SDO HMI 2011-08-18 09:59:09 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 6.30 | 31.78 | 3.48 | 17.54 | -18.10 | 113.97 | 7.79 | 196.97 | 0.4414 | -154.0 | -330.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.99 | 0.00 | 0.55 | -18.22 | 118.03 | 11.84 | 204.89 | 0.4651 | 805.0 | 643.5 | |
| 1.80 | 2.07 | 1.01 | 1.16 | -18.74 | 117.28 | 11.10 | 203.03 | 0.4677 | 849.5 | 890.0 | |
| 0.00 | 1.71 | 0.00 | 0.96 | -19.09 | 116.38 | 10.20 | 201.07 | 0.4675 | 671.0 | 552.4 | |
| 0.00 | 1.71 | 0.00 | 0.96 | -19.26 | 116.36 | 10.18 | 200.90 | 0.4698 | 672.0 | 508.9 | |
| 0.00 | 1.17 | 0.00 | 0.65 | -18.44 | 115.96 | 9.77 | 200.78 | 0.4558 | 749.0 | 547.2 | |
| 0.00 | 2.52 | 0.00 | 1.39 | -17.66 | 113.88 | 7.70 | 197.19 | 0.4338 | -1009.0 | -799.9 | |
| 3.51 | 7.03 | 1.93 | 3.85 | -17.69 | 113.34 | 7.15 | 196.02 | 0.4317 | -969.5 | -737.5 | |
| 0.00 | 3.15 | 0.00 | 1.73 | -18.06 | 113.35 | 7.17 | 195.81 | 0.4373 | -815.0 | -657.1 | |
| 0.00 | 4.50 | 0.00 | 2.49 | -18.66 | 113.34 | 7.16 | 195.41 | 0.4464 | -972.0 | -776.0 | |
| 0.99 | 1.71 | 0.54 | 0.93 | -16.99 | 113.24 | 7.06 | 196.30 | 0.4207 | 698.6 | 654.4 | |
| 0.00 | 1.08 | 0.00 | 0.59 | -16.00 | 113.18 | 6.99 | 196.86 | 0.4052 | 578.0 | 514.2 | |
| 0.00 | 0.81 | 0.00 | 0.45 | -18.36 | 113.27 | 7.09 | 195.44 | 0.4415 | -848.0 | -721.2 | |
| 0.00 | 1.35 | 0.00 | 0.74 | -17.69 | 111.19 | 5.01 | 191.36 | 0.4238 | -762.0 | -646.5 | |
| 0.00 | 1.98 | 0.00 | 1.09 | -18.36 | 111.05 | 4.87 | 190.74 | 0.4337 | -663.0 | -617.4 | |
| 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. | |