1084.0 | -799.6 | |
| 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. | |