| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 27.11 | 63.47 | 17.49 | 41.33 | 20.11 | 64.90 | -30.92 | 48.01 | 0.6507 | -102.5 | 231.5 | |
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back to the solar disc SDO HMI 2011-02-09 10:58:56 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 8.47 | 23.61 | 5.36 | 14.97 | 19.68 | 67.24 | -28.58 | 46.42 | 0.6240 | -873.9 | -652.0 | |
| 2.99 | -1.00 | 1.90 | -1.00 | 19.53 | 66.91 | -28.91 | 46.92 | 0.6260 | -842.7 | 999999 | |
| 5.56 | -1.00 | 3.54 | -1.00 | 19.77 | 66.75 | -29.06 | 46.78 | 0.6297 | -751.8 | 999999 | |
| 0.00 | 3.76 | 0.00 | 2.41 | 20.13 | 66.25 | -29.57 | 46.82 | 0.6377 | -645.0 | -554.9 | |
| 0.00 | 0.86 | 0.00 | 0.54 | 19.20 | 66.40 | -29.42 | 47.82 | 0.6283 | -669.0 | -583.7 | |
| 0.00 | 1.20 | 0.00 | 0.77 | 20.35 | 65.87 | -29.94 | 46.90 | 0.6433 | -558.0 | -433.0 | |
| 4.19 | 8.30 | 2.77 | 5.48 | 20.88 | 64.28 | -31.54 | 47.70 | 0.6631 | 837.8 | 695.0 | |
| 0.00 | 1.28 | 0.00 | 0.85 | 21.26 | 64.00 | -31.82 | 47.49 | 0.6688 | 487.0 | 391.3 | |
| 2.05 | 11.03 | 1.36 | 7.31 | 20.48 | 63.74 | -32.08 | 48.64 | 0.6652 | 916.1 | 697.5 | |
| 0.00 | 2.14 | 0.00 | 1.42 | 20.31 | 63.29 | -32.52 | 49.22 | 0.6682 | 855.0 | 654.9 | |
| 0.00 | 1.03 | 0.00 | 0.68 | 19.84 | 63.03 | -32.79 | 50.02 | 0.6671 | 797.0 | 607.2 | |
| 2.22 | 8.04 | 1.48 | 5.34 | 19.75 | 62.79 | -33.03 | 50.32 | 0.6689 | 831.7 | 660.5 | |
| 1.63 | -12.00 | 1.08 | -12.00 | 19.60 | 62.63 | -33.18 | 50.63 | 0.6692 | 756.3 | 999999 | |
| 0.00 | 2.22 | 0.00 | 1.56 | 20.75 | 59.34 | -36.48 | 51.80 | 0.7099 | 556.0 | 440.8 | |
| 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. | |