SDO HMI 2014-04-22 20:00:35 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 5.50 | 30.19 | 2.84 | 16.00 | -19.57 | 141.21 | -14.52 | 138.16 | 0.3498 | 365.8 | 166.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 4.79 | 7.01 | 2.46 | 3.60 | -17.60 | 146.89 | -8.84 | 146.30 | 0.2651 | 1137.4 | 698.5 | |
| 0.00 | 1.15 | 0.00 | 0.60 | -18.39 | 145.40 | -10.33 | 143.89 | 0.2899 | 1034.0 | 740.1 | |
| 0.00 | 2.66 | 0.00 | 1.39 | -18.74 | 144.21 | -11.51 | 141.71 | 0.3064 | 962.0 | 828.1 | |
| 0.00 | 1.24 | 0.00 | 0.64 | -17.14 | 143.19 | -12.54 | 135.71 | 0.2983 | 755.0 | 544.9 | |
| 0.00 | 1.33 | 0.00 | 0.70 | -20.18 | 141.76 | -13.96 | 139.46 | 0.3498 | 917.0 | 694.5 | |
| 0.00 | 1.07 | 0.00 | 0.57 | -20.58 | 141.23 | -14.49 | 139.21 | 0.3602 | 788.0 | 683.5 | |
| 0.71 | 1.95 | 0.38 | 1.04 | -20.69 | 140.59 | -15.14 | 138.24 | 0.3684 | 921.6 | 697.9 | |
| 0.00 | 2.93 | 0.00 | 1.56 | -20.68 | 140.19 | -15.54 | 137.51 | 0.3726 | 811.0 | 728.4 | |
| 0.00 | 3.73 | 0.00 | 2.03 | -21.42 | 137.29 | -18.43 | 134.30 | 0.4130 | -1028.0 | -865.6 | |
| 0.00 | 1.07 | 0.00 | 0.59 | -22.99 | 136.90 | -18.82 | 136.56 | 0.4337 | -705.0 | -482.2 | |
| 0.00 | 0.98 | 0.00 | 0.53 | -21.03 | 136.80 | -18.92 | 132.86 | 0.4147 | -855.0 | -660.1 | |
| 0.00 | 1.69 | 0.00 | 0.90 | -16.82 | 137.26 | -18.46 | 124.64 | 0.3700 | 894.0 | 756.3 | |
| 0.00 | 1.60 | 0.00 | 0.87 | -20.64 | 136.10 | -19.62 | 131.15 | 0.4191 | -899.0 | -671.4 | |
| 0.00 | 1.78 | 0.00 | 0.98 | -21.21 | 135.33 | -20.39 | 131.22 | 0.4337 | -950.0 | -752.0 | |
| 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. | |