SDO HMI 2011-06-02 00:59:10 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 46.36 | 280.96 | 27.76 | 168.54 | 17.11 | 20.16 | -29.77 | 57.39 | 0.5646 | -332.9 | -291.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.81 | 0.00 | 1.06 | 18.76 | 23.57 | -26.36 | 51.83 | 0.5368 | -726.0 | -532.5 | |
| 0.00 | 1.08 | 0.00 | 0.64 | 18.22 | 22.94 | -26.98 | 53.28 | 0.5398 | -807.0 | -572.2 | |
| 0.00 | 0.81 | 0.00 | 0.48 | 18.64 | 22.61 | -27.31 | 52.94 | 0.5469 | -478.0 | -352.7 | |
| 1.36 | 6.33 | 0.82 | 3.83 | 21.34 | 21.84 | -28.08 | 49.66 | 0.5775 | -856.1 | -570.0 | |
| 0.00 | 1.45 | 0.00 | 0.86 | 18.48 | 22.28 | -27.64 | 53.49 | 0.5496 | -603.0 | -501.4 | |
| 0.00 | 1.54 | 0.00 | 0.93 | 21.08 | 21.78 | -28.14 | 50.08 | 0.5760 | -671.0 | -503.8 | |
| 0.00 | 0.90 | 0.00 | 0.53 | 15.51 | 22.50 | -27.42 | 58.09 | 0.5248 | -823.0 | -638.6 | |
| 0.00 | 1.17 | 0.00 | 0.70 | 19.09 | 21.48 | -28.45 | 53.28 | 0.5637 | -661.0 | -561.9 | |
| 37.50 | 215.89 | 22.18 | 127.63 | 16.53 | 21.20 | -28.73 | 57.52 | 0.5483 | -1104.8 | -427.0 | |
| 0.00 | 0.99 | 0.00 | 0.60 | 19.45 | 20.56 | -29.37 | 53.54 | 0.5771 | -755.0 | -608.9 | |
| 0.00 | 1.27 | 0.00 | 0.76 | 17.11 | 20.26 | -29.66 | 57.36 | 0.5638 | -602.0 | -461.9 | |
| 0.00 | 1.45 | 0.00 | 0.88 | 18.55 | 19.99 | -29.93 | 55.36 | 0.5771 | -512.0 | -457.4 | |
| 0.00 | 1.17 | 0.00 | 0.71 | 17.82 | 19.21 | -30.72 | 57.10 | 0.5813 | -531.0 | -402.3 | |
| 0.00 | 0.81 | 0.00 | 0.50 | 17.63 | 18.83 | -31.09 | 57.68 | 0.5846 | -416.0 | -352.6 | |
| 0.00 | 3.89 | 0.00 | 2.38 | 17.70 | 18.22 | -31.70 | 58.03 | 0.5923 | -869.0 | -681.1 | |
| 0.00 | 1.17 | 0.00 | 0.72 | 17.86 | 17.89 | -32.04 | 58.03 | 0.5974 | -485.0 | -315.2 | |
| 2.35 | 2.53 | 1.47 | 1.58 | 18.57 | 17.13 | -32.79 | 57.52 | 0.6108 | 841.7 | 666.5 | |
| 2.44 | 3.52 | 1.53 | 2.21 | 18.51 | 16.84 | -33.09 | 57.82 | 0.6139 | 783.5 | 576.9 | |
| 0.00 | 1.27 | 0.00 | 0.80 | 18.71 | 15.75 | -34.17 | 58.27 | 0.6278 | -606.0 | -438.7 | |
| 0.00 | 1.36 | 0.00 | 0.87 | 20.14 | 15.25 | -34.68 | 56.59 | 0.6422 | 670.0 | 595.4 | |
| 0.00 | 2.62 | 0.00 | 1.68 | 19.42 | 15.27 | -34.66 | 57.57 | 0.6376 | 893.0 | 680.1 | |
| 0.00 | 1.72 | 0.00 | 1.11 | 19.88 | 15.15 | -34.77 | 57.01 | 0.6416 | 710.0 | 599.9 | |
| 1.72 | 2.08 | 1.11 | 1.34 | 19.52 | 14.89 | -35.04 | 57.68 | 0.6425 | 711.2 | 560.2 | |
| 0.00 | 1.36 | 0.00 | 0.88 | 19.69 | 14.41 | -35.51 | 57.76 | 0.6489 | 755.0 | 587.8 | |
| 0.00 | 0.81 | 0.00 | 0.53 | 19.79 | 14.27 | -35.66 | 57.72 | 0.6511 | 554.0 | 509.7 | |
| 0.00 | 0.99 | 0.00 | 0.65 | 19.56 | 14.04 | -35.88 | 58.17 | 0.6523 | 481.0 | 427.0 | |
| 0.00 | 1.81 | 0.00 | 1.16 | 17.43 | 14.48 | -35.44 | 60.92 | 0.6354 | 732.0 | 603.3 | |
| 0.00 | 0.90 | 0.00 | 0.59 | 19.27 | 14.00 | -35.92 | 58.60 | 0.6511 | 822.0 | 728.5 | |
| 0.00 | 1.17 | 0.00 | 0.76 | 18.82 | 13.95 | -35.97 | 59.26 | 0.6491 | 804.0 | 671.3 | |
| 0.00 | 1.45 | 0.00 | 0.94 | 18.50 | 13.91 | -36.01 | 59.74 | 0.6478 | 756.0 | 711.1 | |
| 0.00 | 1.36 | 0.00 | 0.88 | 18.34 | 13.79 | -36.13 | 60.04 | 0.6483 | 746.0 | 630.5 | |
| 0.00 | 1.36 | 0.00 | 0.88 | 18.66 | 13.67 | -36.25 | 59.66 | 0.6514 | 937.0 | 740.5 | |
| 0.00 | 1.45 | 0.00 | 0.95 | 18.86 | 13.47 | -36.46 | 59.51 | 0.6549 | 760.0 | 594.7 | |
| 0.00 | 5.60 | 0.00 | 3.66 | 18.40 | 13.38 | -36.54 | 60.19 | 0.6534 | 888.0 | 722.2 | |
| 0.99 | 2.71 | 0.65 | 1.78 | 18.76 | 13.21 | -36.71 | 59.79 | 0.6573 | 633.9 | 523.6 | |
| 0.00 | 1.17 | 0.00 | 0.77 | 18.05 | 13.11 | -36.82 | 60.84 | 0.6547 | 640.0 | 521.8 | |
| 0.00 | 1.99 | 0.00 | 1.31 | 18.41 | 12.90 | -37.03 | 60.47 | 0.6590 | 407.0 | 366.0 | |
| 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. | |