SDO HMI 2011-10-13 10:59:02 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 58.42 | 261.19 | 36.99 | 164.49 | -14.78 | 118.49 | 32.23 | 236.53 | 0.6197 | 311.8 | 157.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 8.75 | 9.53 | 5.70 | 6.21 | -13.66 | 121.88 | 35.63 | 240.72 | 0.6513 | 663.3 | 562.3 | |
| 1.66 | 2.10 | 1.07 | 1.36 | -13.90 | 121.17 | 34.92 | 239.90 | 0.6445 | 692.3 | 671.2 | |
| 0.00 | 0.87 | 0.00 | 0.56 | -13.35 | 121.04 | 34.78 | 240.57 | 0.6396 | 499.0 | 427.5 | |
| 0.00 | 3.24 | 0.00 | 2.09 | -14.34 | 120.68 | 34.43 | 238.94 | 0.6418 | 678.0 | 577.7 | |
| 0.00 | 1.84 | 0.00 | 1.17 | -13.94 | 120.32 | 34.06 | 239.23 | 0.6349 | 816.0 | 636.0 | |
| 1.57 | 6.39 | 1.00 | 4.06 | -13.64 | 120.08 | 33.82 | 239.48 | 0.6303 | 825.7 | 615.8 | |
| 0.00 | 1.40 | 0.00 | 0.89 | -13.33 | 119.73 | 33.48 | 239.65 | 0.6243 | 849.0 | 736.2 | |
| 35.69 | 167.60 | 22.82 | 107.03 | -14.77 | 119.83 | 33.57 | 237.72 | 0.6347 | 984.5 | 359.3 | |
| 0.00 | 1.14 | 0.00 | 0.74 | -16.63 | 119.80 | 33.55 | 235.20 | 0.6472 | 361.0 | 394.2 | |
| 0.00 | 0.70 | 0.00 | 0.43 | -14.50 | 116.82 | 30.56 | 235.68 | 0.5984 | -723.0 | -650.4 | |
| 0.00 | 1.75 | 0.00 | 1.08 | -14.74 | 116.64 | 30.39 | 235.17 | 0.5982 | -705.0 | -586.7 | |
| 0.00 | 1.05 | 0.00 | 0.65 | -15.40 | 116.46 | 30.20 | 234.08 | 0.6011 | -506.0 | -459.8 | |
| 0.00 | 0.96 | 0.00 | 0.59 | -14.63 | 116.34 | 30.08 | 235.07 | 0.5938 | -781.0 | -636.0 | |
| 0.00 | 1.14 | 0.00 | 0.70 | -15.20 | 116.21 | 29.96 | 234.15 | 0.5967 | -719.0 | -572.7 | |
| 0.00 | 2.71 | 0.00 | 1.64 | -14.35 | 115.19 | 28.94 | 234.44 | 0.5784 | -633.0 | -532.8 | |
| 0.00 | 1.40 | 0.00 | 0.85 | -14.66 | 115.20 | 28.95 | 233.99 | 0.5811 | -807.0 | -690.9 | |
| 0.00 | 0.96 | 0.00 | 0.58 | -14.42 | 114.89 | 28.63 | 234.04 | 0.5755 | -730.0 | -593.7 | |
| 2.01 | 3.59 | 1.21 | 2.15 | -13.69 | 114.75 | 28.50 | 235.00 | 0.5681 | 794.8 | 762.3 | |
| 0.00 | 3.24 | 0.00 | 1.97 | -15.81 | 114.38 | 28.13 | 231.60 | 0.5811 | -615.0 | -579.4 | |
| 0.00 | 3.15 | 0.00 | 1.87 | -13.27 | 114.00 | 27.74 | 234.91 | 0.5559 | 608.0 | 523.6 | |
| 0.00 | 5.42 | 0.00 | 3.28 | -15.66 | 114.12 | 27.86 | 231.53 | 0.5769 | -730.0 | -684.4 | |
| 0.00 | 1.49 | 0.00 | 0.90 | -16.02 | 114.14 | 27.88 | 231.05 | 0.5801 | -828.0 | -616.5 | |
| 6.82 | 8.48 | 4.04 | 5.02 | -12.93 | 113.65 | 27.39 | 235.07 | 0.5490 | 925.3 | 693.7 | |
| 0.00 | 4.37 | 0.00 | 2.66 | -16.47 | 114.13 | 27.88 | 230.43 | 0.5840 | -515.0 | -590.5 | |
| 0.00 | 1.22 | 0.00 | 0.73 | -13.22 | 113.68 | 27.43 | 234.67 | 0.5517 | 661.0 | 589.0 | |
| 0.00 | 1.40 | 0.00 | 0.85 | -16.24 | 114.03 | 27.77 | 230.64 | 0.5808 | -903.0 | -720.8 | |
| 0.00 | 0.87 | 0.00 | 0.53 | -16.75 | 113.93 | 27.68 | 229.84 | 0.5842 | -752.0 | -612.2 | |
| 0.00 | 1.31 | 0.00 | 0.79 | -15.93 | 113.77 | 27.52 | 230.81 | 0.5754 | -725.0 | -644.5 | |
| 0.00 | 0.79 | 0.00 | 0.48 | -17.30 | 113.95 | 27.70 | 229.12 | 0.5892 | -663.0 | -556.6 | |
| 0.00 | 1.40 | 0.00 | 0.86 | -17.69 | 114.02 | 27.76 | 228.66 | 0.5933 | -577.0 | -391.6 | |
| 0.00 | 1.05 | 0.00 | 0.64 | -16.99 | 113.55 | 27.29 | 229.13 | 0.5821 | -375.0 | -451.7 | |
| 0.00 | 0.70 | 0.00 | 0.42 | -15.44 | 112.97 | 26.71 | 230.68 | 0.5622 | -729.0 | -594.1 | |
| 1.92 | 11.46 | 1.15 | 6.83 | -15.65 | 112.58 | 26.32 | 229.98 | 0.5597 | -767.8 | -713.5 | |
| 0.00 | 1.31 | 0.00 | 0.78 | -15.23 | 112.52 | 26.27 | 230.52 | 0.5554 | -975.0 | -822.3 | |
| 0.00 | 1.49 | 0.00 | 0.88 | -14.97 | 112.45 | 26.20 | 230.82 | 0.5523 | -857.0 | -748.6 | |
| 0.00 | 3.67 | 0.00 | 2.22 | -17.76 | 112.05 | 25.80 | 226.52 | 0.5734 | -678.0 | -574.6 | |
| 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. | |