SDO HMI 2011-11-13 06:58:58 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 11.02 | 42.94 | 8.98 | 34.51 | 8.52 | 347.68 | -51.95 | 81.60 | 0.7891 | 184.9 | 163.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.29 | 4.30 | 1.00 | 3.32 | 8.34 | 349.51 | -50.13 | 81.71 | 0.7697 | -649.9 | -429.3 | |
| 0.00 | 4.56 | 0.00 | 3.51 | 7.81 | 349.60 | -50.04 | 82.40 | 0.7684 | -623.0 | -470.1 | |
| 0.00 | 0.52 | 0.00 | 0.40 | 7.45 | 349.56 | -50.07 | 82.87 | 0.7686 | -290.0 | -361.3 | |
| 0.00 | 1.38 | 0.00 | 1.09 | 9.11 | 348.51 | -51.13 | 80.79 | 0.7811 | -376.0 | -286.9 | |
| 5.94 | 17.13 | 4.70 | 13.55 | 8.29 | 348.37 | -51.26 | 81.84 | 0.7821 | 802.6 | 589.4 | |
| 1.29 | 1.89 | 1.03 | 1.50 | 9.16 | 348.21 | -51.43 | 80.75 | 0.7843 | -340.7 | -232.1 | |
| 0.00 | 0.69 | 0.00 | 0.55 | 8.78 | 347.79 | -51.84 | 81.26 | 0.7885 | 494.0 | 393.0 | |
| 0.00 | 1.12 | 0.00 | 0.91 | 9.18 | 347.22 | -52.41 | 80.80 | 0.7948 | 677.0 | 602.0 | |
| 0.00 | 3.53 | 0.00 | 2.88 | 9.28 | 346.95 | -52.68 | 80.68 | 0.7977 | 640.0 | 541.3 | |
| 0.00 | 0.86 | 0.00 | 0.70 | 7.56 | 347.14 | -52.50 | 82.84 | 0.7949 | -504.0 | -448.8 | |
| 0.00 | 1.29 | 0.00 | 1.07 | 8.86 | 346.23 | -53.40 | 81.25 | 0.8048 | 230.0 | 215.3 | |
| 0.00 | 1.03 | 0.00 | 0.86 | 7.49 | 346.20 | -53.44 | 82.97 | 0.8046 | -474.0 | -373.1 | |
| 0.00 | 0.77 | 0.00 | 0.67 | 9.41 | 344.40 | -55.24 | 80.68 | 0.8235 | -341.0 | -246.6 | |
| 2.50 | 3.87 | 2.25 | 3.50 | 9.29 | 342.91 | -56.72 | 80.91 | 0.8377 | 580.1 | 344.0 | |
| 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. | |