SDO HMI 2011-12-03 17:58:56 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 40.03 | 195.97 | 28.50 | 139.88 | 19.07 | 172.89 | 42.90 | 296.50 | 0.7204 | -147.7 | -39.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 20.31 | 125.34 | 14.92 | 92.17 | 18.77 | 174.86 | 44.88 | 295.22 | 0.7408 | -853.1 | -201.6 | |
| 5.72 | -1.00 | 4.18 | -1.00 | 19.11 | 174.54 | 44.55 | 295.79 | 0.7386 | -847.5 | 999999 | |
| 0.00 | 1.02 | 0.00 | 0.74 | 19.31 | 173.64 | 43.66 | 296.40 | 0.7297 | -674.0 | -539.6 | |
| 0.00 | 2.30 | 0.00 | 1.64 | 18.28 | 173.23 | 43.24 | 295.22 | 0.7214 | -507.0 | -470.5 | |
| 1.45 | 2.82 | 1.03 | 2.00 | 18.31 | 173.02 | 43.03 | 295.35 | 0.7192 | -747.6 | -651.4 | |
| 0.00 | 1.79 | 0.00 | 1.28 | 19.15 | 173.03 | 43.04 | 296.45 | 0.7226 | -834.0 | -687.0 | |
| 0.00 | 0.68 | 0.00 | 0.48 | 18.50 | 172.82 | 42.84 | 295.68 | 0.7178 | -536.0 | -654.9 | |
| 0.00 | 1.37 | 0.00 | 0.96 | 18.78 | 172.32 | 42.33 | 296.26 | 0.7133 | -690.0 | -585.2 | |
| 0.00 | 0.85 | 0.00 | 0.62 | 21.61 | 172.68 | 42.69 | 299.80 | 0.7288 | -482.0 | -399.4 | |
| 0.00 | 0.68 | 0.00 | 0.48 | 20.23 | 171.55 | 41.57 | 298.52 | 0.7109 | -540.0 | -455.6 | |
| 2.05 | 10.15 | 1.38 | 6.87 | 18.27 | 169.68 | 39.69 | 296.76 | 0.6816 | -654.9 | 277.9 | |
| 0.00 | 1.28 | 0.00 | 0.86 | 18.36 | 169.42 | 39.44 | 297.01 | 0.6790 | -674.0 | -532.6 | |
| 0.00 | 0.94 | 0.00 | 0.64 | 20.11 | 169.93 | 39.94 | 299.15 | 0.6927 | 686.0 | 492.8 | |
| 0.00 | 1.45 | 0.00 | 0.99 | 20.55 | 169.86 | 39.88 | 299.78 | 0.6940 | 579.0 | 493.6 | |
| 2.39 | 5.72 | 1.61 | 3.84 | 18.71 | 169.28 | 39.29 | 297.56 | 0.6789 | 681.6 | 410.7 | |
| 1.28 | 2.65 | 0.87 | 1.80 | 19.92 | 169.51 | 39.52 | 299.11 | 0.6871 | -618.3 | -636.3 | |
| 0.34 | -16.00 | 0.23 | -16.00 | 20.02 | 169.45 | 39.47 | 299.27 | 0.6870 | -814.8 | 999999 | |
| 0.00 | 3.07 | 0.00 | 2.09 | 20.49 | 169.35 | 39.36 | 299.96 | 0.6881 | 841.0 | 650.3 | |
| 0.00 | 1.11 | 0.00 | 0.75 | 20.65 | 169.16 | 39.17 | 300.27 | 0.6867 | 795.0 | 631.0 | |
| 0.00 | 0.51 | 0.00 | 0.35 | 20.75 | 168.98 | 38.99 | 300.50 | 0.6853 | 467.0 | 525.5 | |
| 0.00 | 0.60 | 0.00 | 0.40 | 20.75 | 168.82 | 38.83 | 300.58 | 0.6835 | 736.0 | 655.6 | |
| 0.00 | 0.85 | 0.00 | 0.57 | 19.30 | 168.40 | 38.41 | 298.83 | 0.6717 | 440.0 | 290.8 | |
| 0.00 | 1.19 | 0.00 | 0.80 | 20.31 | 168.48 | 38.50 | 300.17 | 0.6776 | 579.0 | 526.7 | |
| 0.00 | 5.55 | 0.00 | 3.75 | 21.00 | 168.65 | 38.66 | 301.02 | 0.6829 | 772.0 | 638.8 | |
| 0.00 | 0.68 | 0.00 | 0.46 | 20.37 | 168.34 | 38.35 | 300.33 | 0.6763 | 680.0 | 507.5 | |
| 0.00 | 1.19 | 0.00 | 0.79 | 19.56 | 167.99 | 38.00 | 299.40 | 0.6683 | 435.0 | 341.7 | |
| 0.00 | 1.11 | 0.00 | 0.74 | 19.65 | 167.85 | 37.87 | 299.61 | 0.6672 | 533.0 | 352.5 | |
| 4.27 | 9.04 | 2.82 | 5.97 | 19.37 | 167.66 | 37.67 | 299.32 | 0.6636 | 645.5 | 588.6 | |
| 0.00 | 0.77 | 0.00 | 0.51 | 20.72 | 167.96 | 37.97 | 301.02 | 0.6739 | 612.0 | 451.2 | |
| 2.22 | 2.47 | 1.46 | 1.62 | 19.56 | 167.16 | 37.17 | 299.87 | 0.6588 | 782.0 | 629.0 | |
| 0.00 | 2.99 | 0.00 | 1.96 | 20.13 | 167.03 | 37.05 | 300.72 | 0.6604 | 761.0 | 678.4 | |
| 0.00 | 1.28 | 0.00 | 0.84 | 20.22 | 166.75 | 36.76 | 301.02 | 0.6576 | 904.0 | 701.0 | |
| 0.00 | 1.71 | 0.00 | 1.11 | 20.22 | 166.24 | 36.25 | 301.33 | 0.6519 | 812.0 | 693.2 | |
| 0.00 | 1.02 | 0.00 | 0.65 | 19.64 | 165.04 | 35.05 | 301.23 | 0.6348 | 774.0 | 663.8 | |
| 0.00 | 1.79 | 0.00 | 1.15 | 20.80 | 165.07 | 35.08 | 302.86 | 0.6419 | 761.0 | 610.5 | |
| 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. | |