SDO HMI 2011-08-18 04:59:09 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 13.95 | 38.80 | 7.64 | 21.29 | -18.04 | 114.00 | 5.08 | 191.27 | 0.4302 | -342.2 | -336.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 2.34 | 4.59 | 1.30 | 2.55 | -18.61 | 117.21 | 8.29 | 197.73 | 0.4507 | 928.8 | 838.4 | |
| 0.00 | 0.99 | 0.00 | 0.55 | -18.52 | 116.27 | 7.35 | 195.88 | 0.4452 | 808.0 | 672.9 | |
| 0.00 | 1.62 | 0.00 | 0.90 | -19.23 | 116.24 | 7.32 | 195.37 | 0.4557 | 467.0 | 480.9 | |
| 1.26 | 2.34 | 0.69 | 1.29 | -18.27 | 115.39 | 6.47 | 194.21 | 0.4379 | 581.9 | 651.4 | |
| 1.35 | 3.78 | 0.74 | 2.07 | -17.65 | 113.80 | 4.88 | 191.10 | 0.4228 | -866.3 | -826.4 | |
| 1.71 | 3.42 | 0.94 | 1.87 | -17.92 | 113.55 | 4.63 | 190.43 | 0.4262 | -777.8 | -758.4 | |
| 0.00 | 1.08 | 0.00 | 0.59 | -17.42 | 113.48 | 4.55 | 190.48 | 0.4182 | -888.0 | -779.2 | |
| 0.00 | 5.85 | 0.00 | 3.22 | -18.62 | 113.41 | 4.49 | 189.82 | 0.4367 | -721.0 | -724.1 | |
| 0.00 | 0.99 | 0.00 | 0.54 | -18.25 | 113.37 | 4.45 | 189.88 | 0.4309 | -917.0 | -778.0 | |
| 5.22 | 8.11 | 2.85 | 4.43 | -17.68 | 113.32 | 4.40 | 190.02 | 0.4219 | -1019.4 | -660.4 | |
| 2.07 | 2.97 | 1.12 | 1.61 | -16.98 | 113.15 | 4.23 | 189.93 | 0.4104 | 612.7 | 507.5 | |
| 0.00 | 1.17 | 0.00 | 0.64 | -17.70 | 111.22 | 2.30 | 185.26 | 0.4177 | -814.0 | -686.5 | |
| 0.00 | 0.90 | 0.00 | 0.49 | -18.43 | 111.03 | 2.11 | 184.70 | 0.4291 | -611.0 | -554.7 | |
| 0.00 | 0.99 | 0.00 | 0.54 | -17.53 | 110.58 | 1.66 | 183.83 | 0.4142 | -693.0 | -556.1 | |
| 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. | |