SDO HMI 2011-08-28 19:59:08 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.79 | 28.93 | 0.90 | 14.61 | 16.98 | 327.01 | -1.51 | 324.99 | 0.1861 | 324.4 | 261.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 3.05 | 0.00 | 1.54 | 17.62 | 332.54 | 4.03 | 339.87 | 0.1953 | -994.0 | -792.5 | |
| 0.00 | 1.16 | 0.00 | 0.59 | 17.69 | 332.26 | 3.74 | 341.29 | 0.1947 | -1046.0 | -800.2 | |
| 0.00 | 3.05 | 0.00 | 1.55 | 19.49 | 329.28 | 0.76 | 356.66 | 0.2156 | -1213.0 | -847.8 | |
| 0.00 | 1.43 | 0.00 | 0.73 | 19.21 | 328.67 | 0.15 | 359.32 | 0.2104 | -926.0 | -642.2 | |
| 1.79 | 7.17 | 0.90 | 3.61 | 17.27 | 328.45 | -0.07 | 0.39 | 0.1770 | 1027.5 | 915.0 | |
| 0.00 | 2.42 | 0.00 | 1.21 | 15.89 | 326.59 | -1.93 | 11.99 | 0.1565 | 977.0 | 821.6 | |
| 0.00 | 2.15 | 0.00 | 1.08 | 17.05 | 326.51 | -2.00 | 10.97 | 0.1765 | 836.0 | 600.9 | |
| 0.00 | 0.72 | 0.00 | 0.36 | 16.84 | 326.52 | -2.00 | 11.20 | 0.1729 | 913.0 | 687.4 | |
| 0.00 | 1.25 | 0.00 | 0.63 | 15.48 | 325.43 | -3.09 | 19.63 | 0.1552 | 729.0 | 544.9 | |
| 0.00 | 0.63 | 0.00 | 0.32 | 21.33 | 323.01 | -5.51 | 19.98 | 0.2629 | 731.0 | 579.0 | |
| 0.00 | 1.16 | 0.00 | 0.59 | 14.38 | 322.22 | -6.30 | 39.92 | 0.1664 | 827.0 | 647.8 | |
| 0.00 | 2.06 | 0.00 | 1.03 | 13.16 | 321.88 | -6.64 | 46.76 | 0.1554 | 1009.0 | 782.6 | |
| 0.00 | 1.16 | 0.00 | 0.60 | 18.67 | 319.92 | -8.60 | 35.11 | 0.2475 | 837.0 | 769.7 | |
| 0.00 | 1.52 | 0.00 | 0.77 | 13.55 | 319.57 | -8.95 | 53.14 | 0.1898 | 905.0 | 644.2 | |
| 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. | |