SDO HMI 2011-07-04 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 |
| 48.67 | 162.90 | 36.85 | 124.56 | 15.43 | 26.44 | 48.88 | 287.61 | 0.7639 | -257.6 | -357.4 | |
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back to the solar disc SDO HMI 2011-07-04 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 |
| 0.00 | 1.45 | 0.00 | 1.17 | 16.81 | 28.89 | 51.32 | 288.85 | 0.7919 | -500.0 | -399.9 | |
| 18.98 | 114.14 | 14.76 | 88.42 | 15.39 | 27.29 | 49.72 | 287.37 | 0.7729 | -904.0 | -438.5 | |
| 7.81 | -2.00 | 6.01 | -2.00 | 14.91 | 26.84 | 49.28 | 286.83 | 0.7674 | -824.8 | 999999 | |
| 0.00 | 1.36 | 0.00 | 1.03 | 15.22 | 26.12 | 48.55 | 287.38 | 0.7601 | -522.0 | -459.1 | |
| 0.00 | 1.63 | 0.00 | 1.24 | 15.04 | 26.06 | 48.49 | 287.15 | 0.7592 | -690.0 | -620.3 | |
| 0.00 | 1.00 | 0.00 | 0.75 | 13.99 | 25.66 | 48.09 | 285.85 | 0.7530 | -633.0 | -529.0 | |
| 0.00 | 1.09 | 0.00 | 0.81 | 13.72 | 25.40 | 47.83 | 285.54 | 0.7496 | -624.0 | -538.5 | |
| 0.00 | 2.09 | 0.00 | 1.58 | 15.83 | 25.88 | 48.31 | 288.22 | 0.7586 | -694.0 | -571.3 | |
| 2.72 | 8.08 | 2.05 | 6.09 | 15.40 | 25.65 | 48.08 | 287.70 | 0.7553 | 419.1 | -245.9 | |
| 3.18 | 27.42 | 2.33 | 20.12 | 15.80 | 24.22 | 46.65 | 288.55 | 0.7404 | 475.1 | 181.4 | |
| 14.35 | -10.00 | 10.52 | -10.00 | 16.34 | 24.02 | 46.45 | 289.32 | 0.7393 | 669.5 | 999999 | |
| 0.00 | 1.73 | 0.00 | 1.26 | 15.88 | 23.74 | 46.17 | 288.78 | 0.7352 | 801.0 | 677.1 | |
| 1.63 | 2.91 | 1.18 | 2.09 | 15.71 | 23.28 | 45.71 | 288.66 | 0.7296 | 726.1 | 646.6 | |
| 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. | |