SDO HMI 2014-03-03 06:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 13.74 | 101.24 | 7.43 | 54.82 | 16.41 | 102.16 | -0.77 | 1.72 | 0.4052 | -101.1 | -198.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.90 | 0.00 | 1.03 | 16.00 | 105.05 | 2.12 | 354.86 | 0.3978 | -884.0 | -724.4 | |
| 0.00 | 1.21 | 0.00 | 0.64 | 14.36 | 105.03 | 2.10 | 354.49 | 0.3713 | -805.0 | -618.6 | |
| 0.78 | 5.87 | 0.42 | 3.17 | 16.16 | 104.86 | 1.93 | 355.33 | 0.4001 | -1033.0 | -777.7 | |
| 0.00 | 1.81 | 0.00 | 0.97 | 14.29 | 104.78 | 1.85 | 355.12 | 0.3699 | -806.0 | -680.5 | |
| 0.00 | 3.46 | 0.00 | 1.88 | 17.00 | 104.81 | 1.88 | 355.63 | 0.4135 | -556.0 | -527.5 | |
| 0.00 | 2.25 | 0.00 | 1.22 | 16.77 | 104.78 | 1.85 | 355.66 | 0.4099 | -756.0 | -600.8 | |
| 0.00 | 1.64 | 0.00 | 0.89 | 16.74 | 104.53 | 1.60 | 356.24 | 0.4091 | -852.0 | -738.9 | |
| 0.00 | 5.36 | 0.00 | 2.91 | 16.90 | 104.34 | 1.41 | 356.70 | 0.4115 | -529.0 | -651.7 | |
| 0.00 | 1.04 | 0.00 | 0.56 | 17.07 | 104.16 | 1.23 | 357.15 | 0.4139 | -700.0 | -578.2 | |
| 0.00 | 3.97 | 0.00 | 2.16 | 16.90 | 103.94 | 1.01 | 357.64 | 0.4111 | -873.0 | -760.0 | |
| 0.00 | 0.60 | 0.00 | 0.32 | 14.67 | 103.74 | 0.81 | 357.90 | 0.3751 | -627.0 | -537.6 | |
| 0.00 | 1.04 | 0.00 | 0.57 | 17.43 | 103.72 | 0.79 | 358.18 | 0.4193 | -617.0 | -526.1 | |
| 0.00 | 0.69 | 0.00 | 0.37 | 14.83 | 103.62 | 0.69 | 358.23 | 0.3776 | -713.0 | -591.4 | |
| 0.00 | 1.56 | 0.00 | 0.83 | 14.54 | 103.53 | 0.60 | 358.45 | 0.3729 | -771.0 | -572.7 | |
| 2.25 | 11.40 | 1.21 | 6.14 | 15.93 | 103.25 | 0.32 | 359.21 | 0.3952 | -989.1 | -763.7 | |
| 0.00 | 2.59 | 0.00 | 1.41 | 16.87 | 103.13 | 0.20 | 359.53 | 0.4103 | -521.0 | -481.3 | |
| 10.71 | 24.54 | 5.80 | 13.27 | 16.48 | 102.98 | 0.05 | 359.89 | 0.4040 | -1022.1 | -503.2 | |
| 0.00 | 1.21 | 0.00 | 0.64 | 14.32 | 101.53 | -1.40 | 3.68 | 0.3699 | 861.0 | 749.1 | |
| 0.00 | 0.86 | 0.00 | 0.47 | 16.26 | 101.43 | -1.50 | 3.61 | 0.4012 | 808.0 | 618.5 | |
| 0.00 | 0.86 | 0.00 | 0.46 | 15.17 | 100.26 | -2.67 | 6.72 | 0.3854 | 807.0 | 655.5 | |
| 0.00 | 1.12 | 0.00 | 0.61 | 16.72 | 100.21 | -2.72 | 6.38 | 0.4103 | 654.0 | 550.0 | |
| 0.00 | 3.20 | 0.00 | 1.71 | 15.01 | 99.99 | -2.94 | 7.46 | 0.3834 | 898.0 | 714.1 | |
| 0.00 | 1.47 | 0.00 | 0.79 | 15.04 | 99.71 | -3.22 | 8.15 | 0.3845 | 622.0 | 399.7 | |
| 0.00 | 1.90 | 0.00 | 1.03 | 16.60 | 99.56 | -3.37 | 7.93 | 0.4096 | 732.0 | 589.4 | |
| 0.00 | 1.38 | 0.00 | 0.75 | 16.08 | 99.23 | -3.70 | 8.91 | 0.4022 | 756.0 | 546.9 | |
| 0.00 | 1.21 | 0.00 | 0.65 | 15.76 | 98.68 | -4.25 | 10.36 | 0.3986 | 764.0 | 621.1 | |
| 0.00 | 0.69 | 0.00 | 0.38 | 17.19 | 98.43 | -4.50 | 10.28 | 0.4218 | 827.0 | 583.1 | |
| 0.00 | 5.87 | 0.00 | 3.20 | 16.94 | 97.94 | -4.99 | 11.50 | 0.4193 | 709.0 | 669.1 | |
| 0.00 | 1.73 | 0.00 | 0.94 | 17.20 | 97.90 | -5.03 | 11.46 | 0.4235 | 936.0 | 750.3 | |
| 0.00 | 1.12 | 0.00 | 0.62 | 18.82 | 97.48 | -5.45 | 11.59 | 0.4498 | 571.0 | 365.9 | |
| 0.00 | 2.16 | 0.00 | 1.18 | 16.59 | 97.35 | -5.58 | 13.00 | 0.4159 | 767.0 | 624.3 | |
| 0.00 | 1.04 | 0.00 | 0.56 | 16.36 | 97.30 | -5.63 | 13.25 | 0.4125 | 843.0 | 626.2 | |
| 0.00 | 0.69 | 0.00 | 0.38 | 17.01 | 97.25 | -5.68 | 13.00 | 0.4228 | 692.0 | 600.6 | |
| 0.00 | 1.38 | 0.00 | 0.76 | 17.54 | 96.95 | -5.98 | 13.35 | 0.4320 | 722.0 | 550.9 | |
| 0.00 | 1.38 | 0.00 | 0.78 | 20.13 | 96.64 | -6.29 | 12.64 | 0.4724 | 793.0 | 590.1 | |
| 0.00 | 1.04 | 0.00 | 0.57 | 17.78 | 96.31 | -6.62 | 14.57 | 0.4381 | 650.0 | 499.3 | |
| 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. | |