SDO HMI 2013-08-23 01:59:08 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 47.71 | 288.81 | 26.57 | 160.65 | -6.99 | 139.36 | 23.20 | 239.34 | 0.4565 | 742.3 | 374.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.90 | 0.00 | 0.51 | -5.68 | 141.77 | 25.61 | 244.25 | 0.4794 | -583.0 | -435.1 | |
| 46.81 | 270.28 | 26.06 | 150.42 | -6.90 | 139.51 | 23.35 | 239.68 | 0.4577 | 1267.9 | 411.3 | |
| 0.00 | 1.35 | 0.00 | 0.76 | -9.48 | 139.57 | 23.41 | 235.08 | 0.4799 | 561.0 | 460.0 | |
| 0.45 | 1.44 | 0.25 | 0.81 | -9.40 | 138.73 | 22.57 | 234.21 | 0.4687 | 741.2 | 609.1 | |
| 0.45 | 1.53 | 0.26 | 0.89 | -15.92 | 138.46 | 22.29 | 223.80 | 0.5292 | -721.8 | -598.4 | |
| 0.00 | 3.32 | 0.00 | 1.82 | -7.31 | 137.06 | 20.90 | 235.95 | 0.4288 | 889.0 | 848.3 | |
| 0.00 | 0.99 | 0.00 | 0.54 | -7.81 | 136.92 | 20.76 | 234.82 | 0.4314 | 811.0 | 757.0 | |
| 0.00 | 1.53 | 0.00 | 0.84 | -7.64 | 136.62 | 20.46 | 234.74 | 0.4260 | -659.0 | -518.0 | |
| 0.00 | 1.26 | 0.00 | 0.69 | -7.19 | 136.43 | 20.27 | 235.36 | 0.4195 | -796.0 | -614.2 | |
| 0.00 | 1.62 | 0.00 | 0.88 | -7.09 | 136.13 | 19.97 | 235.17 | 0.4147 | -1013.0 | -851.8 | |
| 0.00 | 0.63 | 0.00 | 0.35 | -10.28 | 135.75 | 19.59 | 228.70 | 0.4410 | -564.0 | -506.3 | |
| 0.00 | 1.71 | 0.00 | 0.92 | -5.49 | 135.33 | 19.17 | 237.35 | 0.3898 | -767.0 | -575.2 | |
| 0.00 | 1.08 | 0.00 | 0.59 | -10.10 | 135.28 | 19.12 | 228.32 | 0.4337 | -712.0 | -557.8 | |
| 0.00 | 1.17 | 0.00 | 0.63 | -5.45 | 134.91 | 18.75 | 236.86 | 0.3837 | -853.0 | -655.8 | |
| 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. | |