SDO HMI 2011-02-10 19:58:56 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.88 | 22.59 | 1.05 | 12.74 | 19.15 | 65.63 | -12.06 | 24.42 | 0.4790 | 35.8 | -138.2 | |
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back to the solar disc SDO HMI 2011-02-10 19:58:56 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.88 | 8.12 | 1.05 | 4.53 | 19.36 | 68.84 | -8.85 | 18.39 | 0.4619 | -975.5 | -720.3 | |
| 0.00 | 0.86 | 0.00 | 0.48 | 18.46 | 67.69 | -10.00 | 21.32 | 0.4550 | -717.0 | -610.5 | |
| 0.00 | 0.86 | 0.00 | 0.48 | 18.56 | 67.53 | -10.17 | 21.55 | 0.4574 | -690.0 | -571.6 | |
| 0.00 | 1.45 | 0.00 | 0.81 | 19.10 | 67.11 | -10.58 | 21.89 | 0.4674 | -700.0 | -563.2 | |
| 0.00 | 1.03 | 0.00 | 0.58 | 19.34 | 66.55 | -11.14 | 22.71 | 0.4741 | -766.0 | -627.2 | |
| 0.00 | 0.94 | 0.00 | 0.54 | 20.25 | 64.65 | -13.04 | 25.25 | 0.4984 | 772.0 | 661.8 | |
| 0.00 | 1.20 | 0.00 | 0.68 | 19.62 | 63.38 | -14.31 | 27.97 | 0.4987 | 889.0 | 691.2 | |
| 0.00 | 1.37 | 0.00 | 0.78 | 19.41 | 62.98 | -14.72 | 28.84 | 0.4987 | 926.0 | 777.8 | |
| 0.00 | 1.37 | 0.00 | 0.82 | 24.06 | 62.31 | -15.38 | 25.57 | 0.5635 | 466.0 | 350.7 | |
| 0.00 | 1.80 | 0.00 | 0.98 | 13.87 | 63.03 | -14.66 | 35.37 | 0.4263 | -666.0 | -556.4 | |
| 0.00 | 0.94 | 0.00 | 0.54 | 20.32 | 62.20 | -15.49 | 29.15 | 0.5162 | 607.0 | 514.7 | |
| 0.00 | 1.62 | 0.00 | 0.93 | 18.51 | 61.21 | -16.48 | 32.64 | 0.5008 | 770.0 | 601.5 | |
| 0.00 | 1.03 | 0.00 | 0.59 | 18.49 | 60.95 | -16.74 | 33.07 | 0.5027 | 601.0 | 446.9 | |
| 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. | |