SDO HMI 2014-11-22 23:04:11 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 28.53 | 0.00 | 15.42 | -12.59 | 224.79 | 18.51 | 231.03 | 0.3994 | -143.9 | -238.2 | |
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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 | 0.48 | -13.54 | 228.34 | 22.06 | 234.10 | 0.4527 | 578.0 | 574.0 | |
| 0.00 | 0.77 | 0.00 | 0.43 | -12.90 | 228.21 | 21.93 | 235.15 | 0.4455 | 917.0 | 837.1 | |
| 0.00 | 2.14 | 0.00 | 1.19 | -13.54 | 228.08 | 21.80 | 233.79 | 0.4493 | 668.0 | 640.4 | |
| 0.00 | 2.91 | 0.00 | 1.61 | -12.92 | 227.92 | 21.64 | 234.75 | 0.4420 | 679.0 | 612.9 | |
| 0.00 | 0.86 | 0.00 | 0.47 | -13.22 | 227.20 | 20.92 | 233.29 | 0.4354 | 737.0 | 544.6 | |
| 0.00 | 1.71 | 0.00 | 0.94 | -13.03 | 227.12 | 20.84 | 233.54 | 0.4327 | 870.0 | 758.0 | |
| 0.00 | 0.86 | 0.00 | 0.46 | -12.99 | 223.76 | 17.48 | 228.84 | 0.3906 | -747.0 | -602.5 | |
| 0.00 | 6.00 | 0.00 | 3.20 | -11.46 | 223.41 | 17.13 | 231.44 | 0.3708 | -743.0 | -706.2 | |
| 0.00 | 1.63 | 0.00 | 0.88 | -13.97 | 223.55 | 17.27 | 226.59 | 0.3983 | -741.0 | -472.2 | |
| 0.00 | 2.66 | 0.00 | 1.42 | -11.73 | 223.33 | 17.05 | 230.73 | 0.3725 | -904.0 | -777.2 | |
| 0.00 | 1.37 | 0.00 | 0.73 | -12.68 | 223.23 | 16.95 | 228.60 | 0.3809 | -821.0 | -695.2 | |
| 0.00 | 3.34 | 0.00 | 1.78 | -12.19 | 223.04 | 16.76 | 229.30 | 0.3735 | -958.0 | -728.8 | |
| 0.00 | 2.31 | 0.00 | 1.24 | -13.63 | 223.14 | 16.86 | 226.58 | 0.3898 | -716.0 | -617.9 | |
| 0.00 | 1.11 | 0.00 | 0.59 | -12.40 | 222.80 | 16.52 | 228.46 | 0.3728 | -834.0 | -650.8 | |
| 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. | |