SDO HMI 2011-11-13 03:58:58 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 43.06 | 307.98 | 23.53 | 168.39 | 28.07 | 43.23 | 1.96 | 355.92 | 0.4250 | -984.2 | -431.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.95 | 299.37 | 0.52 | 163.68 | 27.83 | 44.07 | 2.80 | 354.11 | 0.4221 | -926.1 | -445.8 | |
| 1.03 | -1.00 | 0.56 | -1.00 | 27.79 | 43.93 | 2.66 | 354.38 | 0.4214 | -941.5 | 999999 | |
| 8.44 | -1.00 | 4.62 | -1.00 | 28.19 | 43.54 | 2.27 | 355.30 | 0.4271 | -1188.9 | 999999 | |
| 19.97 | -1.00 | 10.90 | -1.00 | 27.89 | 43.40 | 2.13 | 355.53 | 0.4222 | -1466.4 | 999999 | |
| 0.95 | -1.00 | 0.52 | -1.00 | 27.47 | 43.36 | 2.08 | 355.53 | 0.4155 | -1207.5 | 999999 | |
| 3.36 | -1.00 | 1.84 | -1.00 | 28.22 | 43.17 | 1.90 | 356.07 | 0.4272 | -988.7 | 999999 | |
| 4.13 | -1.00 | 2.26 | -1.00 | 28.42 | 43.04 | 1.76 | 356.37 | 0.4301 | -876.0 | 999999 | |
| 1.64 | -1.00 | 0.90 | -1.00 | 28.68 | 43.04 | 1.77 | 356.41 | 0.4343 | -540.6 | 999999 | |
| 1.38 | -1.00 | 0.75 | -1.00 | 28.22 | 42.90 | 1.63 | 356.63 | 0.4269 | -922.2 | 999999 | |
| 1.21 | -1.00 | 0.66 | -1.00 | 28.12 | 42.66 | 1.39 | 357.10 | 0.4251 | -860.6 | 999999 | |
| 0.00 | 2.58 | 0.00 | 1.42 | 28.81 | 40.54 | -0.73 | 1.48 | 0.4357 | -843.0 | -651.6 | |
| 0.00 | 1.64 | 0.00 | 0.90 | 28.78 | 40.30 | -0.97 | 1.96 | 0.4352 | -734.0 | -528.3 | |
| 0.00 | 1.72 | 0.00 | 0.94 | 27.92 | 37.59 | -3.69 | 7.71 | 0.4253 | 816.0 | 644.7 | |
| 0.00 | 1.29 | 0.00 | 0.70 | 27.66 | 37.50 | -3.78 | 7.99 | 0.4214 | 838.0 | 626.6 | |
| 0.00 | 1.38 | 0.00 | 0.75 | 28.18 | 37.38 | -3.90 | 8.05 | 0.4299 | 503.0 | 358.1 | |
| 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. | |