SDO HMI 2014-07-20 07:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 39.68 | 165.66 | 21.92 | 91.69 | -21.38 | 67.94 | 2.51 | 185.31 | 0.4460 | 362.6 | 9.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 15.25 | 82.60 | 8.44 | 45.73 | -21.36 | 69.47 | 4.03 | 188.45 | 0.4475 | 1144.4 | 339.8 | |
| 1.36 | -1.00 | 0.75 | -1.00 | -20.95 | 69.36 | 3.92 | 188.36 | 0.4409 | 1092.3 | 999999 | |
| 0.00 | 2.00 | 0.00 | 1.10 | -20.71 | 69.32 | 3.88 | 188.37 | 0.4371 | 1089.0 | 883.3 | |
| 2.72 | -1.00 | 1.50 | -1.00 | -21.08 | 69.10 | 3.66 | 187.78 | 0.4424 | 1085.3 | 999999 | |
| 1.82 | -1.00 | 1.00 | -1.00 | -21.18 | 68.94 | 3.50 | 187.41 | 0.4436 | 746.0 | 999999 | |
| 6.54 | 25.05 | 3.60 | 13.79 | -20.74 | 68.70 | 3.26 | 187.04 | 0.4363 | 1114.0 | 638.8 | |
| 0.73 | -6.00 | 0.40 | -6.00 | -20.57 | 68.34 | 2.90 | 186.31 | 0.4329 | 995.9 | 999999 | |
| 0.00 | 1.09 | 0.00 | 0.60 | -21.79 | 67.60 | 2.17 | 184.49 | 0.4509 | -319.0 | -419.4 | |
| 0.00 | 1.27 | 0.00 | 0.71 | -21.99 | 66.03 | 0.59 | 181.22 | 0.4528 | -687.0 | -498.4 | |
| 4.18 | 22.97 | 2.31 | 12.70 | -21.51 | 65.86 | 0.43 | 180.90 | 0.4453 | -1125.0 | -655.1 | |
| 5.17 | -10.00 | 2.86 | -10.00 | -21.68 | 65.70 | 0.26 | 180.55 | 0.4479 | -1091.2 | 999999 | |
| 0.00 | 2.09 | 0.00 | 1.16 | -22.33 | 65.70 | 0.26 | 180.54 | 0.4580 | -743.0 | -614.8 | |
| 0.00 | 1.72 | 0.00 | 0.96 | -22.53 | 65.50 | 0.07 | 180.13 | 0.4612 | -535.0 | -423.7 | |
| 1.91 | 26.87 | 1.06 | 14.94 | -21.98 | 65.14 | -0.29 | 179.39 | 0.4527 | -1147.9 | -824.7 | |
| 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. | |