SDO HMI 2014-05-30 11:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 32.05 | 134.30 | 16.18 | 67.72 | -9.14 | 24.85 | 6.62 | 217.61 | 0.1877 | 709.2 | 431.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 3.52 | 28.90 | 1.78 | 14.60 | -9.05 | 26.17 | 7.93 | 223.74 | 0.1980 | 1093.8 | 528.7 | |
| 2.89 | -1.00 | 1.46 | -1.00 | -8.92 | 26.16 | 7.93 | 224.17 | 0.1964 | 1085.3 | 999999 | |
| 0.00 | 1.35 | 0.00 | 0.68 | -9.63 | 25.74 | 7.51 | 220.20 | 0.2005 | -4.0 | 14.0 | |
| 5.96 | 78.30 | 3.01 | 39.50 | -9.29 | 25.70 | 7.47 | 221.19 | 0.1957 | 999.5 | 509.8 | |
| 18.33 | -4.00 | 9.25 | -4.00 | -9.02 | 25.42 | 7.19 | 221.05 | 0.1889 | 1353.4 | 999999 | |
| 0.00 | 1.35 | 0.00 | 0.68 | -7.85 | 24.07 | 5.84 | 219.63 | 0.1587 | 921.0 | 705.7 | |
| 0.00 | 4.34 | 0.00 | 2.18 | -9.66 | 23.29 | 5.06 | 209.62 | 0.1767 | 1110.0 | 925.1 | |
| 0.00 | 2.26 | 0.00 | 1.14 | -10.03 | 23.24 | 5.00 | 208.33 | 0.1818 | 807.0 | 682.2 | |
| 1.35 | 8.31 | 0.68 | 4.18 | -9.88 | 22.86 | 4.63 | 206.91 | 0.1765 | 1179.7 | 831.9 | |
| 0.00 | 1.08 | 0.00 | 0.54 | -9.11 | 20.57 | 2.34 | 195.70 | 0.1496 | -1108.0 | -892.2 | |
| 0.00 | 3.61 | 0.00 | 1.81 | -8.25 | 20.08 | 1.84 | 193.91 | 0.1330 | -767.0 | -743.8 | |
| 0.00 | 1.54 | 0.00 | 0.77 | -8.43 | 19.92 | 1.69 | 192.49 | 0.1355 | -1122.0 | -967.1 | |
| 0.00 | 1.54 | 0.00 | 0.77 | -9.35 | 19.71 | 1.48 | 189.78 | 0.1504 | -899.0 | -754.4 | |
| 0.00 | 1.72 | 0.00 | 0.87 | -10.78 | 10.79 | -7.45 | 143.54 | 0.2152 | -941.0 | -777.6 | |
| 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. | |