SDO HMI 2014-07-13 11:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 13.80 | 37.41 | 10.86 | 28.40 | 6.18 | 205.20 | 49.33 | 274.64 | 0.7576 | -180.2 | -122.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 3.09 | 6.81 | 2.49 | 5.49 | 5.13 | 208.17 | 52.30 | 273.27 | 0.7916 | -582.7 | -510.6 | |
| 0.64 | -1.00 | 0.51 | -1.00 | 5.27 | 207.89 | 52.02 | 273.44 | 0.7885 | -609.9 | 999999 | |
| 0.00 | 0.27 | 0.00 | 0.21 | 5.84 | 206.97 | 51.10 | 274.15 | 0.7785 | -219.0 | -195.3 | |
| 2.72 | 15.98 | 2.14 | 12.47 | 6.03 | 206.85 | 50.98 | 274.39 | 0.7771 | -513.9 | -509.4 | |
| 6.90 | -4.00 | 5.37 | -4.00 | 6.17 | 206.52 | 50.66 | 274.57 | 0.7736 | -757.8 | 999999 | |
| 0.00 | 2.45 | 0.00 | 1.88 | 5.78 | 205.85 | 49.98 | 274.06 | 0.7661 | -621.0 | -550.0 | |
| 0.45 | 1.54 | 0.35 | 1.17 | 4.19 | 205.35 | 49.48 | 271.95 | 0.7608 | 288.0 | 245.4 | |
| 0.00 | 1.18 | 0.00 | 0.89 | 9.37 | 204.80 | 48.93 | 278.81 | 0.7550 | 489.0 | 427.2 | |
| 0.00 | 0.82 | 0.00 | 0.61 | 8.33 | 204.61 | 48.74 | 277.45 | 0.7524 | 200.0 | 259.9 | |
| 0.00 | 1.82 | 0.00 | 1.33 | 6.46 | 203.50 | 47.63 | 274.96 | 0.7392 | -120.0 | -271.9 | |
| 0.00 | 1.09 | 0.00 | 0.76 | 9.52 | 200.69 | 44.82 | 279.34 | 0.7068 | 471.0 | 408.8 | |
| 0.00 | 1.09 | 0.00 | 0.74 | 6.68 | 198.75 | 42.88 | 275.34 | 0.6811 | 262.0 | 320.2 | |
| 0.00 | 1.91 | 0.00 | 1.25 | 6.09 | 196.87 | 41.00 | 274.51 | 0.6567 | 741.0 | 688.6 | |
| 0.00 | 1.18 | 0.00 | 0.77 | 6.80 | 196.86 | 40.99 | 275.59 | 0.6567 | 642.0 | 507.2 | |
| 0.00 | 1.27 | 0.00 | 0.83 | 8.27 | 196.18 | 40.31 | 277.90 | 0.6486 | 759.0 | 665.7 | |
| 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. | |