SDO HMI 2011-06-01 22:59:10 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 48.16 | 283.11 | 29.05 | 172.43 | 17.21 | 19.93 | -31.10 | 58.26 | 0.5815 | -330.9 | -240.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.99 | 0.00 | 0.59 | 18.59 | 23.55 | -27.48 | 53.15 | 0.5487 | -731.0 | -638.8 | |
| 0.00 | 5.78 | 0.00 | 3.54 | 21.39 | 21.85 | -29.17 | 50.55 | 0.5900 | -739.0 | -708.9 | |
| 0.00 | 0.99 | 0.00 | 0.59 | 18.50 | 22.29 | -28.74 | 54.42 | 0.5628 | -705.0 | -627.2 | |
| 0.00 | 1.63 | 0.00 | 0.99 | 19.12 | 21.32 | -29.70 | 54.31 | 0.5786 | -731.0 | -543.5 | |
| 41.92 | 210.06 | 25.05 | 125.57 | 16.52 | 21.25 | -29.78 | 58.37 | 0.5613 | -1107.9 | -395.7 | |
| 0.00 | 0.63 | 0.00 | 0.40 | 22.16 | 19.97 | -31.06 | 51.09 | 0.6163 | -700.0 | -593.4 | |
| 0.00 | 0.90 | 0.00 | 0.55 | 19.48 | 20.54 | -30.49 | 54.42 | 0.5903 | -661.0 | -583.1 | |
| 0.00 | 1.08 | 0.00 | 0.66 | 18.93 | 20.43 | -30.60 | 55.32 | 0.5877 | -646.0 | -569.1 | |
| 0.00 | 2.80 | 0.00 | 1.71 | 18.29 | 20.04 | -30.99 | 56.59 | 0.5879 | -574.0 | -469.1 | |
| 0.00 | 1.17 | 0.00 | 0.72 | 17.62 | 18.97 | -32.06 | 58.39 | 0.5962 | -547.0 | -437.1 | |
| 0.00 | 1.08 | 0.00 | 0.67 | 17.94 | 18.41 | -32.62 | 58.31 | 0.6049 | -579.0 | -524.8 | |
| 0.00 | 4.34 | 0.00 | 2.70 | 17.75 | 18.22 | -32.81 | 58.72 | 0.6060 | -780.0 | -575.8 | |
| 0.00 | 1.72 | 0.00 | 1.04 | 14.67 | 18.76 | -32.27 | 63.11 | 0.5813 | -648.0 | -402.5 | |
| 4.70 | 7.14 | 2.98 | 4.52 | 18.53 | 16.98 | -34.05 | 58.43 | 0.6254 | 885.5 | 819.4 | |
| 0.00 | 1.26 | 0.00 | 0.87 | 25.07 | 14.43 | -36.60 | 51.38 | 0.6936 | 619.0 | 474.6 | |
| 0.00 | 0.90 | 0.00 | 0.59 | 20.35 | 15.54 | -35.49 | 56.81 | 0.6526 | 733.0 | 553.6 | |
| 0.00 | 0.99 | 0.00 | 0.65 | 20.06 | 15.46 | -35.57 | 57.27 | 0.6518 | 680.0 | 551.5 | |
| 0.00 | 2.53 | 0.00 | 1.63 | 18.67 | 15.73 | -35.30 | 59.04 | 0.6406 | -662.0 | -427.7 | |
| 0.00 | 2.44 | 0.00 | 1.59 | 20.16 | 15.24 | -35.79 | 57.27 | 0.6549 | 708.0 | 573.2 | |
| 0.00 | 1.26 | 0.00 | 0.84 | 21.41 | 14.89 | -36.14 | 55.81 | 0.6661 | 699.0 | 445.6 | |
| 0.00 | 1.90 | 0.00 | 1.21 | 17.67 | 15.73 | -35.30 | 60.47 | 0.6351 | 648.0 | 492.1 | |
| 0.00 | 1.81 | 0.00 | 1.18 | 19.45 | 15.22 | -35.81 | 58.27 | 0.6509 | 874.0 | 761.8 | |
| 0.00 | 1.17 | 0.00 | 0.77 | 19.71 | 15.00 | -36.03 | 58.05 | 0.6550 | 769.0 | 584.7 | |
| 0.00 | 2.53 | 0.00 | 1.66 | 19.55 | 14.84 | -36.19 | 58.37 | 0.6558 | 779.0 | 642.4 | |
| 0.00 | 0.81 | 0.00 | 0.54 | 19.68 | 14.44 | -36.59 | 58.43 | 0.6610 | 634.0 | 563.0 | |
| 0.00 | 1.99 | 0.00 | 1.26 | 15.48 | 15.38 | -35.65 | 63.89 | 0.6278 | -876.0 | -636.6 | |
| 0.00 | 1.36 | 0.00 | 0.91 | 21.64 | 13.72 | -37.31 | 56.23 | 0.6801 | 432.0 | 446.8 | |
| 0.00 | 1.90 | 0.00 | 1.28 | 21.35 | 13.72 | -37.31 | 56.62 | 0.6783 | 179.0 | 213.4 | |
| 0.00 | 1.08 | 0.00 | 0.72 | 19.52 | 14.04 | -36.99 | 58.89 | 0.6646 | 600.0 | 476.8 | |
| 0.00 | 1.72 | 0.00 | 1.13 | 19.20 | 14.08 | -36.95 | 59.31 | 0.6624 | 793.0 | 655.1 | |
| 0.00 | 0.81 | 0.00 | 0.53 | 18.26 | 13.92 | -37.11 | 60.70 | 0.6593 | 719.0 | 536.6 | |
| 0.00 | 2.80 | 0.00 | 1.84 | 18.43 | 13.80 | -37.23 | 60.54 | 0.6615 | 746.0 | 693.1 | |
| 0.00 | 1.08 | 0.00 | 0.72 | 18.59 | 13.76 | -37.27 | 60.34 | 0.6628 | 759.0 | 731.0 | |
| 0.00 | 0.81 | 0.00 | 0.54 | 18.88 | 13.52 | -37.51 | 60.08 | 0.6670 | 524.0 | 419.3 | |
| 0.00 | 7.86 | 0.00 | 5.20 | 18.30 | 13.47 | -37.56 | 60.91 | 0.6646 | 882.0 | 630.3 | |
| 1.54 | 2.80 | 1.02 | 1.86 | 18.72 | 13.28 | -37.75 | 60.43 | 0.6690 | 556.1 | 470.5 | |
| 0.00 | 0.99 | 0.00 | 0.66 | 18.46 | 12.81 | -38.22 | 61.04 | 0.6729 | 484.0 | 324.5 | |
| 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. | |