SDO HMI 2011-12-13 00:58:55 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 3.49 | 18.22 | 2.22 | 11.52 | 7.80 | 45.19 | 37.66 | 283.39 | 0.6241 | -385.5 | -278.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.36 | 0.00 | 0.89 | 7.58 | 47.49 | 39.97 | 282.38 | 0.6543 | -551.0 | -463.9 | |
| 0.00 | 1.02 | 0.00 | 0.66 | 7.73 | 47.12 | 39.60 | 282.71 | 0.6498 | -609.0 | -448.8 | |
| 0.00 | 0.85 | 0.00 | 0.55 | 8.18 | 47.02 | 39.49 | 283.41 | 0.6495 | -532.0 | -504.2 | |
| 1.79 | 3.07 | 1.15 | 1.98 | 7.84 | 46.67 | 39.14 | 283.01 | 0.6442 | -702.9 | -655.5 | |
| 0.00 | 0.34 | 0.00 | 0.22 | 8.44 | 46.66 | 39.14 | 283.92 | 0.6456 | -506.0 | -629.2 | |
| 0.00 | 0.94 | 0.00 | 0.60 | 8.44 | 46.28 | 38.75 | 284.03 | 0.6406 | -780.0 | -662.7 | |
| 0.00 | 0.51 | 0.00 | 0.33 | 7.90 | 46.14 | 38.61 | 283.24 | 0.6374 | -598.0 | -484.5 | |
| 0.51 | 1.36 | 0.33 | 0.87 | 7.63 | 45.77 | 38.24 | 282.93 | 0.6318 | -870.8 | -790.2 | |
| 0.00 | 1.53 | 0.00 | 0.97 | 7.87 | 45.41 | 37.89 | 283.40 | 0.6277 | -786.0 | -591.0 | |
| 0.00 | 0.85 | 0.00 | 0.54 | 7.75 | 45.29 | 37.76 | 283.25 | 0.6257 | -628.0 | -595.1 | |
| 0.00 | 1.62 | 0.00 | 1.01 | 7.89 | 44.51 | 36.99 | 283.72 | 0.6157 | -536.0 | -417.2 | |
| 1.19 | 2.47 | 0.74 | 1.52 | 7.55 | 43.37 | 35.84 | 283.54 | 0.5993 | 686.0 | 670.9 | |
| 0.00 | 1.11 | 0.00 | 0.67 | 7.84 | 41.25 | 33.72 | 284.76 | 0.5710 | 727.0 | 573.4 | |
| 0.00 | 1.19 | 0.00 | 0.71 | 7.39 | 40.57 | 33.04 | 284.24 | 0.5600 | 776.0 | 659.4 | |
| 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. | |