SDO HMI 2011-11-30 19:58:56 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 87.63 | 302.68 | 45.72 | 158.02 | 18.93 | 171.64 | 3.22 | 350.21 | 0.3177 | 23.9 | -99.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.94 | 0.00 | 0.49 | 19.39 | 174.99 | 6.57 | 341.13 | 0.3354 | -710.0 | -526.4 | |
| 1.88 | 142.97 | 0.98 | 74.64 | 18.36 | 174.54 | 6.13 | 341.28 | 0.3171 | -752.8 | -486.4 | |
| 0.00 | 2.90 | 0.00 | 1.53 | 19.64 | 174.31 | 5.89 | 343.20 | 0.3359 | 51.0 | 180.7 | |
| 0.00 | 1.54 | 0.00 | 0.81 | 20.11 | 174.14 | 5.72 | 344.07 | 0.3424 | -798.0 | -568.2 | |
| 24.60 | -2.00 | 12.84 | -2.00 | 18.58 | 173.99 | 5.57 | 343.09 | 0.3177 | -1301.0 | 999999 | |
| 0.00 | 1.02 | 0.00 | 0.54 | 19.73 | 173.62 | 5.20 | 345.15 | 0.3343 | 327.0 | 223.2 | |
| 0.00 | 1.45 | 0.00 | 0.75 | 17.93 | 173.44 | 5.02 | 344.08 | 0.3047 | -250.0 | -229.5 | |
| 5.64 | 7.69 | 2.95 | 4.02 | 18.93 | 173.31 | 4.89 | 345.34 | 0.3200 | -952.2 | -703.2 | |
| 0.00 | 0.68 | 0.00 | 0.36 | 19.02 | 173.00 | 4.58 | 346.30 | 0.3203 | -755.0 | -649.0 | |
| 0.00 | 0.94 | 0.00 | 0.49 | 17.97 | 172.91 | 4.49 | 345.71 | 0.3029 | -783.0 | -613.9 | |
| 0.00 | 1.37 | 0.00 | 0.71 | 18.58 | 172.55 | 4.13 | 347.28 | 0.3116 | -854.0 | -650.8 | |
| 6.23 | 7.35 | 3.25 | 3.83 | 18.86 | 172.46 | 4.04 | 347.74 | 0.3158 | -1004.7 | -770.7 | |
| 4.95 | 10.76 | 2.58 | 5.61 | 18.86 | 171.62 | 3.20 | 350.25 | 0.3131 | -1049.4 | -619.9 | |
| 0.00 | 3.16 | 0.00 | 1.65 | 19.30 | 171.37 | 2.96 | 351.20 | 0.3196 | -507.0 | -688.8 | |
| 3.84 | 8.03 | 2.00 | 4.17 | 18.28 | 171.23 | 2.81 | 351.09 | 0.3024 | 904.3 | 836.4 | |
| 0.00 | 1.79 | 0.00 | 0.94 | 19.33 | 171.09 | 2.68 | 352.04 | 0.3194 | -590.0 | -436.9 | |
| 0.00 | 1.45 | 0.00 | 0.75 | 18.21 | 170.73 | 2.31 | 352.62 | 0.3002 | 1060.0 | 742.2 | |
| 0.00 | 6.23 | 0.00 | 3.24 | 18.49 | 170.67 | 2.26 | 352.93 | 0.3047 | 777.0 | 763.6 | |
| 0.00 | 1.20 | 0.00 | 0.63 | 19.93 | 170.47 | 2.06 | 354.07 | 0.3280 | -727.0 | -620.6 | |
| 0.00 | 1.96 | 0.00 | 1.03 | 20.14 | 170.04 | 1.62 | 355.38 | 0.3309 | -679.0 | -531.5 | |
| 0.00 | 1.11 | 0.00 | 0.58 | 18.68 | 169.83 | 1.42 | 355.60 | 0.3064 | 800.0 | 659.9 | |
| 1.88 | 2.90 | 0.98 | 1.52 | 19.49 | 169.65 | 1.24 | 356.34 | 0.3196 | 859.9 | 845.3 | |
| 0.00 | 1.62 | 0.00 | 0.85 | 19.89 | 169.47 | 1.05 | 356.96 | 0.3261 | 876.0 | 744.1 | |
| 0.00 | 1.37 | 0.00 | 0.71 | 19.24 | 169.34 | 0.92 | 357.23 | 0.3152 | 493.0 | 455.8 | |
| 1.45 | 16.06 | 0.76 | 8.36 | 18.74 | 169.21 | 0.79 | 357.54 | 0.3068 | 1090.5 | 806.9 | |
| 7.43 | -25.00 | 3.87 | -25.00 | 19.02 | 169.06 | 0.64 | 358.05 | 0.3114 | 1121.6 | 999999 | |
| 0.00 | 2.22 | 0.00 | 1.16 | 19.33 | 168.87 | 0.45 | 358.65 | 0.3164 | 992.0 | 790.5 | |
| 0.00 | 1.20 | 0.00 | 0.63 | 20.96 | 168.37 | -0.05 | 0.14 | 0.3433 | 889.0 | 656.7 | |
| 0.00 | 1.54 | 0.00 | 0.80 | 18.84 | 168.34 | -0.08 | 0.25 | 0.3081 | 890.0 | 667.2 | |
| 0.00 | 1.96 | 0.00 | 1.04 | 21.62 | 168.21 | -0.21 | 0.55 | 0.3542 | 755.0 | 610.7 | |
| 4.87 | 5.64 | 2.54 | 2.94 | 19.43 | 167.96 | -0.46 | 1.36 | 0.3180 | 945.8 | 572.0 | |
| 3.76 | 5.47 | 1.97 | 2.87 | 20.14 | 167.74 | -0.68 | 1.94 | 0.3300 | 992.0 | 774.5 | |
| 14.52 | 41.42 | 7.58 | 21.59 | 19.36 | 167.52 | -0.90 | 2.68 | 0.3172 | 1119.8 | 572.4 | |
| 5.21 | -33.00 | 2.71 | -33.00 | 18.96 | 167.52 | -0.89 | 2.73 | 0.3105 | 1105.0 | 999999 | |
| 0.00 | 6.66 | 0.00 | 3.50 | 20.40 | 167.52 | -0.90 | 2.54 | 0.3343 | 733.0 | 707.0 | |
| 0.00 | 6.41 | 0.00 | 3.36 | 20.11 | 167.20 | -1.21 | 3.47 | 0.3299 | 911.0 | 794.1 | |
| 1.37 | 2.39 | 0.71 | 1.25 | 19.24 | 166.52 | -1.90 | 5.69 | 0.3164 | 903.7 | 672.6 | |
| 0.00 | 1.28 | 0.00 | 0.67 | 19.64 | 165.86 | -2.56 | 7.49 | 0.3243 | 686.0 | 583.9 | |
| 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. | |