SDO HMI 2011-11-10 05:58:58 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 55.08 | 347.20 | 29.89 | 188.38 | 9.51 | 56.40 | -23.33 | 74.20 | 0.4076 | -856.1 | -372.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 42.67 | 300.06 | 23.04 | 162.24 | 9.38 | 56.87 | -22.86 | 74.25 | 0.4000 | -1376.6 | -429.3 | |
| 1.72 | 2.41 | 0.93 | 1.31 | 10.96 | 56.72 | -23.01 | 70.55 | 0.4088 | -783.3 | -629.6 | |
| 1.38 | 1.55 | 0.75 | 0.84 | 10.38 | 56.17 | -23.56 | 72.27 | 0.4145 | -629.3 | -709.0 | |
| 2.93 | -1.00 | 1.59 | -1.00 | 9.72 | 56.13 | -23.61 | 73.85 | 0.4127 | -675.0 | 999999 | |
| 0.00 | 1.98 | 0.00 | 1.09 | 12.17 | 55.75 | -23.98 | 68.46 | 0.4290 | -762.0 | -612.2 | |
| 0.00 | 9.14 | 0.00 | 4.98 | 10.58 | 55.86 | -23.87 | 71.99 | 0.4201 | -340.0 | -461.8 | |
| 0.00 | 3.28 | 0.00 | 1.79 | 9.10 | 55.22 | -24.52 | 75.76 | 0.4245 | -801.0 | -566.9 | |
| 0.00 | 1.72 | 0.00 | 0.94 | 8.62 | 55.05 | -24.68 | 76.95 | 0.4256 | 162.0 | 301.0 | |
| 0.00 | 1.90 | 0.00 | 1.05 | 12.46 | 54.15 | -25.59 | 68.92 | 0.4538 | 808.0 | 634.3 | |
| 1.81 | 12.24 | 1.00 | 6.73 | 8.63 | 54.32 | -25.41 | 77.23 | 0.4369 | 969.7 | 527.0 | |
| 0.00 | 1.38 | 0.00 | 0.76 | 9.10 | 54.15 | -25.58 | 76.23 | 0.4408 | 791.0 | 587.7 | |
| 0.00 | 1.03 | 0.00 | 0.58 | 9.59 | 52.36 | -27.37 | 75.91 | 0.4693 | -981.0 | -788.0 | |
| 4.57 | 5.60 | 2.58 | 3.16 | 10.11 | 51.67 | -28.07 | 75.11 | 0.4813 | -899.3 | -724.2 | |
| 0.00 | 1.21 | 0.00 | 0.70 | 14.03 | 49.77 | -29.96 | 68.42 | 0.5231 | 591.0 | 432.6 | |
| 0.00 | 1.29 | 0.00 | 0.75 | 10.76 | 49.24 | -30.49 | 74.78 | 0.5187 | -487.0 | -440.1 | |
| 0.00 | 1.72 | 0.00 | 1.04 | 13.19 | 45.97 | -33.76 | 71.68 | 0.5722 | 761.0 | 590.1 | |
| 0.00 | 0.69 | 0.00 | 0.42 | 10.99 | 44.23 | -35.50 | 75.98 | 0.5899 | 591.0 | 476.2 | |
| 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. | |