| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 15.06 | 93.68 | 37.45 | 246.87 | -16.80 | 106.31 | 77.67 | 252.21 | 0.9813 | 62.4 | 17.0 | |
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back to the solar disc SDO HMI 2011-11-14 02:58:58 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 3.87 | 64.09 | 11.95 | 196.52 | -16.18 | 108.06 | 79.42 | 253.06 | 0.9876 | 364.3 | 27.9 | |
| 2.06 | -1.00 | 6.38 | -1.00 | -16.78 | 108.16 | 79.53 | 252.47 | 0.9881 | -369.2 | 999999 | |
| 3.36 | -1.00 | 10.03 | -1.00 | -16.67 | 107.81 | 79.17 | 252.54 | 0.9871 | 356.2 | 999999 | |
| 0.00 | 0.52 | 0.00 | 1.39 | -17.57 | 106.49 | 77.85 | 251.49 | 0.9837 | 312.0 | 401.2 | |
| 0.00 | 0.77 | 0.00 | 2.08 | -17.98 | 106.50 | 77.87 | 251.08 | 0.9839 | 460.0 | 418.0 | |
| 0.00 | 1.46 | 0.00 | 3.42 | -18.86 | 104.68 | 76.04 | 249.97 | 0.9785 | 47.0 | 32.6 | |
| 0.00 | 1.29 | 0.00 | 2.72 | -17.94 | 103.36 | 74.72 | 250.74 | 0.9732 | 326.0 | 290.7 | |
| 0.00 | 0.95 | 0.00 | 1.74 | -18.29 | 101.06 | 72.42 | 250.05 | 0.9641 | 198.0 | 172.3 | |
| 0.00 | 0.86 | 0.00 | 1.57 | -18.63 | 100.90 | 72.26 | 249.68 | 0.9636 | -17.0 | -31.2 | |
| 2.84 | 7.57 | 4.37 | 11.69 | -17.15 | 97.88 | 69.24 | 250.73 | 0.9479 | -446.8 | -175.6 | |
| 0.00 | 6.97 | 0.00 | 11.35 | -18.27 | 98.86 | 70.22 | 249.73 | 0.9539 | 353.0 | 172.6 | |
| 2.93 | 5.76 | 4.72 | 9.31 | -18.83 | 98.64 | 70.00 | 249.12 | 0.9533 | -375.2 | -343.6 | |
| 0.00 | 3.44 | 0.00 | 5.08 | -17.30 | 97.04 | 68.40 | 250.44 | 0.9436 | -690.0 | -554.0 | |
| 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. | |