| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 19.05 | 67.83 | 10.39 | 37.18 | 8.55 | 195.05 | -22.72 | 63.39 | 0.4285 | -31.2 | 184.5 | |
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back to the solar disc SDO HMI 2014-05-15 09:00:38 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.17 | 0.00 | 0.63 | 11.59 | 200.50 | -17.27 | 50.03 | 0.3810 | -555.0 | -460.8 | |
| 10.15 | 21.82 | 5.47 | 11.76 | 8.08 | 197.19 | -20.58 | 62.26 | 0.3948 | -1122.0 | -747.5 | |
| 0.00 | 0.90 | 0.00 | 0.48 | 7.37 | 197.07 | -20.70 | 64.02 | 0.3917 | -895.0 | -764.3 | |
| 0.00 | 1.08 | 0.00 | 0.58 | 8.49 | 196.78 | -20.99 | 61.81 | 0.4037 | -722.0 | -565.0 | |
| 0.00 | 1.71 | 0.00 | 0.93 | 8.46 | 196.45 | -21.32 | 62.23 | 0.4081 | -966.0 | -704.6 | |
| 1.44 | 2.60 | 0.78 | 1.42 | 8.69 | 196.01 | -21.76 | 62.22 | 0.4160 | -878.2 | -712.0 | |
| 0.00 | 1.98 | 0.00 | 1.09 | 9.17 | 194.88 | -22.89 | 62.36 | 0.4352 | 157.0 | 289.7 | |
| 0.00 | 1.44 | 0.00 | 0.79 | 9.05 | 194.69 | -23.08 | 62.80 | 0.4371 | 909.0 | 701.8 | |
| 0.00 | 2.16 | 0.00 | 1.19 | 9.50 | 194.16 | -23.61 | 62.42 | 0.4476 | 844.0 | 650.4 | |
| 0.90 | 4.85 | 0.50 | 2.68 | 9.09 | 194.12 | -23.65 | 63.27 | 0.4454 | 1066.7 | 912.2 | |
| 1.71 | 4.40 | 0.95 | 2.44 | 9.07 | 193.75 | -24.02 | 63.67 | 0.4503 | 833.6 | 621.0 | |
| 0.00 | 5.93 | 0.00 | 3.28 | 8.18 | 193.58 | -24.19 | 65.65 | 0.4471 | 1001.0 | 729.0 | |
| 0.00 | 1.44 | 0.00 | 0.80 | 8.70 | 193.47 | -24.30 | 64.66 | 0.4519 | 781.0 | 656.2 | |
| 4.85 | 14.55 | 2.69 | 8.08 | 8.34 | 193.23 | -24.54 | 65.62 | 0.4531 | 997.1 | 694.0 | |
| 0.00 | 1.80 | 0.00 | 1.03 | 10.30 | 190.06 | -27.71 | 64.46 | 0.5091 | 527.0 | 504.3 | |
| 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. | |