| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 26.85 | 75.91 | 14.52 | 41.17 | 3.22 | 139.13 | -21.74 | 65.62 | 0.4077 | -57.2 | 53.7 | |
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back to the solar disc SDO HMI 2014-03-26 04:00:31 UT
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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 | 0.61 | 4.08 | 141.40 | -19.47 | 61.22 | 0.3811 | -543.0 | -417.6 | |
| 11.90 | 21.60 | 6.36 | 11.55 | 3.51 | 141.32 | -19.56 | 62.66 | 0.3778 | -1054.0 | -720.1 | |
| 1.57 | 3.06 | 0.84 | 1.64 | 4.07 | 141.02 | -19.86 | 61.74 | 0.3863 | -941.5 | -748.2 | |
| 0.00 | 1.22 | 0.00 | 0.66 | 4.99 | 140.77 | -20.11 | 59.99 | 0.3972 | -744.0 | -561.5 | |
| 0.00 | 0.96 | 0.00 | 0.52 | 3.65 | 140.81 | -20.07 | 62.95 | 0.3862 | -698.0 | -482.1 | |
| 0.96 | 3.41 | 0.52 | 1.83 | 3.01 | 140.21 | -20.66 | 65.13 | 0.3901 | -1017.1 | -769.5 | |
| 0.00 | 4.29 | 0.00 | 2.31 | 2.80 | 139.54 | -21.33 | 66.34 | 0.3984 | -791.0 | -636.4 | |
| 0.00 | 0.70 | 0.00 | 0.38 | 3.53 | 139.30 | -21.58 | 64.92 | 0.4070 | -584.0 | -468.1 | |
| 0.00 | 1.22 | 0.00 | 0.67 | 5.07 | 139.06 | -21.81 | 61.87 | 0.4215 | -893.0 | -657.5 | |
| 0.00 | 0.70 | 0.00 | 0.38 | 3.15 | 138.37 | -22.50 | 66.72 | 0.4178 | 707.0 | 638.0 | |
| 0.00 | 1.31 | 0.00 | 0.72 | 3.07 | 138.21 | -22.67 | 67.05 | 0.4196 | 808.0 | 510.0 | |
| 3.85 | 15.48 | 2.10 | 8.46 | 3.53 | 138.10 | -22.77 | 66.16 | 0.4242 | 975.0 | 692.7 | |
| 0.00 | 1.14 | 0.00 | 0.62 | 2.83 | 138.12 | -22.76 | 67.67 | 0.4195 | 902.0 | 712.2 | |
| 7.35 | 13.47 | 4.02 | 7.36 | 2.76 | 137.66 | -23.21 | 68.24 | 0.4257 | 1000.3 | 684.9 | |
| 0.00 | 1.92 | 0.00 | 1.07 | 2.26 | 135.57 | -25.31 | 71.03 | 0.4535 | 911.0 | 806.0 | |
| 1.22 | 2.80 | 0.68 | 1.56 | 2.04 | 135.21 | -25.67 | 71.76 | 0.4577 | 941.1 | 751.3 | |
| 0.00 | 1.49 | 0.00 | 0.83 | 0.25 | 134.83 | -26.05 | 75.78 | 0.4550 | 780.0 | 581.2 | |
| 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. | |