SDO HMI 2011-05-09 17:59:08 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 29.00 | 117.80 | 26.35 | 106.78 | 16.71 | 51.87 | 53.81 | 292.49 | 0.8384 | -463.2 | -243.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 3.67 | 100.78 | 3.39 | 92.10 | 16.64 | 52.78 | 54.72 | 292.11 | 0.8464 | -359.5 | -267.5 | |
| 0.00 | 0.90 | 0.00 | 0.87 | 19.99 | 53.83 | 55.77 | 295.57 | 0.8634 | 481.0 | 397.8 | |
| 22.82 | -1.00 | 20.76 | -1.00 | 16.70 | 52.10 | 54.04 | 292.39 | 0.8406 | -716.3 | 999999 | |
| 0.00 | 0.90 | 0.00 | 0.82 | 17.58 | 52.26 | 54.20 | 293.34 | 0.8442 | -202.0 | -196.4 | |
| 0.00 | 0.81 | 0.00 | 0.72 | 16.25 | 51.27 | 53.21 | 292.12 | 0.8321 | -646.0 | -621.1 | |
| 0.00 | 1.07 | 0.00 | 0.95 | 16.27 | 51.07 | 53.01 | 292.21 | 0.8303 | -763.0 | -690.7 | |
| 0.00 | 1.79 | 0.00 | 1.58 | 16.55 | 50.97 | 52.91 | 292.57 | 0.8302 | -684.0 | -606.7 | |
| 2.51 | 4.39 | 2.20 | 3.86 | 16.76 | 50.69 | 52.63 | 292.90 | 0.8282 | -516.9 | -422.1 | |
| 0.00 | 1.88 | 0.00 | 1.62 | 15.56 | 50.12 | 52.06 | 291.67 | 0.8198 | 498.0 | 348.5 | |
| 0.00 | 1.25 | 0.00 | 1.09 | 16.62 | 50.32 | 52.26 | 292.85 | 0.8244 | -725.0 | -605.2 | |
| 0.00 | 0.81 | 0.00 | 0.66 | 16.32 | 47.98 | 49.92 | 293.29 | 0.8017 | 449.0 | 343.6 | |
| 0.00 | 0.81 | 0.00 | 0.64 | 17.02 | 45.72 | 47.66 | 294.98 | 0.7820 | 375.0 | 323.6 | |
| 0.00 | 0.98 | 0.00 | 0.76 | 17.34 | 44.33 | 46.27 | 295.95 | 0.7694 | 633.0 | 481.9 | |
| 0.00 | 1.43 | 0.00 | 1.11 | 17.57 | 44.27 | 46.21 | 296.25 | 0.7696 | 511.0 | 384.8 | |
| 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. | |