| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 22.96 | 67.39 | 12.75 | 37.51 | 19.81 | 63.17 | 5.76 | 348.03 | 0.4578 | 666.6 | 503.7 | |
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back to the solar disc SDO HMI 2011-02-12 08:58:57 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.63 | 3.34 | 0.91 | 1.87 | 19.95 | 65.65 | 8.24 | 343.24 | 0.4691 | -849.9 | -686.2 | |
| 0.00 | 1.88 | 0.00 | 1.05 | 19.78 | 65.54 | 8.14 | 343.33 | 0.4661 | -823.0 | -785.2 | |
| 0.00 | 0.94 | 0.00 | 0.52 | 18.97 | 64.02 | 6.61 | 345.86 | 0.4477 | 685.0 | 575.9 | |
| 2.14 | 41.19 | 1.18 | 22.86 | 19.03 | 63.74 | 6.33 | 346.47 | 0.4476 | 928.4 | 562.8 | |
| 1.80 | -4.00 | 1.00 | -4.00 | 19.12 | 63.55 | 6.15 | 346.91 | 0.4484 | 1159.0 | 999999 | |
| 3.85 | -4.00 | 2.14 | -4.00 | 19.38 | 63.34 | 5.93 | 347.47 | 0.4516 | 1010.9 | 999999 | |
| 0.69 | -4.00 | 0.38 | -4.00 | 19.78 | 63.17 | 5.76 | 348.02 | 0.4570 | -199.1 | 999999 | |
| 12.16 | -4.00 | 6.76 | -4.00 | 19.74 | 63.01 | 5.60 | 348.33 | 0.4560 | 905.7 | 999999 | |
| 0.00 | 1.71 | 0.00 | 0.95 | 19.94 | 62.67 | 5.26 | 349.11 | 0.4579 | 827.0 | 773.2 | |
| 0.69 | 7.36 | 0.38 | 4.12 | 20.27 | 62.65 | 5.24 | 349.29 | 0.4629 | 921.0 | 691.4 | |
| 0.00 | 2.31 | 0.00 | 1.29 | 20.04 | 62.48 | 5.07 | 349.53 | 0.4589 | 930.0 | 865.3 | |
| 0.00 | 3.00 | 0.00 | 1.68 | 20.60 | 62.44 | 5.03 | 349.85 | 0.4674 | 632.0 | 540.6 | |
| 0.00 | 2.57 | 0.00 | 1.44 | 20.56 | 62.18 | 4.77 | 350.34 | 0.4661 | 591.0 | 626.8 | |
| 0.00 | 1.63 | 0.00 | 0.91 | 20.30 | 62.08 | 4.67 | 350.44 | 0.4618 | 830.0 | 605.2 | |
| 0.00 | 1.46 | 0.00 | 0.82 | 20.86 | 62.00 | 4.59 | 350.81 | 0.4702 | 729.0 | 545.9 | |
| 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. | |