SDO HMI 2014-04-05 05:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 30.61 | 177.70 | 16.59 | 96.36 | 17.59 | 30.15 | 1.74 | 355.93 | 0.4090 | 28.8 | -398.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.97 | 151.49 | 0.52 | 82.12 | 17.43 | 31.33 | 2.91 | 353.13 | 0.4071 | -758.6 | -495.9 | |
| 11.79 | -1.00 | 6.39 | -1.00 | 17.59 | 30.92 | 2.51 | 354.12 | 0.4090 | -1249.9 | 999999 | |
| 0.79 | -1.00 | 0.43 | -1.00 | 17.26 | 30.85 | 2.44 | 354.20 | 0.4036 | -1373.1 | 999999 | |
| 1.67 | -1.00 | 0.91 | -1.00 | 17.42 | 30.67 | 2.25 | 354.68 | 0.4060 | -1343.6 | 999999 | |
| 2.02 | -1.00 | 1.10 | -1.00 | 17.85 | 30.58 | 2.16 | 354.98 | 0.4126 | -823.3 | 999999 | |
| 0.00 | 1.23 | 0.00 | 0.67 | 18.91 | 29.23 | 0.81 | 358.19 | 0.4281 | 552.0 | 334.9 | |
| 0.00 | 1.14 | 0.00 | 0.65 | 23.65 | 27.82 | -0.59 | 1.09 | 0.5016 | 725.0 | 609.7 | |
| 0.00 | 0.97 | 0.00 | 0.52 | 16.35 | 27.18 | -1.23 | 3.06 | 0.3875 | 661.0 | 554.3 | |
| 0.00 | 0.88 | 0.00 | 0.47 | 16.61 | 27.15 | -1.26 | 3.11 | 0.3917 | 753.0 | 557.2 | |
| 0.00 | 1.41 | 0.00 | 0.76 | 17.66 | 25.66 | -2.75 | 6.42 | 0.4106 | 690.0 | 597.0 | |
| 13.37 | 17.33 | 7.24 | 9.39 | 17.37 | 25.64 | -2.78 | 6.57 | 0.4059 | 1043.1 | 750.2 | |
| 0.00 | 1.41 | 0.00 | 0.77 | 18.26 | 25.37 | -3.04 | 6.92 | 0.4205 | 815.0 | 620.8 | |
| 0.00 | 0.70 | 0.00 | 0.38 | 16.95 | 25.27 | -3.15 | 7.58 | 0.3999 | 710.0 | 562.9 | |
| 0.00 | 1.14 | 0.00 | 0.63 | 18.53 | 25.05 | -3.37 | 7.55 | 0.4254 | 753.0 | 566.2 | |
| 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. | |