SDO HMI 2011-02-10 01:58:56 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 11.89 | 45.93 | 7.09 | 27.45 | 19.61 | 65.65 | -21.91 | 38.91 | 0.5606 | 44.6 | -150.2 | |
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back to the solar disc SDO HMI 2011-02-10 01:58:56 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 2.57 | 3.51 | 1.50 | 2.05 | 19.31 | 68.03 | -19.53 | 36.24 | 0.5358 | -844.4 | -681.5 | |
| 3.08 | 13.26 | 1.81 | 7.79 | 19.23 | 67.61 | -19.95 | 36.91 | 0.5386 | -963.9 | -717.9 | |
| 0.00 | 0.60 | 0.00 | 0.35 | 18.64 | 67.52 | -20.04 | 37.74 | 0.5327 | -685.0 | -585.3 | |
| 1.97 | 10.09 | 1.17 | 5.98 | 19.72 | 66.91 | -20.65 | 37.28 | 0.5503 | -670.3 | -592.0 | |
| 0.00 | 1.62 | 0.00 | 0.96 | 19.32 | 66.86 | -20.70 | 37.80 | 0.5463 | -659.0 | -542.1 | |
| 1.11 | 1.97 | 0.68 | 1.20 | 20.65 | 64.53 | -23.03 | 39.19 | 0.5816 | 700.2 | 778.7 | |
| 1.62 | 4.70 | 0.99 | 2.87 | 19.76 | 63.12 | -24.44 | 41.89 | 0.5854 | 836.1 | 770.3 | |
| 0.00 | 1.71 | 0.00 | 1.04 | 19.48 | 62.89 | -24.67 | 42.50 | 0.5847 | 1006.0 | 789.1 | |
| 1.54 | 3.85 | 0.94 | 2.35 | 19.36 | 62.57 | -25.00 | 43.01 | 0.5867 | 866.8 | 748.4 | |
| 0.00 | 1.03 | 0.00 | 0.64 | 20.84 | 62.17 | -25.39 | 41.68 | 0.6050 | 557.0 | 400.8 | |
| 0.00 | 0.94 | 0.00 | 0.58 | 20.27 | 62.17 | -25.39 | 42.35 | 0.5995 | 803.0 | 624.5 | |
| 0.00 | 2.39 | 0.00 | 1.48 | 20.32 | 62.02 | -25.54 | 42.46 | 0.6012 | 803.0 | 519.6 | |
| 0.00 | 0.26 | 0.00 | 0.16 | 21.15 | 59.01 | -28.55 | 44.58 | 0.6373 | 481.0 | 412.3 | |
| 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. | |