SDO HMI 2014-04-05 14:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 34.03 | 153.88 | 18.59 | 84.02 | 17.68 | 30.11 | 6.63 | 344.90 | 0.4226 | -453.7 | -264.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 24.01 | 126.01 | 13.13 | 68.89 | 17.70 | 30.92 | 7.44 | 343.08 | 0.4256 | -1242.4 | -443.1 | |
| 2.02 | -1.00 | 1.11 | -1.00 | 18.02 | 30.59 | 7.10 | 344.03 | 0.4290 | -848.3 | 999999 | |
| 3.43 | -1.00 | 1.87 | -1.00 | 17.79 | 30.55 | 7.06 | 343.96 | 0.4254 | -1132.3 | 999999 | |
| 0.00 | 1.14 | 0.00 | 0.63 | 18.35 | 30.19 | 6.70 | 345.09 | 0.4323 | -615.0 | -503.8 | |
| 0.00 | 1.58 | 0.00 | 0.87 | 18.02 | 30.08 | 6.59 | 345.11 | 0.4268 | -814.0 | -667.3 | |
| 0.00 | 1.14 | 0.00 | 0.62 | 17.32 | 29.93 | 6.44 | 345.00 | 0.4156 | -968.0 | -713.5 | |
| 0.00 | 1.06 | 0.00 | 0.59 | 20.57 | 29.35 | 5.86 | 348.03 | 0.4630 | 692.0 | 473.8 | |
| 0.00 | 1.49 | 0.00 | 0.80 | 15.55 | 27.58 | 4.10 | 349.50 | 0.3795 | 879.0 | 660.6 | |
| 0.00 | 5.01 | 0.00 | 2.70 | 16.52 | 27.32 | 3.84 | 350.59 | 0.3942 | 426.0 | 703.6 | |
| 4.57 | 10.64 | 2.48 | 5.76 | 17.42 | 25.64 | 2.16 | 354.89 | 0.4052 | 1083.3 | 840.1 | |
| 0.00 | 0.88 | 0.00 | 0.48 | 18.11 | 25.59 | 2.10 | 355.17 | 0.4162 | 750.0 | 639.1 | |
| 0.00 | 1.32 | 0.00 | 0.72 | 17.75 | 25.55 | 2.07 | 355.18 | 0.4103 | 768.0 | 656.7 | |
| 0.00 | 1.06 | 0.00 | 0.58 | 18.28 | 25.53 | 2.04 | 355.35 | 0.4187 | 669.0 | 595.1 | |
| 0.00 | 1.41 | 0.00 | 0.77 | 18.51 | 25.31 | 1.82 | 355.88 | 0.4221 | 825.0 | 694.5 | |
| 0.00 | 1.14 | 0.00 | 0.61 | 16.41 | 24.41 | 0.92 | 357.70 | 0.3877 | 649.0 | 514.5 | |
| 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. | |