SDO HMI 2011-08-29 09:59:08 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 22.96 | 0.00 | 11.62 | 16.95 | 325.68 | 4.86 | 336.46 | 0.1971 | 553.1 | 498.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.81 | 0.00 | 0.42 | 17.22 | 334.22 | 13.39 | 308.89 | 0.2854 | -669.0 | -550.9 | |
| 0.00 | 1.52 | 0.00 | 0.78 | 17.04 | 331.48 | 10.66 | 314.57 | 0.2493 | -830.0 | -650.2 | |
| 0.00 | 1.26 | 0.00 | 0.64 | 17.50 | 328.55 | 7.72 | 324.70 | 0.2228 | 1104.0 | 772.5 | |
| 0.00 | 1.17 | 0.00 | 0.60 | 22.01 | 328.02 | 7.19 | 335.76 | 0.2839 | -800.0 | -535.5 | |
| 0.00 | 1.79 | 0.00 | 0.91 | 16.63 | 327.31 | 6.48 | 326.88 | 0.1988 | 747.0 | 622.6 | |
| 0.00 | 4.21 | 0.00 | 2.13 | 16.51 | 327.02 | 6.19 | 327.72 | 0.1944 | 952.0 | 816.0 | |
| 0.00 | 1.17 | 0.00 | 0.59 | 17.19 | 326.69 | 5.86 | 330.90 | 0.2015 | 935.0 | 740.3 | |
| 0.00 | 1.52 | 0.00 | 0.77 | 17.46 | 326.63 | 5.80 | 331.81 | 0.2051 | 899.0 | 670.3 | |
| 0.00 | 1.43 | 0.00 | 0.72 | 15.95 | 324.47 | 3.64 | 338.31 | 0.1660 | 831.0 | 587.0 | |
| 0.00 | 1.17 | 0.00 | 0.59 | 20.21 | 324.27 | 3.44 | 346.03 | 0.2344 | 819.0 | 655.2 | |
| 0.00 | 1.70 | 0.00 | 0.85 | 14.34 | 323.38 | 2.55 | 341.05 | 0.1334 | 890.0 | 781.8 | |
| 0.00 | 1.52 | 0.00 | 0.76 | 13.18 | 322.03 | 1.20 | 349.06 | 0.1079 | 839.0 | 632.9 | |
| 0.00 | 1.26 | 0.00 | 0.63 | 14.77 | 320.97 | 0.14 | 358.95 | 0.1336 | 771.0 | 513.6 | |
| 0.00 | 1.17 | 0.00 | 0.59 | 18.33 | 320.08 | -0.75 | 3.64 | 0.1955 | 926.0 | 671.8 | |
| 0.00 | 1.26 | 0.00 | 0.64 | 19.44 | 319.02 | -1.81 | 7.95 | 0.2163 | 882.0 | 663.1 | |
| 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. | |