SDO HMI 2011-07-24 12:59:11 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 15.86 | 31.39 | 8.32 | 16.47 | 23.86 | 79.36 | 4.24 | 347.88 | 0.3319 | -411.1 | -267.9 | |
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back to the solar disc SDO HMI 2011-07-24 12:59:11 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 6.98 | 7.89 | 3.66 | 4.14 | 23.50 | 81.15 | 6.04 | 343.00 | 0.3312 | -868.7 | -824.2 | |
| 5.71 | 6.35 | 3.00 | 3.33 | 23.60 | 80.69 | 5.57 | 344.32 | 0.3306 | -875.7 | -695.0 | |
| 3.17 | 4.35 | 1.66 | 2.28 | 23.61 | 80.26 | 5.14 | 345.48 | 0.3288 | -944.9 | -764.9 | |
| 0.00 | 0.91 | 0.00 | 0.47 | 22.46 | 79.78 | 4.67 | 345.83 | 0.3085 | -881.0 | -696.2 | |
| 0.00 | 3.08 | 0.00 | 1.61 | 22.72 | 79.43 | 4.31 | 347.07 | 0.3113 | -975.0 | -761.1 | |
| 0.00 | 1.27 | 0.00 | 0.66 | 23.04 | 79.21 | 4.09 | 347.95 | 0.3157 | -851.0 | -761.4 | |
| 0.00 | 1.27 | 0.00 | 0.66 | 23.52 | 79.02 | 3.90 | 348.80 | 0.3229 | -918.0 | -684.4 | |
| 0.00 | 1.27 | 0.00 | 0.67 | 24.49 | 78.31 | 3.20 | 351.30 | 0.3366 | -695.0 | -576.1 | |
| 0.00 | 0.82 | 0.00 | 0.43 | 24.24 | 76.64 | 1.52 | 355.78 | 0.3294 | 841.0 | 733.6 | |
| 0.00 | 1.09 | 0.00 | 0.58 | 27.23 | 75.03 | -0.09 | 0.21 | 0.3776 | 838.0 | 655.8 | |
| 0.00 | 1.00 | 0.00 | 0.53 | 27.17 | 74.28 | -0.84 | 1.99 | 0.3767 | 888.0 | 762.3 | |
| 0.00 | 1.18 | 0.00 | 0.63 | 26.41 | 73.43 | -1.69 | 4.15 | 0.3652 | 702.0 | 589.5 | |
| 0.00 | 0.91 | 0.00 | 0.48 | 24.59 | 72.96 | -2.16 | 5.88 | 0.3361 | 894.0 | 707.9 | |
| 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. | |