SDO HMI 2014-07-22 12:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 27.67 | 115.88 | 18.29 | 76.57 | -21.00 | 68.95 | 32.72 | 229.82 | 0.6623 | 463.6 | 191.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 16.97 | 91.81 | 11.30 | 61.13 | -20.96 | 69.82 | 33.59 | 230.62 | 0.6706 | 1028.4 | 307.2 | |
| 0.00 | 1.00 | 0.00 | 0.66 | -20.36 | 69.32 | 33.09 | 230.96 | 0.6612 | 341.0 | 281.8 | |
| 2.99 | -1.00 | 1.98 | -1.00 | -20.79 | 69.27 | 33.04 | 230.38 | 0.6639 | 978.8 | 999999 | |
| 2.81 | -1.00 | 1.85 | -1.00 | -20.81 | 69.00 | 32.77 | 230.14 | 0.6614 | 908.4 | 999999 | |
| 0.73 | 5.99 | 0.48 | 3.92 | -21.05 | 68.28 | 32.05 | 229.26 | 0.6560 | 757.6 | 584.5 | |
| 1.63 | -5.00 | 1.07 | -5.00 | -21.18 | 68.16 | 31.93 | 228.99 | 0.6558 | 789.2 | 999999 | |
| 0.00 | 1.27 | 0.00 | 0.82 | -19.81 | 67.73 | 31.50 | 230.34 | 0.6407 | 702.0 | 549.9 | |
| 0.00 | 0.73 | 0.00 | 0.46 | -20.76 | 65.90 | 29.67 | 227.51 | 0.6298 | -695.0 | -588.0 | |
| 0.00 | 3.45 | 0.00 | 2.20 | -21.57 | 65.70 | 29.47 | 226.33 | 0.6347 | -652.0 | -496.1 | |
| 0.00 | 0.91 | 0.00 | 0.58 | -21.21 | 65.36 | 29.13 | 226.45 | 0.6283 | -754.0 | -658.5 | |
| 0.00 | 2.09 | 0.00 | 1.34 | -21.83 | 65.49 | 29.26 | 225.82 | 0.6349 | -533.0 | -479.6 | |
| 2.54 | 6.90 | 1.61 | 4.37 | -21.62 | 64.73 | 28.50 | 225.35 | 0.6258 | -902.4 | -684.9 | |
| 0.00 | 0.64 | 0.00 | 0.40 | -21.06 | 64.24 | 28.01 | 225.57 | 0.6160 | -639.0 | -612.1 | |
| 0.00 | 1.09 | 0.00 | 0.69 | -22.12 | 63.65 | 27.42 | 223.68 | 0.6199 | -871.0 | -727.7 | |
| 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. | |