SDO HMI 2011-10-06 18:59:03 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 35.97 | 167.59 | 18.81 | 87.68 | -11.35 | 179.82 | 5.62 | 197.46 | 0.3226 | 508.4 | 319.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 32.55 | 151.26 | 17.03 | 79.12 | -11.25 | 180.38 | 6.18 | 199.19 | 0.3225 | 1225.2 | 434.4 | |
| 2.02 | -1.00 | 1.05 | -1.00 | -11.24 | 179.92 | 5.72 | 197.86 | 0.3200 | 933.3 | 999999 | |
| 0.00 | 1.32 | 0.00 | 0.70 | -13.42 | 179.62 | 5.42 | 195.16 | 0.3531 | 757.0 | 496.7 | |
| 1.40 | 2.11 | 0.73 | 1.10 | -11.42 | 179.52 | 5.32 | 196.52 | 0.3210 | 856.3 | 797.4 | |
| 0.00 | 0.79 | 0.00 | 0.41 | -8.99 | 175.74 | 1.54 | 185.71 | 0.2686 | -793.0 | -564.3 | |
| 0.00 | 1.58 | 0.00 | 0.83 | -12.63 | 174.54 | 0.33 | 181.00 | 0.3283 | -971.0 | -728.1 | |
| 0.00 | 0.70 | 0.00 | 0.37 | -12.63 | 174.38 | 0.18 | 180.54 | 0.3282 | -1164.0 | -886.0 | |
| 0.00 | 1.14 | 0.00 | 0.60 | -13.77 | 173.89 | -0.31 | 179.12 | 0.3472 | -875.0 | -657.5 | |
| 0.00 | 2.46 | 0.00 | 1.29 | -12.60 | 173.49 | -0.71 | 177.88 | 0.3279 | -850.0 | -701.0 | |
| 0.00 | 1.93 | 0.00 | 1.01 | -12.34 | 173.40 | -0.80 | 177.57 | 0.3238 | -954.0 | -805.4 | |
| 0.00 | 1.58 | 0.00 | 0.83 | -12.25 | 173.25 | -0.95 | 177.09 | 0.3223 | -944.0 | -786.5 | |
| 0.00 | 1.67 | 0.00 | 0.87 | -12.12 | 173.06 | -1.14 | 176.51 | 0.3204 | -1183.0 | -994.5 | |
| 0.00 | 1.05 | 0.00 | 0.55 | -12.03 | 172.88 | -1.32 | 175.93 | 0.3190 | -845.0 | -631.4 | |
| 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. | |