SDO HMI 2011-10-19 16:02:01 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 13.59 | 48.18 | 7.16 | 25.38 | -14.19 | 3.29 | -1.04 | 176.93 | 0.3414 | -171.3 | -244.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 3.22 | 4.09 | 1.70 | 2.16 | -14.85 | 6.28 | 1.94 | 185.37 | 0.3515 | 877.8 | 582.3 | |
| 3.05 | 11.67 | 1.61 | 6.17 | -14.76 | 6.06 | 1.72 | 184.79 | 0.3496 | 1129.6 | 713.6 | |
| 0.35 | -2.00 | 0.18 | -2.00 | -14.66 | 5.90 | 1.57 | 184.39 | 0.3479 | 1062.8 | 999999 | |
| 0.00 | 1.22 | 0.00 | 0.64 | -12.89 | 5.62 | 1.28 | 183.94 | 0.3183 | 1012.0 | 685.9 | |
| 0.00 | 1.39 | 0.00 | 0.73 | -14.37 | 5.16 | 0.83 | 182.35 | 0.3424 | 973.0 | 743.2 | |
| 0.00 | 1.05 | 0.00 | 0.55 | -13.33 | 2.67 | -1.66 | 175.02 | 0.3261 | -722.0 | -532.9 | |
| 0.00 | 1.05 | 0.00 | 0.55 | -14.89 | 2.29 | -2.04 | 174.36 | 0.3522 | -646.0 | -491.1 | |
| 0.00 | 1.48 | 0.00 | 0.78 | -13.27 | 2.09 | -2.24 | 173.26 | 0.3261 | -1047.0 | -795.0 | |
| 0.00 | 1.13 | 0.00 | 0.60 | -14.15 | 2.05 | -2.28 | 173.46 | 0.3407 | -855.0 | -623.1 | |
| 2.53 | 7.23 | 1.33 | 3.81 | -14.38 | 1.96 | -2.38 | 173.27 | 0.3445 | -936.5 | -787.1 | |
| 0.00 | 3.31 | 0.00 | 1.74 | -13.55 | 1.97 | -2.37 | 173.00 | 0.3310 | -623.0 | -678.5 | |
| 0.00 | 1.92 | 0.00 | 1.01 | -13.71 | 1.81 | -2.52 | 172.61 | 0.3339 | -1124.0 | -898.1 | |
| 0.00 | 3.14 | 0.00 | 1.65 | -14.00 | 1.50 | -2.84 | 171.83 | 0.3393 | -957.0 | -790.6 | |
| 4.44 | 9.50 | 2.34 | 4.99 | -13.78 | 0.98 | -3.36 | 170.25 | 0.3371 | -969.8 | -724.9 | |
| 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. | |