SDO HMI 2014-11-23 06:00:26 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 23.00 | 0.00 | 12.87 | -12.70 | 226.24 | 23.77 | 237.51 | 0.4673 | -28.5 | 141.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.86 | 0.00 | 0.49 | -12.07 | 228.46 | 25.98 | 240.97 | 0.4920 | 683.0 | 564.3 | |
| 0.00 | 3.86 | 0.00 | 2.20 | -13.08 | 228.43 | 25.96 | 239.13 | 0.4988 | 475.0 | 584.1 | |
| 0.00 | 0.86 | 0.00 | 0.49 | -12.75 | 228.40 | 25.92 | 239.70 | 0.4959 | 569.0 | 507.4 | |
| 0.00 | 2.06 | 0.00 | 1.17 | -12.74 | 228.19 | 25.72 | 239.51 | 0.4932 | 887.0 | 770.2 | |
| 0.00 | 1.37 | 0.00 | 0.78 | -13.54 | 228.15 | 25.67 | 238.06 | 0.4984 | 711.0 | 599.1 | |
| 0.00 | 3.86 | 0.00 | 2.19 | -12.95 | 227.91 | 25.44 | 238.87 | 0.4910 | 835.0 | 714.5 | |
| 0.00 | 0.69 | 0.00 | 0.39 | -13.50 | 227.50 | 25.03 | 237.50 | 0.4897 | 748.0 | 544.2 | |
| 0.00 | 1.29 | 0.00 | 0.71 | -11.89 | 223.94 | 21.47 | 236.66 | 0.4305 | -599.0 | -517.0 | |
| 0.00 | 1.29 | 0.00 | 0.70 | -12.55 | 223.51 | 21.03 | 234.82 | 0.4305 | -813.0 | -709.3 | |
| 0.00 | 0.86 | 0.00 | 0.47 | -10.87 | 223.38 | 20.90 | 238.04 | 0.4147 | -769.0 | -609.3 | |
| 0.00 | 1.80 | 0.00 | 0.98 | -11.85 | 223.32 | 20.85 | 235.98 | 0.4220 | -989.0 | -786.8 | |
| 0.00 | 1.37 | 0.00 | 0.75 | -12.95 | 223.38 | 20.90 | 233.89 | 0.4323 | -658.0 | -569.6 | |
| 0.00 | 1.03 | 0.00 | 0.56 | -11.42 | 223.22 | 20.75 | 236.73 | 0.4171 | -939.0 | -739.6 | |
| 0.00 | 1.80 | 0.00 | 0.99 | -13.46 | 222.94 | 20.46 | 232.33 | 0.4313 | -540.0 | -369.8 | |
| 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. | |