SDO HMI 2014-11-06 18:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 16.23 | 0.00 | 9.50 | -21.63 | 79.16 | 19.15 | 215.36 | 0.5336 | 471.4 | 416.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.21 | 0.00 | 0.77 | -27.00 | 84.40 | 24.39 | 215.98 | 0.6287 | -743.0 | -577.3 | |
| 0.00 | 1.38 | 0.00 | 0.81 | -19.77 | 82.65 | 22.65 | 222.52 | 0.5383 | 767.0 | 637.6 | |
| 0.00 | 1.12 | 0.00 | 0.66 | -20.32 | 82.70 | 22.70 | 221.85 | 0.5445 | 563.0 | 459.2 | |
| 0.00 | 0.95 | 0.00 | 0.56 | -20.16 | 82.61 | 22.60 | 221.95 | 0.5419 | 731.0 | 580.4 | |
| 0.00 | 1.21 | 0.00 | 0.71 | -20.38 | 82.47 | 22.46 | 221.49 | 0.5429 | 732.0 | 595.0 | |
| 0.00 | 1.04 | 0.00 | 0.61 | -19.69 | 82.33 | 22.33 | 222.22 | 0.5344 | 813.0 | 620.9 | |
| 0.00 | 3.11 | 0.00 | 1.81 | -20.97 | 80.27 | 20.26 | 217.90 | 0.5285 | 835.0 | 665.9 | |
| 0.00 | 1.21 | 0.00 | 0.71 | -22.56 | 80.51 | 20.50 | 216.30 | 0.5485 | 546.0 | 389.3 | |
| 0.00 | 1.29 | 0.00 | 0.74 | -20.76 | 78.42 | 18.42 | 215.59 | 0.5096 | 620.0 | 505.9 | |
| 0.00 | 1.21 | 0.00 | 0.69 | -21.27 | 76.18 | 16.18 | 211.63 | 0.4970 | 618.0 | 543.0 | |
| 0.00 | 0.86 | 0.00 | 0.48 | -18.20 | 75.12 | 15.11 | 213.61 | 0.4494 | 736.0 | 607.2 | |
| 0.00 | 0.69 | 0.00 | 0.39 | -22.11 | 73.56 | 13.55 | 206.50 | 0.4885 | 597.0 | 550.9 | |
| 0.00 | 0.95 | 0.00 | 0.56 | -28.73 | 58.36 | -1.65 | 177.31 | 0.5406 | -687.0 | -512.0 | |
| 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. | |