SDO HMI 2014-07-09 10:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 42.70 | 205.23 | 42.96 | 205.71 | -11.91 | 267.93 | 58.58 | 253.98 | 0.8705 | 113.4 | -106.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.91 | 0.00 | 1.01 | -12.40 | 271.10 | 61.75 | 254.13 | 0.8962 | 272.0 | 258.6 | |
| 1.73 | 3.18 | 1.85 | 3.41 | -12.37 | 270.11 | 60.75 | 253.96 | 0.8886 | 496.5 | 387.4 | |
| 21.62 | 99.02 | 22.38 | 102.88 | -10.57 | 269.33 | 59.98 | 255.81 | 0.8798 | 724.2 | 96.6 | |
| 1.09 | -3.00 | 1.10 | -3.00 | -10.55 | 268.59 | 59.23 | 255.68 | 0.8738 | 668.7 | 999999 | |
| 0.00 | 0.82 | 0.00 | 0.85 | -14.01 | 268.94 | 59.58 | 251.88 | 0.8823 | -288.0 | -266.7 | |
| 0.00 | 0.45 | 0.00 | 0.46 | -12.38 | 268.17 | 58.82 | 253.53 | 0.8733 | 368.0 | 302.2 | |
| 0.00 | 1.91 | 0.00 | 1.91 | -12.33 | 267.85 | 58.50 | 253.51 | 0.8706 | 440.0 | 324.3 | |
| 0.00 | 0.27 | 0.00 | 0.27 | -11.08 | 267.43 | 58.08 | 254.83 | 0.8650 | 451.0 | 385.0 | |
| 0.00 | 1.18 | 0.00 | 1.12 | -8.63 | 266.64 | 57.28 | 257.48 | 0.8541 | 428.0 | 448.3 | |
| 0.00 | 0.91 | 0.00 | 0.85 | -8.58 | 266.23 | 56.87 | 257.46 | 0.8504 | 455.0 | 447.1 | |
| 0.00 | 1.64 | 0.00 | 1.52 | -9.27 | 265.88 | 56.53 | 256.58 | 0.8484 | 557.0 | 454.9 | |
| 0.64 | 1.36 | 0.63 | 1.36 | -13.95 | 267.33 | 57.97 | 251.57 | 0.8692 | -352.6 | -269.0 | |
| 17.62 | 93.03 | 17.00 | 89.56 | -13.48 | 266.32 | 56.97 | 251.85 | 0.8600 | -825.4 | -381.6 | |
| 0.00 | 0.55 | 0.00 | 0.51 | -14.20 | 264.99 | 55.64 | 250.68 | 0.8501 | -399.0 | -368.3 | |
| 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. | |