SDO HMI 2014-10-21 23:00:30 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 48.84 | 305.29 | 42.70 | 266.28 | -8.94 | 321.92 | 53.69 | 255.27 | 0.8252 | 620.1 | 262.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.31 | 0.00 | 1.18 | -9.14 | 323.37 | 55.13 | 255.42 | 0.8392 | -244.0 | -194.2 | |
| 47.36 | 291.36 | 41.42 | 254.79 | -8.88 | 322.05 | 53.82 | 255.38 | 0.8264 | 855.8 | 284.3 | |
| 1.48 | -2.00 | 1.28 | -2.00 | -9.39 | 321.55 | 53.32 | 254.63 | 0.8227 | 914.1 | 999999 | |
| 0.00 | 1.04 | 0.00 | 0.88 | -9.20 | 320.60 | 52.37 | 254.60 | 0.8131 | 536.0 | 534.4 | |
| 0.00 | 1.31 | 0.00 | 1.10 | -8.99 | 320.31 | 52.08 | 254.76 | 0.8097 | 729.0 | 693.9 | |
| 0.00 | 0.70 | 0.00 | 0.60 | -11.47 | 320.89 | 52.66 | 251.98 | 0.8215 | -488.0 | -334.1 | |
| 0.00 | 1.04 | 0.00 | 0.85 | -7.87 | 319.22 | 50.99 | 255.82 | 0.7961 | -376.0 | -314.2 | |
| 0.00 | 1.04 | 0.00 | 0.86 | -10.84 | 319.15 | 50.92 | 252.18 | 0.8030 | -420.0 | -272.8 | |
| 0.00 | 0.96 | 0.00 | 0.79 | -10.49 | 318.97 | 50.74 | 252.55 | 0.8003 | -321.0 | -291.2 | |
| 0.00 | 2.44 | 0.00 | 2.01 | -10.71 | 318.97 | 50.74 | 252.29 | 0.8009 | -414.0 | -316.9 | |
| 0.00 | 1.74 | 0.00 | 1.42 | -10.80 | 318.61 | 50.38 | 252.06 | 0.7975 | -349.0 | -299.4 | |
| 0.00 | 0.78 | 0.00 | 0.62 | -9.07 | 317.73 | 49.50 | 253.89 | 0.7838 | -440.0 | -353.4 | |
| 0.00 | 0.70 | 0.00 | 0.53 | -9.36 | 315.67 | 47.44 | 252.86 | 0.7628 | -286.0 | -330.9 | |
| 0.00 | 0.87 | 0.00 | 0.65 | -8.65 | 314.36 | 46.12 | 253.31 | 0.7463 | -626.0 | -537.7 | |
| 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. | |