SDO HMI 2011-11-09 11:58:58 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 36.29 | 75.43 | 19.66 | 40.79 | -17.73 | 100.28 | 10.64 | 205.86 | 0.4040 | 245.8 | -110.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.86 | 0.00 | 0.47 | -18.39 | 102.35 | 12.72 | 209.33 | 0.4282 | 645.0 | 445.9 | |
| 29.05 | 46.03 | 15.79 | 25.01 | -17.99 | 101.18 | 11.54 | 207.50 | 0.4138 | 985.0 | 518.8 | |
| 0.00 | 0.95 | 0.00 | 0.51 | -17.86 | 100.59 | 10.95 | 206.46 | 0.4076 | 490.0 | 409.9 | |
| 0.00 | 2.33 | 0.00 | 1.25 | -17.03 | 100.39 | 10.75 | 207.00 | 0.3944 | -814.0 | -564.5 | |
| 0.00 | 1.12 | 0.00 | 0.60 | -17.27 | 99.17 | 9.53 | 204.06 | 0.3894 | -687.0 | -530.7 | |
| 0.00 | 1.12 | 0.00 | 0.60 | -17.20 | 98.97 | 9.34 | 203.70 | 0.3872 | -905.0 | -722.5 | |
| 0.00 | 0.95 | 0.00 | 0.51 | -17.58 | 98.90 | 9.26 | 203.13 | 0.3923 | -735.0 | -613.6 | |
| 0.00 | 2.76 | 0.00 | 1.48 | -17.42 | 98.77 | 9.13 | 202.99 | 0.3891 | -976.0 | -867.7 | |
| 1.81 | 9.22 | 0.97 | 4.97 | -17.64 | 98.75 | 9.11 | 202.72 | 0.3922 | -836.4 | -629.1 | |
| 1.90 | -9.00 | 1.02 | -9.00 | -17.84 | 98.72 | 9.08 | 202.47 | 0.3949 | -740.1 | 999999 | |
| 0.00 | 2.07 | 0.00 | 1.11 | -17.23 | 98.69 | 9.05 | 203.03 | 0.3858 | -1127.0 | -788.8 | |
| 0.00 | 1.81 | 0.00 | 0.97 | -17.10 | 98.18 | 8.54 | 202.00 | 0.3807 | -1066.0 | -821.9 | |
| 3.53 | 6.21 | 1.88 | 3.31 | -16.65 | 97.94 | 8.30 | 201.90 | 0.3726 | -939.9 | -666.5 | |
| 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. | |