SDO HMI 2011-08-28 10:59:08 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 8.70 | 43.51 | 4.39 | 22.03 | 18.18 | 330.05 | -3.43 | 355.25 | 0.2082 | 151.6 | -27.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.24 | 0.00 | 1.12 | 14.89 | 337.23 | 3.74 | 335.06 | 0.1503 | 592.0 | 477.2 | |
| 0.00 | 1.52 | 0.00 | 0.78 | 22.17 | 334.35 | 0.86 | 356.93 | 0.2614 | 811.0 | 573.3 | |
| 0.00 | 2.06 | 0.00 | 1.07 | 24.06 | 333.63 | 0.15 | 359.54 | 0.2928 | 925.0 | 775.8 | |
| 0.00 | 1.17 | 0.00 | 0.60 | 24.15 | 333.37 | -0.12 | 0.37 | 0.2944 | 723.0 | 626.8 | |
| 0.00 | 1.08 | 0.00 | 0.54 | 18.12 | 332.48 | -1.01 | 5.00 | 0.1927 | -835.0 | -668.1 | |
| 0.00 | 3.41 | 0.00 | 1.72 | 17.72 | 332.33 | -1.16 | 6.00 | 0.1861 | -747.0 | -622.0 | |
| 0.00 | 1.17 | 0.00 | 0.59 | 18.03 | 331.78 | -1.71 | 8.50 | 0.1925 | -808.0 | -644.5 | |
| 0.00 | 2.24 | 0.00 | 1.13 | 18.34 | 331.68 | -1.81 | 8.73 | 0.1980 | -825.0 | -567.7 | |
| 0.00 | 1.08 | 0.00 | 0.54 | 16.49 | 331.54 | -1.95 | 11.29 | 0.1671 | -924.0 | -665.0 | |
| 0.00 | 4.04 | 0.00 | 2.05 | 19.43 | 329.13 | -4.36 | 18.53 | 0.2265 | -903.0 | -807.9 | |
| 0.00 | 3.32 | 0.00 | 1.69 | 19.12 | 328.69 | -4.80 | 20.76 | 0.2240 | -980.0 | -669.6 | |
| 5.11 | 14.80 | 2.58 | 7.47 | 17.21 | 328.58 | -4.91 | 24.93 | 0.1947 | 1030.9 | 780.4 | |
| 3.59 | -12.00 | 1.81 | -12.00 | 17.08 | 328.36 | -5.13 | 26.19 | 0.1944 | 1046.6 | 999999 | |
| 0.00 | 1.08 | 0.00 | 0.55 | 18.40 | 327.97 | -5.52 | 24.91 | 0.2175 | 761.0 | 674.3 | |
| 0.00 | 1.70 | 0.00 | 0.87 | 19.17 | 327.30 | -6.19 | 25.90 | 0.2341 | -924.0 | -719.7 | |
| 0.00 | 0.72 | 0.00 | 0.36 | 16.66 | 324.94 | -8.55 | 40.41 | 0.2208 | 773.0 | 630.6 | |
| 0.00 | 1.88 | 0.00 | 0.95 | 13.42 | 325.00 | -8.49 | 52.20 | 0.1825 | 747.0 | 582.0 | |
| 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. | |