SDO HMI 2014-03-05 20:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 12.10 | 69.12 | 6.64 | 37.91 | -16.95 | 44.79 | -24.11 | 114.70 | 0.4315 | 48.4 | -52.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 4.23 | 17.54 | 2.29 | 9.47 | -17.10 | 46.92 | -21.98 | 116.68 | 0.4021 | 962.6 | 844.2 | |
| 0.00 | 1.12 | 0.00 | 0.61 | -16.70 | 46.73 | -22.16 | 115.59 | 0.4024 | 886.0 | 669.8 | |
| 1.04 | 6.83 | 0.56 | 3.69 | -16.33 | 46.68 | -22.22 | 114.69 | 0.4011 | 1086.4 | 827.2 | |
| 0.00 | 3.54 | 0.00 | 1.92 | -16.99 | 46.56 | -22.33 | 116.12 | 0.4065 | 719.0 | 542.3 | |
| 0.00 | 0.86 | 0.00 | 0.47 | -17.50 | 45.75 | -23.14 | 116.58 | 0.4210 | 694.0 | 441.8 | |
| 0.00 | 1.64 | 0.00 | 0.89 | -15.95 | 45.65 | -23.25 | 113.00 | 0.4140 | 749.0 | 610.9 | |
| 0.00 | 0.78 | 0.00 | 0.42 | -15.79 | 45.57 | -23.33 | 112.58 | 0.4145 | 762.0 | 664.9 | |
| 1.73 | 3.02 | 0.95 | 1.66 | -17.44 | 45.15 | -23.75 | 115.95 | 0.4291 | 943.9 | 673.4 | |
| 0.00 | 1.38 | 0.00 | 0.76 | -16.33 | 44.28 | -24.62 | 112.90 | 0.4358 | -906.0 | -743.3 | |
| 0.00 | 1.99 | 0.00 | 1.09 | -15.68 | 43.99 | -24.91 | 111.28 | 0.4370 | -1026.0 | -810.5 | |
| 0.00 | 2.68 | 0.00 | 1.48 | -16.19 | 43.89 | -25.01 | 112.33 | 0.4408 | -914.0 | -736.6 | |
| 0.00 | 1.64 | 0.00 | 0.91 | -16.18 | 43.07 | -25.83 | 111.79 | 0.4525 | -857.0 | -612.6 | |
| 5.10 | 25.32 | 2.84 | 14.11 | -17.31 | 42.76 | -26.14 | 113.97 | 0.4622 | -775.1 | -876.3 | |
| 0.00 | 0.78 | 0.00 | 0.43 | -16.54 | 42.46 | -26.44 | 112.18 | 0.4628 | -810.0 | -689.2 | |
| 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. | |