SDO HMI 2014-05-30 13:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 30.88 | 132.01 | 15.62 | 66.75 | -9.11 | 24.98 | 7.84 | 222.53 | 0.2001 | 658.5 | 447.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 2.44 | 32.06 | 1.24 | 16.25 | -8.89 | 26.21 | 9.08 | 228.12 | 0.2103 | 1045.3 | 564.9 | |
| 2.71 | -1.00 | 1.37 | -1.00 | -9.04 | 26.19 | 9.05 | 227.48 | 0.2117 | 1146.3 | 999999 | |
| 4.79 | 78.11 | 2.42 | 39.51 | -9.32 | 25.66 | 8.53 | 224.83 | 0.2085 | 960.7 | 530.3 | |
| 16.16 | -3.00 | 8.17 | -3.00 | -9.01 | 25.41 | 8.27 | 225.04 | 0.2017 | 1365.9 | 999999 | |
| 0.00 | 0.99 | 0.00 | 0.50 | -7.66 | 25.10 | 7.97 | 229.20 | 0.1823 | -725.0 | -570.6 | |
| 1.44 | -3.00 | 0.73 | -3.00 | -8.95 | 25.00 | 7.87 | 223.83 | 0.1961 | 1007.7 | 999999 | |
| 0.45 | 2.98 | 0.23 | 1.50 | -9.66 | 23.25 | 6.11 | 214.45 | 0.1864 | 1163.8 | 925.5 | |
| 0.00 | 1.81 | 0.00 | 0.91 | -9.97 | 23.13 | 5.99 | 213.01 | 0.1896 | 862.0 | 761.3 | |
| 2.89 | 7.68 | 1.46 | 3.87 | -9.94 | 22.88 | 5.74 | 212.01 | 0.1869 | 1138.7 | 799.0 | |
| 0.00 | 1.44 | 0.00 | 0.72 | -9.14 | 20.64 | 3.51 | 202.78 | 0.1568 | -988.0 | -776.4 | |
| 0.00 | 3.25 | 0.00 | 1.63 | -8.31 | 20.08 | 2.95 | 201.45 | 0.1399 | -1142.0 | -885.6 | |
| 0.00 | 1.17 | 0.00 | 0.59 | -8.49 | 19.90 | 2.77 | 199.77 | 0.1417 | -980.0 | -751.5 | |
| 0.00 | 1.44 | 0.00 | 0.72 | -9.35 | 19.78 | 2.65 | 197.16 | 0.1552 | -805.0 | -636.4 | |
| 0.00 | 1.08 | 0.00 | 0.55 | -10.81 | 10.81 | -6.33 | 147.95 | 0.2049 | -848.0 | -681.1 | |
| 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. | |