SDO HMI 2011-11-22 13:58:57 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 41.55 | 229.03 | 36.29 | 199.85 | 17.49 | 223.00 | -54.17 | 70.03 | 0.8249 | -456.8 | -162.6 | |
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back to the solar disc SDO HMI 2011-11-22 13:58:57 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 29.90 | 205.98 | 25.82 | 178.76 | 17.47 | 223.37 | -53.80 | 69.98 | 0.8214 | -827.2 | -221.8 | |
| 3.34 | -1.00 | 2.93 | -1.00 | 18.01 | 222.86 | -54.30 | 69.43 | 0.8271 | -586.5 | 999999 | |
| 2.91 | -1.00 | 2.58 | -1.00 | 18.00 | 222.44 | -54.73 | 69.53 | 0.8310 | -415.1 | 999999 | |
| 0.00 | 0.94 | 0.00 | 0.88 | 20.05 | 220.73 | -56.44 | 67.48 | 0.8495 | 378.0 | 321.2 | |
| 0.00 | 2.06 | 0.00 | 1.81 | 16.06 | 222.42 | -54.75 | 71.85 | 0.8280 | 272.0 | 262.1 | |
| 1.11 | 10.11 | 1.00 | 9.09 | 16.44 | 221.77 | -55.39 | 71.51 | 0.8346 | -137.5 | 357.1 | |
| 0.00 | 0.86 | 0.00 | 0.76 | 16.29 | 221.84 | -55.33 | 71.68 | 0.8337 | -137.0 | -182.4 | |
| 2.83 | -6.00 | 2.55 | -6.00 | 16.52 | 221.41 | -55.76 | 71.48 | 0.8380 | 581.1 | 999999 | |
| 0.00 | 1.46 | 0.00 | 1.31 | 16.15 | 221.35 | -55.82 | 71.93 | 0.8380 | 442.0 | 375.9 | |
| 0.00 | 3.68 | 0.00 | 3.46 | 17.32 | 220.02 | -57.14 | 70.79 | 0.8514 | 712.0 | 574.6 | |
| 0.00 | 0.69 | 0.00 | 0.64 | 16.37 | 220.24 | -56.92 | 71.86 | 0.8482 | 532.0 | 559.1 | |
| 1.46 | 2.91 | 1.41 | 2.81 | 17.26 | 218.94 | -58.22 | 71.03 | 0.8605 | 475.5 | 430.1 | |
| 0.00 | 0.34 | 0.00 | 0.33 | 17.34 | 218.49 | -58.68 | 71.01 | 0.8645 | 156.0 | 174.2 | |
| 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. | |