SDO HMI 2014-04-22 23:00:35 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 64.65 | 419.65 | 35.62 | 231.21 | 17.72 | 166.61 | 12.55 | 331.73 | 0.4383 | -699.1 | -276.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 62.25 | 383.51 | 34.32 | 211.59 | 17.72 | 167.01 | 12.95 | 330.91 | 0.4409 | -1261.7 | -376.8 | |
| 0.00 | 1.33 | 0.00 | 0.72 | 16.45 | 164.67 | 10.61 | 334.10 | 0.4061 | 635.0 | 520.9 | |
| 0.00 | 1.42 | 0.00 | 0.77 | 16.99 | 164.32 | 10.26 | 335.44 | 0.4115 | 609.0 | 446.4 | |
| 0.00 | 1.24 | 0.00 | 0.68 | 17.28 | 163.66 | 9.60 | 337.12 | 0.4114 | 739.0 | 626.5 | |
| 0.00 | 1.07 | 0.00 | 0.58 | 17.43 | 163.32 | 9.26 | 338.01 | 0.4116 | 771.0 | 689.1 | |
| 0.00 | 1.24 | 0.00 | 0.68 | 17.99 | 163.25 | 9.19 | 338.67 | 0.4194 | 865.0 | 739.4 | |
| 0.00 | 11.10 | 0.00 | 6.05 | 18.08 | 162.87 | 8.81 | 339.55 | 0.4186 | 883.0 | 724.4 | |
| 0.00 | 0.98 | 0.00 | 0.53 | 18.28 | 162.72 | 8.66 | 340.04 | 0.4207 | 644.0 | 605.6 | |
| 0.00 | 0.80 | 0.00 | 0.44 | 19.17 | 162.71 | 8.64 | 340.81 | 0.4338 | 420.0 | 407.1 | |
| 0.00 | 1.42 | 0.00 | 0.78 | 18.93 | 162.44 | 8.37 | 341.19 | 0.4289 | 759.0 | 651.3 | |
| 0.00 | 2.31 | 0.00 | 1.25 | 17.91 | 162.32 | 8.26 | 340.59 | 0.4131 | 788.0 | 730.7 | |
| 0.00 | 3.11 | 0.00 | 1.68 | 17.18 | 161.49 | 7.43 | 341.83 | 0.3978 | 898.0 | 779.1 | |
| 0.00 | 3.46 | 0.00 | 1.87 | 17.51 | 161.35 | 7.28 | 342.43 | 0.4021 | 738.0 | 731.4 | |
| 0.98 | 2.40 | 0.53 | 1.30 | 17.73 | 160.43 | 6.37 | 344.67 | 0.4013 | 907.6 | 686.3 | |
| 1.42 | 4.26 | 0.77 | 2.29 | 17.27 | 160.29 | 6.22 | 344.68 | 0.3936 | 1014.2 | 800.8 | |
| 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. | |