SDO HMI 2011-08-08 02:59:10 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 19.98 | 0.00 | 10.68 | 19.89 | 224.59 | -17.62 | 49.40 | 0.3747 | -639.6 | -555.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.99 | 0.00 | 1.04 | 18.66 | 226.81 | -15.40 | 49.00 | 0.3348 | -970.0 | -740.0 | |
| 0.00 | 0.90 | 0.00 | 0.48 | 18.96 | 226.49 | -15.73 | 48.85 | 0.3420 | -827.0 | -598.4 | |
| 0.00 | 2.17 | 0.00 | 1.15 | 19.52 | 226.36 | -15.85 | 47.78 | 0.3491 | -870.0 | -689.0 | |
| 0.00 | 1.63 | 0.00 | 0.86 | 18.80 | 226.27 | -15.95 | 49.60 | 0.3430 | -867.0 | -790.2 | |
| 0.00 | 0.90 | 0.00 | 0.48 | 19.51 | 225.96 | -16.25 | 48.48 | 0.3539 | -1076.0 | -878.4 | |
| 0.00 | 1.27 | 0.00 | 0.67 | 19.13 | 225.87 | -16.35 | 49.49 | 0.3513 | -1037.0 | -924.1 | |
| 0.00 | 2.53 | 0.00 | 1.35 | 21.03 | 225.46 | -16.76 | 46.03 | 0.3755 | -967.0 | -745.5 | |
| 0.00 | 0.45 | 0.00 | 0.24 | 21.38 | 225.35 | -16.87 | 45.51 | 0.3804 | -585.0 | -538.8 | |
| 0.00 | 2.08 | 0.00 | 1.11 | 20.03 | 225.47 | -16.75 | 48.14 | 0.3651 | -870.0 | -586.2 | |
| 0.00 | 1.36 | 0.00 | 0.73 | 21.27 | 225.02 | -17.20 | 46.24 | 0.3831 | -629.0 | -491.9 | |
| 0.00 | 1.27 | 0.00 | 0.67 | 20.24 | 225.07 | -17.14 | 48.31 | 0.3720 | -943.0 | -799.3 | |
| 0.00 | 1.27 | 0.00 | 0.67 | 18.30 | 224.14 | -18.08 | 54.01 | 0.3657 | -875.0 | -718.0 | |
| 0.00 | 1.17 | 0.00 | 0.66 | 20.81 | 216.86 | -25.35 | 56.87 | 0.4799 | 731.0 | 628.6 | |
| 0.00 | 0.99 | 0.00 | 0.57 | 21.55 | 214.49 | -27.72 | 57.51 | 0.5150 | 830.0 | 663.7 | |
| 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. | |