SDO HMI 2011-02-15 21:58:57 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 22.95 | 63.76 | 22.44 | 61.95 | 19.70 | 64.62 | 53.87 | 297.87 | 0.8612 | 174.2 | 192.1 | |
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back to the solar disc SDO HMI 2011-02-15 21:58:57 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 6.85 | 13.96 | 7.45 | 15.24 | 18.86 | 68.98 | 58.22 | 295.31 | 0.8918 | -477.6 | -39.1 | |
| 0.00 | 0.26 | 0.00 | 0.28 | 19.11 | 68.58 | 57.83 | 295.71 | 0.8896 | -373.0 | -445.0 | |
| 0.00 | 0.69 | 0.00 | 0.74 | 19.31 | 68.57 | 57.82 | 295.92 | 0.8900 | -293.0 | -342.5 | |
| 0.00 | 0.86 | 0.00 | 0.88 | 18.26 | 67.20 | 56.45 | 295.28 | 0.8772 | -491.0 | -427.2 | |
| 0.00 | 2.57 | 0.00 | 2.65 | 18.83 | 67.15 | 56.40 | 295.91 | 0.8784 | -409.0 | -376.6 | |
| 2.31 | 5.91 | 2.23 | 5.70 | 19.10 | 64.75 | 53.99 | 297.11 | 0.8608 | 464.0 | 310.1 | |
| 0.00 | 1.46 | 0.00 | 1.38 | 20.00 | 63.64 | 52.89 | 298.52 | 0.8550 | 335.0 | 296.4 | |
| 1.20 | 1.63 | 1.13 | 1.53 | 19.91 | 63.33 | 52.58 | 298.55 | 0.8522 | 433.1 | 449.2 | |
| 5.91 | 31.53 | 5.46 | 29.10 | 19.96 | 62.53 | 51.78 | 298.94 | 0.8459 | 698.7 | 383.6 | |
| 6.68 | -9.00 | 6.17 | -9.00 | 20.27 | 62.42 | 51.67 | 299.33 | 0.8462 | 604.2 | 999999 | |
| 0.00 | 0.94 | 0.00 | 0.90 | 21.80 | 63.18 | 52.43 | 300.66 | 0.8576 | -350.0 | -265.0 | |
| 0.00 | 2.06 | 0.00 | 1.86 | 21.13 | 61.05 | 50.30 | 300.87 | 0.8383 | 475.0 | 416.5 | |
| 0.00 | 1.20 | 0.00 | 1.07 | 20.83 | 60.72 | 49.96 | 300.69 | 0.8344 | 592.0 | 490.8 | |
| 0.00 | 0.69 | 0.00 | 0.62 | 21.85 | 61.00 | 50.25 | 301.68 | 0.8407 | 481.0 | 339.9 | |
| 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. | |