SDO HMI 2011-10-05 19:59:03 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 35.65 | 198.51 | 18.72 | 104.37 | -11.51 | 179.14 | -7.71 | 157.04 | 0.3369 | 558.7 | 354.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.67 | 180.34 | 0.88 | 94.66 | -11.74 | 179.71 | -7.13 | 158.73 | 0.3365 | 840.4 | 450.7 | |
| 33.63 | -1.00 | 17.65 | -1.00 | -11.40 | 179.51 | -7.34 | 157.78 | 0.3325 | 1269.6 | 999999 | |
| 0.00 | 2.28 | 0.00 | 1.20 | -11.82 | 178.57 | -8.28 | 155.79 | 0.3450 | 871.0 | 598.5 | |
| 0.00 | 1.93 | 0.00 | 1.02 | -11.98 | 178.50 | -8.34 | 155.80 | 0.3478 | 651.0 | 508.4 | |
| 0.00 | 2.81 | 0.00 | 1.49 | -12.42 | 176.96 | -9.88 | 152.56 | 0.3652 | -877.0 | -643.8 | |
| 0.00 | 1.32 | 0.00 | 0.70 | -12.62 | 176.68 | -10.17 | 152.13 | 0.3701 | -1122.0 | -874.0 | |
| 0.00 | 1.14 | 0.00 | 0.62 | -14.00 | 174.57 | -12.27 | 149.33 | 0.4061 | -807.0 | -584.7 | |
| 0.00 | 1.05 | 0.00 | 0.57 | -12.48 | 174.40 | -12.45 | 146.89 | 0.3869 | -837.0 | -705.2 | |
| 0.00 | 0.88 | 0.00 | 0.47 | -12.34 | 173.84 | -13.01 | 145.52 | 0.3900 | -873.0 | -682.5 | |
| 0.00 | 3.42 | 0.00 | 1.84 | -12.28 | 173.62 | -13.22 | 144.98 | 0.3912 | -1150.0 | -856.4 | |
| 0.35 | 1.32 | 0.19 | 0.71 | -12.66 | 173.50 | -13.34 | 145.32 | 0.3973 | -943.2 | -760.9 | |
| 0.00 | 0.35 | 0.00 | 0.19 | -14.07 | 173.42 | -13.42 | 147.13 | 0.4165 | -525.0 | -526.8 | |
| 0.00 | 1.67 | 0.00 | 0.90 | -12.45 | 172.25 | -14.59 | 142.55 | 0.4063 | -751.0 | -504.2 | |
| 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. | |