SDO HMI 2014-05-20 12:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 32.39 | 206.32 | 22.74 | 144.11 | -24.86 | 189.97 | 39.98 | 235.81 | 0.7069 | 510.5 | 225.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 32.39 | 186.25 | 22.74 | 130.77 | -24.65 | 190.49 | 40.50 | 236.40 | 0.7109 | 1080.8 | 305.8 | |
| 0.00 | 1.53 | 0.00 | 1.06 | -23.58 | 190.08 | 40.09 | 237.59 | 0.7014 | 482.0 | 397.4 | |
| 0.00 | 1.26 | 0.00 | 0.84 | -25.74 | 185.80 | 35.81 | 232.26 | 0.6687 | -778.0 | -736.4 | |
| 0.00 | 3.06 | 0.00 | 2.04 | -26.07 | 185.83 | 35.84 | 231.85 | 0.6712 | -581.0 | -516.0 | |
| 0.00 | 1.44 | 0.00 | 0.96 | -26.28 | 185.78 | 35.79 | 231.55 | 0.6719 | -617.0 | -522.0 | |
| 0.00 | 0.81 | 0.00 | 0.54 | -26.48 | 185.64 | 35.65 | 231.20 | 0.6718 | -503.0 | -445.3 | |
| 0.00 | 0.99 | 0.00 | 0.66 | -26.75 | 185.49 | 35.50 | 230.74 | 0.6720 | -636.0 | -542.6 | |
| 0.00 | 2.70 | 0.00 | 1.77 | -26.74 | 184.20 | 34.21 | 229.87 | 0.6589 | -285.0 | -317.1 | |
| 0.00 | 0.99 | 0.00 | 0.66 | -27.91 | 184.53 | 34.54 | 228.60 | 0.6703 | -616.0 | -532.1 | |
| 0.00 | 0.45 | 0.00 | 0.30 | -28.80 | 184.27 | 34.28 | 227.30 | 0.6740 | -503.0 | -490.2 | |
| 0.00 | 0.99 | 0.00 | 0.66 | -28.63 | 184.21 | 34.22 | 227.46 | 0.6722 | -662.0 | -542.2 | |
| 0.00 | 2.70 | 0.00 | 1.80 | -28.46 | 184.02 | 34.03 | 227.54 | 0.6692 | -693.0 | -566.8 | |
| 0.00 | 1.44 | 0.00 | 0.96 | -29.33 | 183.46 | 33.47 | 226.06 | 0.6702 | -311.0 | -336.5 | |
| 0.00 | 1.71 | 0.00 | 1.09 | -27.44 | 180.58 | 30.59 | 226.20 | 0.6281 | -631.0 | -532.3 | |
| 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. | |