SDO HMI 2011-08-28 05:59:08 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 12.47 | 36.54 | 6.33 | 18.56 | 17.58 | 328.37 | -7.86 | 35.47 | 0.2286 | 137.4 | -76.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.90 | 0.00 | 0.45 | 18.06 | 332.01 | -4.22 | 20.22 | 0.2035 | -899.0 | -734.3 | |
| 0.00 | 0.99 | 0.00 | 0.50 | 17.75 | 331.76 | -4.47 | 21.89 | 0.2001 | -953.0 | -713.3 | |
| 0.00 | 1.35 | 0.00 | 0.68 | 18.49 | 331.68 | -4.56 | 20.87 | 0.2123 | -849.0 | -692.5 | |
| 0.00 | 1.08 | 0.00 | 0.54 | 17.96 | 331.24 | -4.99 | 23.69 | 0.2068 | -913.0 | -809.7 | |
| 0.00 | 1.26 | 0.00 | 0.64 | 19.11 | 329.60 | -6.63 | 27.62 | 0.2365 | -938.0 | -703.5 | |
| 2.06 | 2.69 | 1.05 | 1.37 | 19.32 | 329.01 | -7.22 | 29.20 | 0.2443 | -1003.7 | -920.9 | |
| 0.00 | 6.37 | 0.00 | 3.25 | 19.22 | 328.69 | -7.54 | 30.46 | 0.2456 | -776.0 | -693.4 | |
| 6.46 | 15.52 | 3.28 | 7.88 | 17.12 | 328.55 | -7.68 | 36.14 | 0.2174 | 1117.6 | 837.6 | |
| 3.95 | -8.00 | 2.00 | -8.00 | 16.99 | 328.34 | -7.89 | 37.26 | 0.2179 | 1025.7 | 999999 | |
| 0.00 | 1.08 | 0.00 | 0.55 | 19.08 | 327.37 | -8.86 | 34.92 | 0.2556 | -802.0 | -684.6 | |
| 0.00 | 0.36 | 0.00 | 0.18 | 16.94 | 326.90 | -9.33 | 42.02 | 0.2328 | 658.0 | 494.5 | |
| 0.00 | 1.44 | 0.00 | 0.73 | 16.72 | 325.14 | -11.09 | 47.47 | 0.2511 | 999.0 | 783.9 | |
| 0.00 | 2.51 | 0.00 | 1.28 | 13.50 | 324.99 | -11.24 | 59.08 | 0.2219 | 773.0 | 666.7 | |
| 0.00 | 0.63 | 0.00 | 0.32 | 12.31 | 323.75 | -12.48 | 66.14 | 0.2319 | 789.0 | 676.6 | |
| 0.00 | 0.36 | 0.00 | 0.19 | 22.70 | 319.97 | -16.26 | 43.39 | 0.3775 | 767.0 | 718.5 | |
| 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. | |