SDO HMI 2011-11-22 19:58:57 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 32.72 | 250.73 | 26.31 | 203.00 | 17.41 | 223.08 | -50.78 | 69.37 | 0.7921 | -565.3 | -199.6 | |
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back to the solar disc SDO HMI 2011-11-22 19:58:57 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 28.35 | 225.98 | 22.73 | 182.14 | 17.42 | 223.44 | -50.42 | 69.27 | 0.7886 | -1036.6 | -283.7 | |
| 1.80 | -1.00 | 1.47 | -1.00 | 17.96 | 222.78 | -51.08 | 68.76 | 0.7963 | -535.1 | 999999 | |
| 2.57 | -1.00 | 2.11 | -1.00 | 17.98 | 222.32 | -51.53 | 68.85 | 0.8008 | -465.8 | 999999 | |
| 0.00 | 1.03 | 0.00 | 0.86 | 18.15 | 221.74 | -52.11 | 68.78 | 0.8068 | 264.0 | 252.1 | |
| 0.00 | 1.88 | 0.00 | 1.53 | 15.49 | 222.37 | -51.49 | 71.92 | 0.7955 | 599.0 | 508.0 | |
| 0.00 | 1.46 | 0.00 | 1.20 | 15.88 | 221.98 | -51.87 | 71.51 | 0.8001 | 648.0 | 599.2 | |
| 0.00 | 12.85 | 0.00 | 10.70 | 16.48 | 221.50 | -52.35 | 70.87 | 0.8059 | 255.0 | 385.3 | |
| 0.00 | 1.28 | 0.00 | 1.11 | 17.46 | 220.07 | -53.79 | 69.98 | 0.8214 | 632.0 | 528.7 | |
| 0.00 | 1.28 | 0.00 | 1.10 | 16.39 | 220.36 | -53.50 | 71.22 | 0.8168 | 584.0 | 527.0 | |
| 0.00 | 1.63 | 0.00 | 1.41 | 17.21 | 219.91 | -53.95 | 70.32 | 0.8224 | 638.0 | 595.9 | |
| 0.00 | 0.94 | 0.00 | 0.82 | 17.05 | 219.66 | -54.19 | 70.56 | 0.8245 | 361.0 | 327.2 | |
| 0.00 | 1.46 | 0.00 | 1.29 | 17.28 | 219.02 | -54.83 | 70.41 | 0.8307 | 626.0 | 494.2 | |
| 0.00 | 0.94 | 0.00 | 0.84 | 17.45 | 218.67 | -55.18 | 70.27 | 0.8342 | 199.0 | 231.8 | |
| 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. | |