SDO HMI 2014-01-15 16:00:24 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 29.74 | 152.80 | 18.40 | 93.98 | -17.36 | 31.15 | 34.80 | 246.67 | 0.5954 | 494.1 | 245.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.02 | 0.00 | 0.63 | -16.48 | 32.38 | 36.03 | 248.63 | 0.6080 | 567.0 | 537.5 | |
| 6.46 | 76.07 | 4.02 | 47.24 | -17.25 | 32.09 | 35.74 | 247.28 | 0.6071 | 753.7 | 349.6 | |
| 1.02 | 6.80 | 0.63 | 4.21 | -16.60 | 31.87 | 35.52 | 248.24 | 0.6018 | 901.2 | 736.4 | |
| 0.00 | 1.36 | 0.00 | 0.84 | -16.60 | 31.72 | 35.37 | 248.17 | 0.5999 | 938.0 | 704.6 | |
| 0.00 | 1.53 | 0.00 | 0.95 | -17.00 | 31.73 | 35.38 | 247.54 | 0.6015 | 719.0 | 662.0 | |
| 17.17 | -2.00 | 10.66 | -2.00 | -17.78 | 31.79 | 35.44 | 246.30 | 0.6053 | 998.5 | 999999 | |
| 2.63 | 28.90 | 1.62 | 17.73 | -16.99 | 31.20 | 34.85 | 247.32 | 0.5946 | 1058.3 | 612.5 | |
| 0.00 | 0.76 | 0.00 | 0.47 | -17.41 | 31.26 | 34.90 | 246.66 | 0.5969 | 776.0 | 657.8 | |
| 0.00 | 19.12 | 0.00 | 11.63 | -17.09 | 30.25 | 33.90 | 246.71 | 0.5826 | 175.0 | -97.9 | |
| 0.00 | 4.42 | 0.00 | 2.65 | -17.39 | 28.80 | 32.44 | 245.48 | 0.5649 | -695.0 | -580.7 | |
| 2.46 | 7.56 | 1.47 | 4.51 | -17.44 | 28.40 | 32.05 | 245.19 | 0.5599 | -1030.5 | -711.9 | |
| 0.00 | 2.21 | 0.00 | 1.31 | -17.54 | 28.06 | 31.71 | 244.83 | 0.5559 | -1002.0 | -913.6 | |
| 0.00 | 0.51 | 0.00 | 0.30 | -18.28 | 27.99 | 31.63 | 243.54 | 0.5585 | -413.0 | -321.3 | |
| 0.00 | 1.78 | 0.00 | 1.06 | -17.84 | 27.61 | 31.25 | 244.07 | 0.5514 | -866.0 | -756.0 | |
| 0.00 | 0.76 | 0.00 | 0.45 | -18.18 | 27.42 | 31.07 | 243.37 | 0.5506 | -607.0 | -556.3 | |
| 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. | |