SDO HMI 2014-04-05 09:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 32.37 | 148.69 | 17.58 | 80.79 | 17.70 | 29.97 | 3.74 | 351.34 | 0.4141 | -222.3 | -409.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.26 | 123.35 | 0.14 | 67.04 | 17.50 | 31.28 | 5.06 | 348.22 | 0.4135 | -958.7 | -548.3 | |
| 16.89 | -1.00 | 9.19 | -1.00 | 17.70 | 30.91 | 4.68 | 349.16 | 0.4153 | -1198.5 | 999999 | |
| 2.11 | -1.00 | 1.15 | -1.00 | 17.56 | 30.68 | 4.46 | 349.61 | 0.4126 | -1338.9 | 999999 | |
| 1.32 | -1.00 | 0.72 | -1.00 | 18.02 | 30.57 | 4.34 | 350.07 | 0.4195 | -762.9 | 999999 | |
| 0.88 | -1.00 | 0.48 | -1.00 | 17.63 | 30.53 | 4.30 | 349.99 | 0.4132 | -1140.5 | 999999 | |
| 0.00 | 1.32 | 0.00 | 0.75 | 23.68 | 27.73 | 1.50 | 357.25 | 0.5022 | 672.0 | 488.5 | |
| 0.00 | 1.06 | 0.00 | 0.57 | 17.06 | 26.24 | 0.02 | 359.96 | 0.3980 | 684.0 | 546.1 | |
| 6.42 | 14.78 | 3.47 | 7.99 | 17.39 | 25.71 | -0.52 | 1.23 | 0.4034 | 1049.2 | 755.4 | |
| 0.00 | 2.02 | 0.00 | 1.10 | 17.68 | 25.58 | -0.64 | 1.51 | 0.4082 | 690.0 | 566.3 | |
| 0.00 | 1.32 | 0.00 | 0.72 | 18.18 | 25.49 | -0.74 | 1.70 | 0.4161 | 783.0 | 658.9 | |
| 4.49 | -8.00 | 2.43 | -8.00 | 17.42 | 25.46 | -0.77 | 1.82 | 0.4040 | 1053.8 | 999999 | |
| 0.00 | 2.20 | 0.00 | 1.20 | 18.41 | 25.36 | -0.87 | 1.97 | 0.4199 | 792.0 | 662.9 | |
| 0.00 | 1.67 | 0.00 | 0.90 | 16.93 | 25.33 | -0.89 | 2.17 | 0.3962 | 864.0 | 658.8 | |
| 0.00 | 0.97 | 0.00 | 0.52 | 15.84 | 22.53 | -3.70 | 9.36 | 0.3832 | -710.0 | -525.1 | |
| 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. | |