| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 32.62 | 171.65 | 52.22 | 275.95 | -15.60 | 267.08 | -70.47 | 107.34 | 0.9515 | 206.6 | -14.5 | |
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back to the solar disc SDO HMI 2011-11-17 23:58:57 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 11.33 | 69.12 | 16.02 | 98.21 | -16.54 | 269.83 | -67.72 | 108.72 | 0.9381 | 617.1 | 99.3 | |
| 2.32 | -1.00 | 3.31 | -1.00 | -16.52 | 269.60 | -67.95 | 108.66 | 0.9395 | -292.7 | 999999 | |
| 0.00 | 2.49 | 0.00 | 3.84 | -17.67 | 268.16 | -69.40 | 109.64 | 0.9484 | 218.0 | 182.2 | |
| 4.46 | 9.87 | 6.88 | 15.28 | -17.33 | 268.09 | -69.46 | 109.27 | 0.9484 | 382.5 | -215.2 | |
| 0.00 | 2.40 | 0.00 | 3.74 | -16.81 | 267.80 | -69.75 | 108.69 | 0.9495 | -523.0 | -505.5 | |
| 0.00 | 3.01 | 0.00 | 4.78 | -16.58 | 267.36 | -70.20 | 108.38 | 0.9516 | -478.0 | -404.6 | |
| 0.00 | 1.55 | 0.00 | 2.37 | -15.87 | 267.93 | -69.63 | 107.72 | 0.9481 | -319.0 | -326.8 | |
| 0.00 | 1.89 | 0.00 | 3.21 | -16.20 | 266.06 | -71.50 | 107.80 | 0.9577 | -469.0 | -417.0 | |
| 0.00 | 1.29 | 0.00 | 2.25 | -16.11 | 265.44 | -72.11 | 107.61 | 0.9606 | -422.0 | -354.1 | |
| 5.41 | 47.14 | 8.72 | 76.48 | -14.16 | 266.74 | -70.82 | 105.77 | 0.9530 | 571.5 | 174.4 | |
| 0.00 | 1.29 | 0.00 | 2.35 | -16.13 | 264.79 | -72.77 | 107.56 | 0.9635 | -481.0 | -435.3 | |
| 2.92 | -10.00 | 4.72 | -10.00 | -13.71 | 266.60 | -70.96 | 105.28 | 0.9534 | 386.4 | 999999 | |
| 0.69 | 4.64 | 1.25 | 8.52 | -15.70 | 264.77 | -72.78 | 107.11 | 0.9634 | 69.9 | -212.7 | |
| 1.63 | 8.93 | 3.52 | 19.30 | -17.77 | 262.33 | -75.22 | 108.93 | 0.9745 | -140.1 | -169.3 | |
| 0.00 | 2.15 | 0.00 | 3.56 | -13.54 | 266.14 | -71.42 | 105.05 | 0.9556 | -241.0 | -256.1 | |
| 3.86 | 15.88 | 7.80 | 32.06 | -13.90 | 262.86 | -74.69 | 105.03 | 0.9706 | -358.3 | -332.2 | |
| 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. | |