SDO HMI 2011-11-20 11:58:57 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 54.56 | 273.20 | 32.24 | 161.68 | -24.17 | 284.15 | -20.48 | 144.36 | 0.5481 | 265.2 | 211.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 38.34 | 210.22 | 22.47 | 123.24 | -24.12 | 285.39 | -19.24 | 145.77 | 0.5367 | 1174.7 | 346.0 | |
| 6.78 | 8.49 | 3.98 | 4.98 | -23.61 | 284.50 | -20.12 | 143.99 | 0.5383 | 812.5 | 676.3 | |
| 0.00 | 1.29 | 0.00 | 0.79 | -27.23 | 283.61 | -21.02 | 146.93 | 0.5866 | 468.0 | 426.1 | |
| 0.00 | 1.80 | 0.00 | 1.03 | -20.52 | 284.39 | -20.24 | 139.89 | 0.5049 | 1013.0 | 805.2 | |
| 0.00 | 2.40 | 0.00 | 1.41 | -23.06 | 283.87 | -20.76 | 142.50 | 0.5378 | 733.0 | 640.7 | |
| 0.60 | 3.52 | 0.36 | 2.08 | -23.92 | 283.59 | -21.04 | 143.18 | 0.5498 | 669.1 | 535.4 | |
| 0.34 | -6.00 | 0.20 | -6.00 | -23.92 | 283.45 | -21.18 | 143.01 | 0.5510 | 684.2 | 999999 | |
| 1.37 | 2.57 | 0.82 | 1.54 | -24.58 | 283.19 | -21.43 | 143.48 | 0.5606 | 670.4 | 238.6 | |
| 0.00 | 1.72 | 0.00 | 0.99 | -20.66 | 283.52 | -21.10 | 138.93 | 0.5149 | 665.0 | 638.7 | |
| 0.00 | 0.69 | 0.00 | 0.41 | -23.43 | 282.98 | -21.65 | 141.83 | 0.5499 | -646.0 | -495.5 | |
| 0.00 | 1.54 | 0.00 | 0.92 | -23.81 | 281.79 | -22.84 | 140.86 | 0.5648 | -607.0 | -470.1 | |
| 0.00 | 1.37 | 0.00 | 0.83 | -24.01 | 281.51 | -23.12 | 140.78 | 0.5695 | -956.0 | -795.2 | |
| 0.00 | 1.97 | 0.00 | 1.19 | -24.16 | 280.84 | -23.79 | 140.19 | 0.5770 | -676.0 | -612.3 | |
| 1.89 | 5.58 | 1.14 | 3.37 | -23.86 | 280.72 | -23.90 | 139.69 | 0.5751 | -926.5 | -741.0 | |
| 0.00 | 1.37 | 0.00 | 0.83 | -24.07 | 280.18 | -24.44 | 139.35 | 0.5822 | -636.0 | -515.9 | |
| 0.00 | 1.29 | 0.00 | 0.78 | -23.91 | 279.93 | -24.70 | 138.87 | 0.5829 | 635.0 | 598.5 | |
| 0.00 | 1.20 | 0.00 | 0.74 | -24.69 | 278.86 | -25.76 | 138.69 | 0.6005 | -807.0 | -669.2 | |
| 0.00 | 1.63 | 0.00 | 1.02 | -25.13 | 278.29 | -26.34 | 138.63 | 0.6100 | -902.0 | -754.2 | |
| 0.00 | 1.03 | 0.00 | 0.65 | -25.34 | 277.80 | -26.83 | 138.39 | 0.6165 | -681.0 | -601.1 | |
| 0.00 | 0.86 | 0.00 | 0.53 | -24.38 | 277.81 | -26.82 | 137.22 | 0.6074 | -796.0 | -625.7 | |
| 3.69 | 7.29 | 2.30 | 4.56 | -24.65 | 277.63 | -26.99 | 137.38 | 0.6115 | -919.6 | -780.7 | |
| 0.26 | -21.00 | 0.16 | -21.00 | -24.75 | 277.39 | -27.24 | 137.27 | 0.6148 | -830.7 | 999999 | |
| 0.00 | 1.03 | 0.00 | 0.65 | -25.09 | 277.27 | -27.35 | 137.56 | 0.6189 | -608.0 | -475.3 | |
| 0.00 | 0.77 | 0.00 | 0.50 | -27.11 | 276.75 | -27.88 | 139.43 | 0.6423 | -706.0 | -628.0 | |
| 0.00 | 1.12 | 0.00 | 0.72 | -26.94 | 276.72 | -27.91 | 139.21 | 0.6410 | -714.0 | -506.2 | |
| 0.00 | 1.12 | 0.00 | 0.72 | -27.22 | 276.53 | -28.09 | 139.35 | 0.6451 | -645.0 | -600.8 | |
| 0.00 | 1.37 | 0.00 | 0.88 | -26.61 | 276.70 | -27.93 | 138.80 | 0.6381 | -540.0 | -456.6 | |
| 0.00 | 1.80 | 0.00 | 1.14 | -25.19 | 277.06 | -27.56 | 137.48 | 0.6218 | -614.0 | -521.9 | |
| 0.00 | 1.20 | 0.00 | 0.78 | -27.22 | 276.42 | -28.21 | 139.24 | 0.6462 | -435.0 | -373.9 | |
| 0.00 | 1.20 | 0.00 | 0.76 | -25.03 | 276.81 | -27.82 | 137.03 | 0.6228 | -802.0 | -618.6 | |
| 1.29 | 1.37 | 0.81 | 0.86 | -24.40 | 276.59 | -28.04 | 136.06 | 0.6192 | -773.9 | -784.0 | |
| 0.00 | 1.12 | 0.00 | 0.70 | -23.77 | 276.70 | -27.92 | 135.39 | 0.6125 | -758.0 | -576.7 | |
| 0.00 | 1.12 | 0.00 | 0.70 | -23.39 | 276.17 | -28.46 | 134.39 | 0.6143 | -646.0 | -473.3 | |
| 0.00 | 1.29 | 0.00 | 0.83 | -25.06 | 274.97 | -29.66 | 135.37 | 0.6404 | -657.0 | -492.7 | |
| 0.00 | 0.86 | 0.00 | 0.55 | -23.53 | 274.17 | -30.46 | 132.76 | 0.6353 | -591.0 | -483.3 | |
| 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. | |