SDO HMI 2014-07-06 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 |
| 1.27 | 30.44 | 0.67 | 15.94 | -14.05 | 255.37 | 7.41 | 202.24 | 0.3293 | 356.4 | 444.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.18 | 0.00 | 1.15 | -13.68 | 259.50 | 11.54 | 213.55 | 0.3532 | 1009.0 | 700.1 | |
| 0.00 | 1.45 | 0.00 | 0.77 | -13.51 | 259.20 | 11.24 | 213.13 | 0.3484 | 882.0 | 720.6 | |
| 0.00 | 0.82 | 0.00 | 0.43 | -13.83 | 259.16 | 11.19 | 212.51 | 0.3523 | 750.0 | 595.0 | |
| 0.00 | 1.73 | 0.00 | 0.91 | -14.21 | 258.50 | 10.54 | 210.41 | 0.3519 | 690.0 | 614.6 | |
| 0.00 | 1.18 | 0.00 | 0.62 | -13.98 | 258.43 | 10.47 | 210.57 | 0.3481 | 938.0 | 744.6 | |
| 0.00 | 1.54 | 0.00 | 0.82 | -14.33 | 258.35 | 10.39 | 209.86 | 0.3524 | 618.0 | 548.1 | |
| 0.00 | 1.91 | 0.00 | 0.99 | -12.33 | 255.96 | 7.99 | 206.61 | 0.3047 | 836.0 | 681.4 | |
| 1.27 | 9.99 | 0.67 | 5.25 | -14.46 | 255.39 | 7.43 | 202.19 | 0.3329 | 1039.4 | 842.9 | |
| 0.00 | 1.82 | 0.00 | 0.95 | -14.67 | 254.16 | 6.20 | 198.59 | 0.3291 | 1001.0 | 814.2 | |
| 0.00 | 2.09 | 0.00 | 1.09 | -14.50 | 251.88 | 3.92 | 192.13 | 0.3163 | -1034.0 | -819.2 | |
| 0.00 | 1.36 | 0.00 | 0.71 | -14.95 | 251.73 | 3.77 | 191.38 | 0.3230 | -863.0 | -692.7 | |
| 0.00 | 1.64 | 0.00 | 0.85 | -14.81 | 251.28 | 3.32 | 190.14 | 0.3195 | -821.0 | -703.2 | |
| 0.00 | 1.73 | 0.00 | 0.88 | -11.16 | 251.05 | 3.09 | 191.86 | 0.2586 | 990.0 | 819.8 | |
| 0.00 | 1.00 | 0.00 | 0.52 | -14.56 | 250.68 | 2.72 | 188.46 | 0.3137 | -821.0 | -664.7 | |
| 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. | |