SDO HMI 2014-04-06 04:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.58 | 24.30 | 0.79 | 12.20 | -8.27 | 7.21 | -8.56 | 106.31 | 0.1559 | 73.3 | -111.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.14 | 0.00 | 0.57 | -7.86 | 12.36 | -3.41 | 115.52 | 0.0656 | 761.0 | 521.0 | |
| 0.00 | 1.06 | 0.00 | 0.52 | -9.06 | 12.04 | -3.73 | 127.39 | 0.0812 | 780.0 | 611.8 | |
| 0.00 | 1.23 | 0.00 | 0.61 | -7.30 | 10.57 | -5.19 | 101.75 | 0.0922 | 816.0 | 602.1 | |
| 0.00 | 1.58 | 0.00 | 0.79 | -10.27 | 10.34 | -5.42 | 127.16 | 0.1173 | 692.0 | 486.3 | |
| 0.00 | 1.50 | 0.00 | 0.75 | -10.39 | 10.19 | -5.58 | 127.20 | 0.1206 | 851.0 | 733.9 | |
| 1.58 | 2.73 | 0.79 | 1.36 | -9.73 | 9.89 | -5.87 | 121.19 | 0.1184 | 982.4 | 851.0 | |
| 0.00 | 1.32 | 0.00 | 0.66 | -6.81 | 9.43 | -6.34 | 95.35 | 0.1107 | 869.0 | 661.3 | |
| 0.00 | 1.32 | 0.00 | 0.67 | -7.28 | 5.26 | -10.51 | 96.19 | 0.1828 | -997.0 | -769.4 | |
| 0.00 | 1.06 | 0.00 | 0.53 | -6.89 | 5.18 | -10.59 | 94.02 | 0.1837 | -987.0 | -750.0 | |
| 0.00 | 1.41 | 0.00 | 0.71 | -7.03 | 5.08 | -10.69 | 94.79 | 0.1855 | -1013.0 | -822.2 | |
| 0.00 | 5.99 | 0.00 | 3.02 | -7.45 | 4.89 | -10.88 | 96.93 | 0.1894 | -581.0 | -723.4 | |
| 0.00 | 0.88 | 0.00 | 0.44 | -7.11 | 4.56 | -11.21 | 95.03 | 0.1946 | -813.0 | -655.4 | |
| 0.00 | 1.67 | 0.00 | 0.85 | -6.65 | 4.17 | -11.60 | 92.62 | 0.2009 | -924.0 | -683.4 | |
| 0.00 | 1.41 | 0.00 | 0.72 | -12.26 | 3.46 | -12.30 | 117.20 | 0.2352 | 780.0 | 611.1 | |
| 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. | |