SDO HMI 2011-02-26 07:58:58 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 13.45 | 50.31 | 13.18 | 49.15 | 16.69 | 178.51 | -55.07 | 65.76 | 0.8629 | -102.3 | 98.2 | |
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back to the solar disc SDO HMI 2011-02-26 07:58:58 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 2.41 | 3.10 | 2.29 | 2.94 | 17.26 | 179.76 | -53.83 | 64.68 | 0.8549 | -411.4 | -375.1 | |
| 0.00 | 0.69 | 0.00 | 0.68 | 18.74 | 178.86 | -54.72 | 63.40 | 0.8666 | -490.0 | -473.8 | |
| 2.50 | 18.01 | 2.32 | 16.81 | 15.58 | 179.91 | -53.67 | 66.48 | 0.8485 | 764.8 | 505.0 | |
| 0.00 | 2.84 | 0.00 | 2.75 | 17.43 | 179.04 | -54.55 | 64.76 | 0.8612 | -624.0 | -445.9 | |
| 2.07 | 3.27 | 1.95 | 3.09 | 16.04 | 179.47 | -54.12 | 66.13 | 0.8536 | 387.2 | 330.1 | |
| 0.00 | 1.64 | 0.00 | 1.55 | 15.67 | 179.35 | -54.24 | 66.59 | 0.8535 | 438.0 | 342.4 | |
| 3.45 | 8.70 | 3.43 | 8.68 | 17.35 | 177.98 | -55.60 | 65.24 | 0.8693 | -555.2 | -309.9 | |
| 0.52 | 1.46 | 0.51 | 1.44 | 15.88 | 178.02 | -55.56 | 66.84 | 0.8649 | 594.3 | 498.9 | |
| 0.00 | 4.74 | 0.00 | 5.02 | 18.79 | 176.36 | -57.23 | 64.27 | 0.8855 | -466.0 | -289.5 | |
| 0.00 | 1.12 | 0.00 | 1.11 | 15.96 | 177.54 | -56.04 | 66.92 | 0.8689 | 438.0 | 340.8 | |
| 0.00 | 1.29 | 0.00 | 1.38 | 17.56 | 175.53 | -58.05 | 65.88 | 0.8883 | -349.0 | -288.1 | |
| 2.50 | 3.19 | 2.68 | 3.43 | 17.26 | 175.26 | -58.32 | 66.28 | 0.8895 | -251.3 | -215.8 | |
| 0.00 | 0.26 | 0.00 | 0.27 | 16.36 | 175.59 | -58.00 | 67.14 | 0.8850 | -323.0 | -356.0 | |
| 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. | |