SDO HMI 2011-07-24 16:59:11 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 12.69 | 37.17 | 6.69 | 19.57 | 23.95 | 79.43 | 6.53 | 341.97 | 0.3420 | -774.8 | -602.3 | |
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back to the solar disc SDO HMI 2011-07-24 16:59:11 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 4.26 | 8.16 | 2.25 | 4.30 | 23.48 | 81.18 | 8.28 | 337.27 | 0.3432 | -985.3 | -739.9 | |
| 5.35 | 5.35 | 2.82 | 2.82 | 23.58 | 80.72 | 7.81 | 338.53 | 0.3419 | -892.9 | -1051.0 | |
| 3.08 | 4.17 | 1.62 | 2.19 | 23.59 | 80.25 | 7.35 | 339.70 | 0.3392 | -988.4 | -791.4 | |
| 0.00 | 4.08 | 0.00 | 2.13 | 22.60 | 79.93 | 7.02 | 339.40 | 0.3223 | -820.0 | -624.9 | |
| 0.00 | 1.00 | 0.00 | 0.52 | 22.09 | 79.77 | 6.87 | 339.21 | 0.3135 | -887.0 | -702.7 | |
| 0.00 | 1.18 | 0.00 | 0.62 | 22.67 | 79.40 | 6.50 | 340.89 | 0.3204 | -678.0 | -534.3 | |
| 0.00 | 1.72 | 0.00 | 0.90 | 23.05 | 79.15 | 6.25 | 341.97 | 0.3251 | -989.0 | -819.9 | |
| 0.00 | 1.36 | 0.00 | 0.71 | 23.37 | 79.10 | 6.20 | 342.44 | 0.3298 | -736.0 | -644.4 | |
| 0.00 | 1.63 | 0.00 | 0.86 | 24.63 | 78.49 | 5.59 | 345.16 | 0.3468 | -719.0 | -601.9 | |
| 0.00 | 3.17 | 0.00 | 1.68 | 25.00 | 77.26 | 4.35 | 348.55 | 0.3481 | -804.0 | -769.2 | |
| 0.00 | 2.63 | 0.00 | 1.40 | 26.76 | 77.22 | 4.32 | 349.66 | 0.3761 | -927.0 | -632.8 | |
| 0.00 | 1.09 | 0.00 | 0.57 | 24.94 | 76.99 | 4.08 | 349.20 | 0.3462 | -777.0 | -670.9 | |
| 0.00 | 1.63 | 0.00 | 0.87 | 27.23 | 73.98 | 1.08 | 357.45 | 0.3778 | 742.0 | 586.3 | |
| 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. | |