SDO HMI 2011-10-21 03:59:01 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 11.24 | 45.39 | 6.01 | 24.34 | 17.56 | 325.43 | -19.13 | 55.33 | 0.3811 | 264.2 | 95.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.39 | 0.00 | 0.73 | 14.64 | 327.66 | -16.90 | 59.75 | 0.3271 | 980.0 | 715.9 | |
| 3.66 | 14.20 | 1.94 | 7.54 | 17.26 | 326.84 | -17.72 | 54.23 | 0.3598 | -1055.5 | -738.0 | |
| 0.00 | 1.05 | 0.00 | 0.56 | 18.02 | 326.43 | -18.13 | 53.07 | 0.3718 | 988.0 | 793.2 | |
| 2.70 | 4.97 | 1.43 | 2.64 | 17.01 | 326.50 | -18.06 | 55.30 | 0.3621 | -793.6 | -232.5 | |
| 0.00 | 0.96 | 0.00 | 0.51 | 16.79 | 326.42 | -18.14 | 55.92 | 0.3614 | -87.0 | -77.5 | |
| 0.00 | 0.96 | 0.00 | 0.51 | 16.99 | 325.91 | -18.65 | 56.13 | 0.3699 | -596.0 | -420.3 | |
| 2.18 | 4.79 | 1.17 | 2.57 | 18.15 | 325.59 | -18.97 | 53.93 | 0.3839 | 839.9 | 682.2 | |
| 0.00 | 2.00 | 0.00 | 1.07 | 16.86 | 325.53 | -19.03 | 56.94 | 0.3740 | 721.0 | 524.8 | |
| 0.70 | 3.57 | 0.37 | 1.92 | 17.95 | 325.08 | -19.48 | 55.03 | 0.3889 | 1005.2 | 726.8 | |
| 0.00 | 4.09 | 0.00 | 2.21 | 18.39 | 324.49 | -20.07 | 54.80 | 0.4002 | 1113.0 | 765.9 | |
| 0.00 | 0.96 | 0.00 | 0.52 | 17.47 | 324.60 | -19.96 | 56.67 | 0.3914 | 775.0 | 609.0 | |
| 0.87 | 3.48 | 0.48 | 1.91 | 19.20 | 322.83 | -21.73 | 55.05 | 0.4283 | 1014.7 | 898.4 | |
| 1.13 | 1.31 | 0.62 | 0.72 | 19.41 | 322.77 | -21.79 | 54.69 | 0.4309 | 741.3 | 651.5 | |
| 0.00 | 1.66 | 0.00 | 0.93 | 16.05 | 318.16 | -26.40 | 65.60 | 0.4711 | -802.0 | -592.4 | |
| 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. | |