SDO HMI 2011-10-14 17:59:02 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 13.71 | 59.75 | 7.99 | 34.75 | 19.89 | 98.32 | 29.11 | 299.12 | 0.5254 | -268.8 | -290.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.05 | 0.00 | 0.62 | 19.64 | 99.84 | 30.63 | 297.57 | 0.5435 | -203.0 | -182.5 | |
| 3.58 | 4.89 | 2.12 | 2.89 | 20.25 | 99.94 | 30.73 | 298.57 | 0.5480 | -689.8 | -555.1 | |
| 0.00 | 0.96 | 0.00 | 0.57 | 20.13 | 99.84 | 30.63 | 298.43 | 0.5461 | -596.0 | -597.3 | |
| 1.57 | 33.54 | 0.92 | 19.67 | 19.59 | 99.58 | 30.36 | 297.66 | 0.5398 | -853.4 | -584.4 | |
| 4.02 | -4.00 | 2.36 | -4.00 | 19.51 | 99.41 | 30.20 | 297.61 | 0.5372 | -1097.3 | 999999 | |
| 0.00 | 1.31 | 0.00 | 0.77 | 20.18 | 99.48 | 30.27 | 298.74 | 0.5417 | -716.0 | -560.7 | |
| 1.40 | -4.00 | 0.82 | -4.00 | 19.61 | 99.25 | 30.04 | 297.89 | 0.5356 | -1070.5 | 999999 | |
| 0.00 | 0.70 | 0.00 | 0.41 | 20.10 | 99.24 | 30.03 | 298.76 | 0.5382 | -675.0 | -617.4 | |
| 0.00 | 1.75 | 0.00 | 1.02 | 19.80 | 98.45 | 29.24 | 298.76 | 0.5263 | -829.0 | -620.5 | |
| 0.00 | 1.75 | 0.00 | 1.00 | 19.08 | 96.65 | 27.44 | 298.72 | 0.4986 | -690.0 | -478.8 | |
| 0.00 | 1.22 | 0.00 | 0.70 | 21.13 | 96.00 | 26.79 | 302.95 | 0.5030 | 707.0 | 643.9 | |
| 0.00 | 1.92 | 0.00 | 1.10 | 20.94 | 95.96 | 26.75 | 302.65 | 0.5013 | 1011.0 | 801.2 | |
| 0.00 | 2.27 | 0.00 | 1.28 | 20.26 | 94.59 | 25.38 | 302.57 | 0.4791 | 784.0 | 581.0 | |
| 3.14 | 6.99 | 1.77 | 3.94 | 20.75 | 94.50 | 25.29 | 303.58 | 0.4815 | 796.1 | 724.5 | |
| 0.00 | 1.40 | 0.00 | 0.78 | 20.58 | 93.59 | 24.38 | 304.09 | 0.4685 | 677.0 | 451.6 | |
| 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. | |