SDO HMI 2014-03-10 16:00:29 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 28.08 | 0.00 | 14.12 | -10.80 | 13.72 | 8.50 | 241.37 | 0.1643 | 201.0 | 321.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.17 | 0.00 | 1.12 | -9.81 | 21.66 | 16.44 | 259.80 | 0.2846 | 819.0 | 600.5 | |
| 0.00 | 1.13 | 0.00 | 0.57 | -10.46 | 16.61 | 11.39 | 253.13 | 0.2039 | 991.0 | 763.1 | |
| 0.00 | 3.55 | 0.00 | 1.79 | -10.86 | 15.95 | 10.73 | 250.24 | 0.1951 | 904.0 | 850.1 | |
| 0.00 | 1.04 | 0.00 | 0.52 | -10.78 | 15.73 | 10.51 | 250.32 | 0.1911 | 1063.0 | 922.2 | |
| 0.00 | 1.99 | 0.00 | 1.00 | -10.72 | 15.51 | 10.29 | 250.24 | 0.1873 | 947.0 | 750.4 | |
| 0.00 | 2.08 | 0.00 | 1.05 | -11.29 | 15.53 | 10.31 | 247.44 | 0.1909 | 809.0 | 682.4 | |
| 0.00 | 1.82 | 0.00 | 0.92 | -10.95 | 14.69 | 9.47 | 247.57 | 0.1755 | 1053.0 | 773.5 | |
| 0.00 | 2.25 | 0.00 | 1.13 | -8.36 | 14.56 | 9.33 | 262.38 | 0.1627 | 888.0 | 686.8 | |
| 0.00 | 3.38 | 0.00 | 1.70 | -10.75 | 14.04 | 8.82 | 247.29 | 0.1640 | 915.0 | 746.0 | |
| 0.00 | 1.39 | 0.00 | 0.69 | -11.46 | 10.51 | 5.29 | 230.53 | 0.1175 | -1087.0 | -813.1 | |
| 0.00 | 0.95 | 0.00 | 0.48 | -13.08 | 8.95 | 3.72 | 211.72 | 0.1209 | -763.0 | -661.5 | |
| 0.00 | 1.04 | 0.00 | 0.52 | -12.28 | 8.88 | 3.65 | 215.17 | 0.1086 | -961.0 | -674.5 | |
| 0.00 | 1.13 | 0.00 | 0.56 | -11.50 | 8.68 | 3.46 | 218.32 | 0.0958 | -876.0 | -616.2 | |
| 0.00 | 1.56 | 0.00 | 0.78 | -12.13 | 8.29 | 3.07 | 211.43 | 0.1009 | -994.0 | -695.8 | |
| 0.00 | 2.60 | 0.00 | 1.29 | -10.61 | 7.86 | 2.63 | 217.31 | 0.0748 | -693.0 | -529.3 | |
| 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. | |