SDO HMI 2014-05-29 02:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 32.14 | 65.27 | 17.40 | 35.28 | -19.35 | 51.31 | 14.91 | 217.48 | 0.4016 | 330.9 | 245.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.17 | 0.00 | 0.62 | -11.88 | 53.31 | 16.91 | 236.44 | 0.3430 | 805.0 | 686.2 | |
| 0.00 | 1.90 | 0.00 | 1.03 | -18.59 | 53.64 | 17.24 | 222.89 | 0.4144 | 824.0 | 710.0 | |
| 0.00 | 1.44 | 0.00 | 0.77 | -14.74 | 53.25 | 16.85 | 229.72 | 0.3691 | 679.0 | 565.5 | |
| 22.21 | 31.78 | 12.09 | 17.30 | -19.20 | 53.23 | 16.83 | 221.19 | 0.4169 | 1026.6 | 762.4 | |
| 0.00 | 1.99 | 0.00 | 1.08 | -19.43 | 52.38 | 15.98 | 219.40 | 0.4107 | 866.0 | 673.2 | |
| 0.00 | 0.72 | 0.00 | 0.39 | -19.88 | 51.05 | 14.65 | 216.33 | 0.4032 | -689.0 | -544.1 | |
| 0.00 | 3.25 | 0.00 | 1.76 | -20.66 | 50.86 | 14.46 | 214.79 | 0.4111 | 847.0 | 734.4 | |
| 0.00 | 1.72 | 0.00 | 0.93 | -20.75 | 50.10 | 13.69 | 213.24 | 0.4056 | 579.0 | 513.5 | |
| 0.00 | 1.53 | 0.00 | 0.83 | -21.18 | 49.40 | 13.00 | 211.32 | 0.4051 | 627.0 | 363.5 | |
| 3.07 | 15.98 | 1.64 | 8.55 | -19.57 | 49.00 | 12.60 | 212.86 | 0.3803 | -948.7 | -782.2 | |
| 6.86 | -10.00 | 3.67 | -10.00 | -19.82 | 48.72 | 12.32 | 211.91 | 0.3813 | -997.4 | 999999 | |
| 0.00 | 1.81 | 0.00 | 0.96 | -19.48 | 46.39 | 9.99 | 207.34 | 0.3578 | -637.0 | -502.6 | |
| 0.00 | 0.99 | 0.00 | 0.53 | -21.93 | 42.32 | 5.92 | 195.02 | 0.3709 | -863.0 | -727.2 | |
| 0.00 | 0.99 | 0.00 | 0.53 | -21.87 | 42.19 | 5.79 | 194.74 | 0.3693 | -836.0 | -701.4 | |
| 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. | |