SDO HMI 2014-05-19 09:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 27.61 | 167.33 | 32.97 | 194.66 | -13.30 | 229.38 | 64.52 | 256.19 | 0.9050 | 330.6 | 156.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.35 | 0.00 | 1.81 | -14.44 | 233.07 | 68.21 | 255.33 | 0.9311 | 306.0 | 216.9 | |
| 13.04 | 146.36 | 15.72 | 174.48 | -12.65 | 230.45 | 65.59 | 257.10 | 0.9132 | 577.7 | 193.0 | |
| 0.00 | 1.35 | 0.00 | 1.58 | -12.65 | 229.70 | 64.83 | 257.05 | 0.9079 | 419.0 | 421.7 | |
| 14.57 | -2.00 | 17.25 | -2.00 | -13.26 | 229.93 | 65.06 | 256.39 | 0.9098 | 627.9 | 999999 | |
| 0.00 | 3.24 | 0.00 | 3.71 | -12.57 | 229.08 | 64.22 | 257.09 | 0.9034 | 572.0 | 573.2 | |
| 0.00 | 0.27 | 0.00 | 0.30 | -11.40 | 228.01 | 63.15 | 258.33 | 0.8949 | -316.0 | -353.0 | |
| 0.00 | 0.99 | 0.00 | 1.09 | -11.59 | 228.01 | 63.15 | 258.12 | 0.8950 | -170.0 | -183.8 | |
| 0.00 | 0.72 | 0.00 | 0.76 | -11.28 | 226.88 | 62.01 | 258.38 | 0.8860 | -237.0 | -286.4 | |
| 0.00 | 1.35 | 0.00 | 1.40 | -15.83 | 225.87 | 61.00 | 253.15 | 0.8811 | -188.0 | -189.7 | |
| 0.00 | 0.63 | 0.00 | 0.60 | -14.06 | 223.36 | 58.49 | 254.87 | 0.8587 | -508.0 | -464.9 | |
| 0.00 | 0.90 | 0.00 | 0.87 | -15.06 | 223.48 | 58.62 | 253.73 | 0.8608 | -494.0 | -392.5 | |
| 0.00 | 1.35 | 0.00 | 1.29 | -18.69 | 222.41 | 57.55 | 249.37 | 0.8562 | -322.0 | -243.9 | |
| 0.00 | 2.25 | 0.00 | 1.90 | -21.94 | 216.68 | 51.81 | 244.25 | 0.8116 | -524.0 | -398.5 | |
| 0.00 | 1.17 | 0.00 | 0.98 | -21.75 | 216.58 | 51.72 | 244.45 | 0.8102 | -507.0 | -400.4 | |
| 0.00 | 0.72 | 0.00 | 0.59 | -20.82 | 215.29 | 50.43 | 245.23 | 0.7958 | -610.0 | -578.8 | |
| 0.00 | 2.34 | 0.00 | 1.75 | -16.32 | 212.14 | 47.28 | 250.04 | 0.7524 | -669.0 | -591.2 | |
| 0.00 | 2.34 | 0.00 | 1.55 | -24.28 | 201.26 | 36.40 | 234.70 | 0.6650 | -804.0 | -645.9 | |
| 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. | |