SDO HMI 2011-11-14 16:58:58 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 27.23 | 216.15 | 16.00 | 126.94 | 28.26 | 42.25 | 21.28 | 323.43 | 0.5386 | -787.7 | -420.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.89 | 206.18 | 1.11 | 121.16 | 28.12 | 42.75 | 21.78 | 322.64 | 0.5415 | -1037.1 | -443.4 | |
| 9.88 | -1.00 | 5.82 | -1.00 | 28.39 | 42.48 | 21.51 | 323.30 | 0.5420 | -1108.3 | 999999 | |
| 11.60 | -1.00 | 6.80 | -1.00 | 28.03 | 42.37 | 21.40 | 322.98 | 0.5371 | -1379.3 | 999999 | |
| 0.77 | -1.00 | 0.45 | -1.00 | 28.33 | 42.04 | 21.07 | 323.77 | 0.5375 | -1062.8 | 999999 | |
| 3.09 | -1.00 | 1.82 | -1.00 | 28.63 | 42.06 | 21.09 | 324.11 | 0.5409 | -804.9 | 999999 | |
| 0.00 | 0.77 | 0.00 | 0.46 | 29.69 | 42.00 | 21.03 | 325.47 | 0.5521 | -550.0 | -414.6 | |
| 0.00 | 1.29 | 0.00 | 0.76 | 29.49 | 41.92 | 20.95 | 325.33 | 0.5493 | -581.0 | -426.5 | |
| 0.00 | 0.95 | 0.00 | 0.56 | 30.29 | 42.02 | 21.05 | 326.14 | 0.5590 | 556.0 | 446.7 | |
| 0.00 | 1.12 | 0.00 | 0.66 | 29.03 | 41.53 | 20.56 | 325.25 | 0.5409 | -685.0 | -534.8 | |
| 0.00 | 2.06 | 0.00 | 1.21 | 29.75 | 40.27 | 19.30 | 327.68 | 0.5388 | -761.0 | -637.8 | |
| 0.00 | 1.20 | 0.00 | 0.68 | 26.68 | 36.50 | 15.53 | 329.39 | 0.4717 | 824.0 | 660.8 | |
| 0.00 | 1.46 | 0.00 | 0.82 | 26.49 | 36.40 | 15.43 | 329.30 | 0.4685 | 808.0 | 679.3 | |
| 0.00 | 1.12 | 0.00 | 0.63 | 27.24 | 36.34 | 15.37 | 330.30 | 0.4776 | 684.0 | 570.2 | |
| 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. | |