SDO HMI 2011-10-08 17:59:02 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 41.37 | 246.45 | 21.57 | 128.57 | 23.41 | 155.02 | 6.65 | 340.13 | 0.3150 | -945.3 | -395.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.19 | 0.00 | 1.15 | 24.42 | 157.23 | 8.87 | 335.77 | 0.3434 | -799.0 | -659.7 | |
| 0.00 | 2.63 | 0.00 | 1.41 | 27.71 | 156.26 | 7.89 | 341.61 | 0.3869 | -627.0 | -582.8 | |
| 0.00 | 1.67 | 0.00 | 0.89 | 26.69 | 155.81 | 7.45 | 341.64 | 0.3692 | -781.0 | -615.3 | |
| 9.38 | 223.93 | 4.89 | 116.74 | 23.06 | 155.53 | 7.16 | 338.33 | 0.3121 | -1307.1 | -420.0 | |
| 30.76 | -4.00 | 16.04 | -4.00 | 23.29 | 155.15 | 6.78 | 339.65 | 0.3133 | -1471.2 | 999999 | |
| 0.00 | 1.31 | 0.00 | 0.70 | 26.52 | 154.42 | 6.05 | 344.73 | 0.3599 | -707.0 | -476.5 | |
| 0.00 | 2.28 | 0.00 | 1.18 | 22.96 | 152.94 | 4.58 | 345.63 | 0.2972 | 689.0 | 552.5 | |
| 0.00 | 2.80 | 0.00 | 1.46 | 24.22 | 152.82 | 4.45 | 347.03 | 0.3170 | -825.0 | -695.7 | |
| 0.00 | 0.70 | 0.00 | 0.37 | 25.23 | 152.79 | 4.42 | 347.85 | 0.3332 | -695.0 | -476.1 | |
| 1.23 | 2.28 | 0.64 | 1.19 | 24.73 | 152.51 | 4.14 | 348.27 | 0.3241 | -818.5 | -672.0 | |
| 0.00 | 1.40 | 0.00 | 0.73 | 24.41 | 151.94 | 3.57 | 349.65 | 0.3172 | -756.0 | -563.6 | |
| 0.00 | 0.88 | 0.00 | 0.46 | 23.67 | 151.03 | 2.67 | 351.86 | 0.3025 | 777.0 | 663.8 | |
| 0.00 | 1.75 | 0.00 | 0.91 | 24.30 | 148.06 | -0.31 | 0.91 | 0.3100 | 892.0 | 660.2 | |
| 0.00 | 1.84 | 0.00 | 0.97 | 26.33 | 147.65 | -0.71 | 1.87 | 0.3437 | 801.0 | 566.9 | |
| 0.00 | 0.79 | 0.00 | 0.41 | 25.34 | 147.33 | -1.04 | 2.88 | 0.3277 | 810.0 | 628.1 | |
| 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. | |