SDO HMI 2014-05-17 13:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 50.33 | 301.40 | 26.84 | 160.82 | -24.03 | 191.81 | 2.69 | 186.70 | 0.3732 | 734.4 | 334.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.44 | 0.00 | 0.75 | -20.02 | 195.53 | 6.41 | 199.08 | 0.3221 | -813.0 | -547.4 | |
| 1.71 | 284.40 | 0.91 | 151.72 | -24.35 | 192.32 | 3.20 | 187.74 | 0.3790 | 659.8 | 407.3 | |
| 17.70 | -2.00 | 9.44 | -2.00 | -23.86 | 192.28 | 3.15 | 187.82 | 0.3711 | 1359.5 | 999999 | |
| 20.94 | -2.00 | 11.18 | -2.00 | -24.16 | 191.92 | 2.79 | 186.84 | 0.3750 | 1161.8 | 999999 | |
| 7.46 | -2.00 | 3.97 | -2.00 | -23.80 | 191.91 | 2.79 | 186.95 | 0.3692 | 1461.2 | 999999 | |
| 2.52 | -2.00 | 1.34 | -2.00 | -23.83 | 191.25 | 2.12 | 185.30 | 0.3686 | 918.7 | 999999 | |
| 0.00 | 4.40 | 0.00 | 2.31 | -21.41 | 191.15 | 2.02 | 185.76 | 0.3289 | -889.0 | -682.9 | |
| 0.00 | 0.99 | 0.00 | 0.52 | -22.86 | 190.61 | 1.48 | 183.90 | 0.3519 | -513.0 | -391.2 | |
| 0.00 | 1.44 | 0.00 | 0.76 | -23.73 | 187.60 | -1.52 | 176.18 | 0.3662 | -764.0 | -723.9 | |
| 0.00 | 1.71 | 0.00 | 0.93 | -26.82 | 185.96 | -3.16 | 173.21 | 0.4182 | -686.0 | -556.5 | |
| 0.00 | 1.08 | 0.00 | 0.61 | -30.27 | 185.71 | -3.41 | 173.72 | 0.4723 | -676.0 | -477.2 | |
| 0.00 | 2.79 | 0.00 | 1.51 | -26.49 | 185.67 | -3.46 | 172.47 | 0.4135 | -898.0 | -808.5 | |
| 0.00 | 1.44 | 0.00 | 0.78 | -26.95 | 185.51 | -3.61 | 172.31 | 0.4212 | -994.0 | -734.6 | |
| 0.00 | 1.71 | 0.00 | 0.93 | -27.32 | 185.33 | -3.79 | 172.06 | 0.4273 | -903.0 | -738.5 | |
| 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. | |