| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 64.60 | 408.76 | 115.78 | 748.03 | 10.09 | 69.88 | 72.47 | 282.68 | 0.9613 | 122.3 | 18.0 | |
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back to the solar disc SDO HMI 2013-02-22 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 |
| 7.83 | 169.63 | 18.95 | 394.96 | 9.86 | 74.11 | 76.69 | 281.66 | 0.9799 | 614.1 | -94.5 | |
| 18.15 | -1.00 | 41.27 | -1.00 | 9.72 | 73.23 | 75.82 | 281.67 | 0.9768 | -687.2 | 999999 | |
| 0.00 | 3.10 | 0.00 | 7.00 | 11.48 | 72.82 | 75.40 | 283.52 | 0.9764 | -125.0 | -66.0 | |
| 0.00 | 1.12 | 0.00 | 2.18 | 9.32 | 71.23 | 73.81 | 281.61 | 0.9686 | -561.0 | -523.5 | |
| 0.00 | 1.12 | 0.00 | 2.16 | 9.48 | 70.99 | 73.57 | 281.81 | 0.9677 | -543.0 | -494.6 | |
| 0.00 | 0.60 | 0.00 | 1.19 | 9.84 | 71.21 | 73.79 | 282.14 | 0.9689 | -394.0 | -414.7 | |
| 0.00 | 2.75 | 0.00 | 5.00 | 8.92 | 70.16 | 72.74 | 281.39 | 0.9636 | -563.0 | -473.5 | |
| 0.00 | 1.12 | 0.00 | 1.99 | 10.34 | 69.52 | 72.10 | 282.96 | 0.9619 | -212.0 | -214.3 | |
| 0.00 | 0.60 | 0.00 | 1.08 | 11.23 | 69.46 | 72.04 | 283.88 | 0.9624 | -534.0 | -510.0 | |
| 0.00 | 2.67 | 0.00 | 4.54 | 10.43 | 68.69 | 71.27 | 283.21 | 0.9580 | 55.0 | -25.6 | |
| 0.00 | 4.73 | 0.00 | 7.61 | 9.26 | 67.91 | 70.49 | 282.16 | 0.9530 | -303.0 | -258.1 | |
| 4.13 | 27.44 | 6.21 | 41.45 | 9.65 | 66.50 | 69.08 | 282.83 | 0.9459 | 453.1 | 133.3 | |
| 0.00 | 1.63 | 0.00 | 2.71 | 12.08 | 67.79 | 70.37 | 285.08 | 0.9552 | -328.0 | -320.5 | |
| 0.00 | 1.20 | 0.00 | 1.97 | 12.24 | 67.62 | 70.20 | 285.29 | 0.9545 | -236.0 | -150.8 | |
| 4.30 | 191.05 | 6.30 | 274.19 | 10.75 | 65.67 | 68.25 | 284.15 | 0.9426 | -305.4 | 213.9 | |
| 27.70 | -15.00 | 39.60 | -15.00 | 10.57 | 65.18 | 67.76 | 284.06 | 0.9395 | 809.3 | 999999 | |
| 2.49 | -15.00 | 3.45 | -15.00 | 10.84 | 64.35 | 66.93 | 284.53 | 0.9350 | 878.1 | 999999 | |
| 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. | |