SDO HMI 2011-05-29 02:59:10 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 87.20 | 371.52 | 53.71 | 229.98 | 20.83 | 131.90 | 30.15 | 308.38 | 0.6001 | -133.6 | -139.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.08 | 229.38 | 0.69 | 144.58 | 21.61 | 133.85 | 32.10 | 307.78 | 0.6273 | -606.9 | -351.0 | |
| 5.60 | -1.00 | 3.55 | -1.00 | 21.84 | 133.67 | 31.92 | 308.23 | 0.6270 | -837.5 | 999999 | |
| 3.34 | 8.30 | 2.08 | 5.18 | 20.00 | 133.24 | 31.48 | 306.03 | 0.6090 | -797.1 | -418.1 | |
| 27.98 | -1.00 | 17.63 | -1.00 | 21.21 | 133.44 | 31.69 | 307.56 | 0.6200 | -913.7 | 999999 | |
| 0.00 | 1.35 | 0.00 | 0.84 | 19.64 | 132.93 | 31.18 | 305.75 | 0.6030 | 512.0 | 307.0 | |
| 8.40 | -1.00 | 5.26 | -1.00 | 20.85 | 133.16 | 31.41 | 307.27 | 0.6143 | -1041.9 | 999999 | |
| 6.32 | 15.62 | 3.92 | 9.69 | 21.13 | 132.05 | 30.30 | 308.58 | 0.6042 | -1022.6 | -617.4 | |
| 0.00 | 1.90 | 0.00 | 1.18 | 21.56 | 132.11 | 30.36 | 309.13 | 0.6082 | -591.0 | -465.0 | |
| 1.99 | 3.25 | 1.22 | 2.00 | 20.51 | 131.84 | 30.09 | 307.89 | 0.5971 | -867.0 | -668.9 | |
| 0.00 | 1.17 | 0.00 | 0.72 | 19.50 | 131.62 | 29.87 | 306.62 | 0.5871 | 274.0 | 208.6 | |
| 0.00 | 1.35 | 0.00 | 0.82 | 19.14 | 131.33 | 29.58 | 306.34 | 0.5811 | 412.0 | 358.8 | |
| 0.00 | 0.63 | 0.00 | 0.39 | 21.06 | 131.47 | 29.72 | 308.98 | 0.5973 | -745.0 | -619.7 | |
| 0.36 | 2.98 | 0.22 | 1.80 | 18.97 | 130.93 | 29.18 | 306.44 | 0.5752 | 690.5 | 555.6 | |
| 0.99 | 3.43 | 0.60 | 2.07 | 18.94 | 130.77 | 29.02 | 306.53 | 0.5732 | 814.5 | 844.8 | |
| 10.11 | 18.87 | 6.11 | 11.41 | 19.55 | 130.56 | 28.81 | 307.62 | 0.5755 | 785.8 | 363.1 | |
| 0.00 | 1.17 | 0.00 | 0.72 | 21.06 | 130.83 | 29.08 | 309.54 | 0.5903 | -674.0 | -606.9 | |
| 2.44 | 7.67 | 1.46 | 4.61 | 19.38 | 129.94 | 28.19 | 307.93 | 0.5671 | 737.4 | 653.3 | |
| 0.00 | 0.81 | 0.00 | 0.48 | 18.70 | 129.52 | 27.77 | 307.29 | 0.5569 | 677.0 | 541.9 | |
| 0.00 | 4.42 | 0.00 | 2.64 | 19.28 | 129.30 | 27.55 | 308.37 | 0.5590 | 716.0 | 668.9 | |
| 0.00 | 1.26 | 0.00 | 0.76 | 21.01 | 129.45 | 27.70 | 310.74 | 0.5749 | 482.0 | 392.8 | |
| 0.00 | 1.53 | 0.00 | 0.91 | 18.73 | 128.98 | 27.23 | 307.84 | 0.5509 | 787.0 | 599.3 | |
| 0.00 | 0.36 | 0.00 | 0.22 | 21.04 | 128.80 | 27.04 | 311.42 | 0.5680 | 630.0 | 555.8 | |
| 3.43 | 3.97 | 2.05 | 2.37 | 20.84 | 128.36 | 26.60 | 311.57 | 0.5615 | 712.2 | 612.3 | |
| 0.00 | 1.08 | 0.00 | 0.64 | 20.25 | 128.14 | 26.38 | 310.94 | 0.5540 | 682.0 | 502.3 | |
| 0.00 | 1.72 | 0.00 | 1.02 | 20.51 | 128.04 | 26.29 | 311.41 | 0.5552 | 803.0 | 648.2 | |
| 0.00 | 2.08 | 0.00 | 1.24 | 20.77 | 127.98 | 26.23 | 311.85 | 0.5569 | 867.0 | 677.6 | |
| 0.00 | 1.44 | 0.00 | 0.85 | 20.21 | 127.62 | 25.87 | 311.40 | 0.5481 | 756.0 | 647.1 | |
| 1.35 | 47.66 | 0.80 | 28.16 | 20.56 | 127.26 | 25.50 | 312.31 | 0.5472 | 927.7 | 496.3 | |
| 2.62 | -28.00 | 1.55 | -28.00 | 20.83 | 127.30 | 25.55 | 312.63 | 0.5501 | 784.4 | 999999 | |
| 1.17 | -28.00 | 0.69 | -28.00 | 20.96 | 127.15 | 25.39 | 312.99 | 0.5496 | 752.8 | 999999 | |
| 4.87 | -28.00 | 2.88 | -28.00 | 20.69 | 126.99 | 25.24 | 312.77 | 0.5455 | 1081.6 | 999999 | |
| 2.35 | 3.79 | 1.35 | 2.18 | 17.58 | 126.41 | 24.66 | 308.65 | 0.5113 | -804.9 | -699.8 | |
| 2.80 | -28.00 | 1.65 | -28.00 | 20.43 | 126.80 | 25.05 | 312.60 | 0.5411 | 900.0 | 999999 | |
| 0.00 | 0.90 | 0.00 | 0.52 | 18.03 | 126.41 | 24.66 | 309.37 | 0.5152 | 457.0 | 326.4 | |
| 0.00 | 2.08 | 0.00 | 1.20 | 18.12 | 126.14 | 24.39 | 309.81 | 0.5129 | 565.0 | 473.3 | |
| 0.00 | 1.35 | 0.00 | 0.78 | 17.99 | 125.91 | 24.16 | 309.85 | 0.5091 | 724.0 | 661.6 | |
| 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. | |