SDO HMI 2014-01-13 18:00:24 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 98.97 | 475.27 | 50.68 | 243.47 | -16.51 | 13.06 | -8.52 | 146.17 | 0.2558 | 1113.2 | 387.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 60.49 | 296.44 | 30.94 | 151.54 | -16.62 | 13.76 | -7.83 | 148.44 | 0.2504 | 1438.9 | 452.0 | |
| 0.00 | 1.44 | 0.00 | 0.75 | -18.49 | 12.86 | -8.73 | 149.50 | 0.2848 | 718.0 | 473.5 | |
| 0.00 | 1.61 | 0.00 | 0.83 | -16.19 | 12.72 | -8.86 | 144.21 | 0.2541 | 814.0 | 582.6 | |
| 0.00 | 2.97 | 0.00 | 1.52 | -15.71 | 12.71 | -8.87 | 143.00 | 0.2478 | 817.0 | 588.8 | |
| 0.76 | 1.95 | 0.39 | 1.00 | -15.31 | 12.54 | -9.04 | 141.47 | 0.2444 | 998.9 | 802.6 | |
| 6.71 | 160.33 | 3.45 | 82.30 | -16.73 | 12.45 | -9.14 | 144.66 | 0.2641 | 1102.8 | 321.7 | |
| 0.00 | 2.29 | 0.00 | 1.17 | -15.55 | 12.41 | -9.17 | 141.69 | 0.2489 | 636.0 | 477.2 | |
| 31.01 | -6.00 | 15.90 | -6.00 | -16.24 | 12.22 | -9.36 | 142.86 | 0.2599 | 1318.8 | 999999 | |
| 0.00 | 1.02 | 0.00 | 0.53 | -15.52 | 7.03 | -14.55 | 128.90 | 0.3125 | -930.0 | -771.2 | |
| 0.00 | 1.19 | 0.00 | 0.62 | -14.86 | 5.25 | -16.34 | 124.16 | 0.3301 | -845.0 | -626.5 | |
| 0.00 | 1.19 | 0.00 | 0.63 | -18.38 | 4.70 | -16.88 | 131.60 | 0.3702 | -799.0 | -709.4 | |
| 0.00 | 1.10 | 0.00 | 0.59 | -17.67 | 4.42 | -17.17 | 129.62 | 0.3667 | -801.0 | -690.9 | |
| 0.00 | 2.55 | 0.00 | 1.36 | -18.14 | 3.55 | -18.03 | 129.34 | 0.3820 | -828.0 | -657.5 | |
| 0.00 | 1.19 | 0.00 | 0.63 | -12.60 | 3.58 | -18.01 | 115.89 | 0.3368 | -799.0 | -502.0 | |
| 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. | |