SDO HMI 2014-04-07 18:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 29.92 | 0.00 | 15.27 | -8.78 | 8.45 | 13.56 | 257.36 | 0.2407 | 366.1 | 281.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.58 | 0.00 | 0.82 | -5.93 | 11.98 | 17.09 | 269.85 | 0.2936 | 902.0 | 715.1 | |
| 0.00 | 1.32 | 0.00 | 0.68 | -11.06 | 11.16 | 16.27 | 251.93 | 0.2905 | -874.0 | -667.3 | |
| 0.00 | 3.78 | 0.00 | 1.95 | -8.60 | 10.91 | 16.02 | 260.27 | 0.2781 | 945.0 | 772.1 | |
| 0.00 | 1.23 | 0.00 | 0.63 | -9.15 | 10.59 | 15.70 | 258.12 | 0.2742 | 997.0 | 843.4 | |
| 0.00 | 2.55 | 0.00 | 1.31 | -9.22 | 10.31 | 15.42 | 257.69 | 0.2698 | 899.0 | 731.4 | |
| 0.00 | 2.38 | 0.00 | 1.22 | -8.93 | 9.88 | 15.00 | 258.50 | 0.2620 | 852.0 | 636.4 | |
| 0.00 | 1.23 | 0.00 | 0.63 | -7.61 | 9.71 | 14.82 | 263.48 | 0.2564 | 793.0 | 690.9 | |
| 0.00 | 3.08 | 0.00 | 1.58 | -7.88 | 9.63 | 14.74 | 262.38 | 0.2554 | 849.0 | 691.1 | |
| 0.00 | 1.14 | 0.00 | 0.58 | -10.19 | 8.56 | 13.67 | 252.47 | 0.2450 | 951.0 | 698.6 | |
| 0.00 | 1.06 | 0.00 | 0.54 | -10.34 | 8.53 | 13.64 | 251.85 | 0.2453 | 822.0 | 642.3 | |
| 0.00 | 2.02 | 0.00 | 1.02 | -7.50 | 6.78 | 11.89 | 262.81 | 0.2069 | -875.0 | -653.3 | |
| 0.00 | 2.38 | 0.00 | 1.20 | -7.40 | 5.95 | 11.06 | 262.91 | 0.1926 | -873.0 | -654.4 | |
| 0.00 | 2.64 | 0.00 | 1.33 | -7.58 | 5.52 | 10.63 | 261.66 | 0.1857 | -921.0 | -750.7 | |
| 0.00 | 0.97 | 0.00 | 0.49 | -8.11 | 4.92 | 10.03 | 258.31 | 0.1769 | -816.0 | -692.7 | |
| 0.00 | 0.88 | 0.00 | 0.44 | -12.26 | 4.70 | 9.81 | 237.06 | 0.1994 | 797.0 | 677.1 | |
| 0.00 | 1.06 | 0.00 | 0.54 | -15.59 | 3.04 | 8.16 | 219.64 | 0.2152 | 932.0 | 774.0 | |
| 0.00 | 0.62 | 0.00 | 0.31 | -9.95 | 358.98 | 4.09 | 226.61 | 0.0972 | 843.0 | 597.4 | |
| 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. | |