SDO HMI 2011-07-05 17:59:11 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 53.84 | 264.49 | 32.02 | 156.47 | 17.06 | 354.34 | 30.56 | 296.85 | 0.5465 | -347.8 | -228.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 28.69 | 199.76 | 17.15 | 119.15 | 16.88 | 355.52 | 31.74 | 295.73 | 0.5610 | -1090.8 | -362.6 | |
| 1.36 | -1.00 | 0.81 | -1.00 | 17.39 | 355.24 | 31.47 | 296.75 | 0.5600 | -591.9 | 999999 | |
| 0.00 | 1.27 | 0.00 | 0.76 | 17.17 | 355.09 | 31.31 | 296.48 | 0.5569 | -655.0 | -601.1 | |
| 0.00 | 1.82 | 0.00 | 1.08 | 17.65 | 355.07 | 31.29 | 297.29 | 0.5591 | -348.0 | -239.2 | |
| 12.35 | -1.00 | 7.31 | -1.00 | 16.84 | 354.65 | 30.88 | 296.18 | 0.5495 | -1116.2 | 999999 | |
| 2.36 | 3.45 | 1.40 | 2.05 | 18.14 | 354.38 | 30.60 | 298.56 | 0.5529 | -438.0 | -26.6 | |
| 0.00 | 1.00 | 0.00 | 0.59 | 17.45 | 354.21 | 30.43 | 297.51 | 0.5469 | -643.0 | -443.5 | |
| 0.00 | 0.73 | 0.00 | 0.43 | 17.67 | 354.03 | 30.25 | 298.01 | 0.5458 | -351.0 | -345.4 | |
| 0.00 | 0.91 | 0.00 | 0.53 | 16.92 | 353.82 | 30.04 | 296.86 | 0.5390 | -532.0 | -311.7 | |
| 4.27 | 7.90 | 2.53 | 4.68 | 18.69 | 354.07 | 30.30 | 299.68 | 0.5522 | 809.0 | 520.2 | |
| 0.00 | 1.54 | 0.00 | 0.93 | 20.52 | 354.46 | 30.69 | 302.40 | 0.5682 | -765.0 | -541.5 | |
| 0.00 | 2.18 | 0.00 | 1.29 | 19.17 | 353.95 | 30.17 | 300.57 | 0.5534 | -848.0 | -680.6 | |
| 1.54 | 2.09 | 0.91 | 1.23 | 18.19 | 353.68 | 29.90 | 299.12 | 0.5443 | -677.8 | -689.0 | |
| 0.00 | 2.72 | 0.00 | 1.59 | 17.03 | 353.43 | 29.66 | 297.30 | 0.5345 | -693.0 | -578.4 | |
| 0.00 | 1.54 | 0.00 | 0.89 | 15.73 | 352.78 | 29.00 | 295.42 | 0.5188 | -871.0 | -668.3 | |
| 0.00 | 1.63 | 0.00 | 0.95 | 16.58 | 352.70 | 28.92 | 297.00 | 0.5223 | -778.0 | -655.4 | |
| 3.27 | 4.27 | 1.91 | 2.49 | 18.22 | 352.76 | 28.99 | 299.82 | 0.5327 | 799.3 | 571.7 | |
| 0.00 | 1.09 | 0.00 | 0.64 | 18.44 | 352.73 | 28.95 | 300.23 | 0.5336 | 642.0 | 522.0 | |
| 0.00 | 0.73 | 0.00 | 0.43 | 19.84 | 352.41 | 28.63 | 302.84 | 0.5386 | -680.0 | -587.1 | |
| 0.00 | 1.91 | 0.00 | 1.11 | 19.06 | 351.97 | 28.19 | 301.88 | 0.5279 | -855.0 | -729.8 | |
| 0.00 | 2.45 | 0.00 | 1.39 | 16.01 | 350.31 | 26.54 | 297.71 | 0.4870 | 625.0 | 498.4 | |
| 0.00 | 2.09 | 0.00 | 1.18 | 15.52 | 350.03 | 26.25 | 296.98 | 0.4802 | 642.0 | 515.3 | |
| 0.00 | 1.09 | 0.00 | 0.61 | 15.03 | 349.75 | 25.98 | 296.24 | 0.4735 | 829.0 | 679.9 | |
| 0.00 | 1.18 | 0.00 | 0.67 | 16.21 | 349.84 | 26.07 | 298.46 | 0.4819 | 714.0 | 588.4 | |
| 0.00 | 2.18 | 0.00 | 1.23 | 16.45 | 349.35 | 25.57 | 299.31 | 0.4767 | 826.0 | 695.7 | |
| 0.00 | 1.45 | 0.00 | 0.81 | 14.83 | 349.10 | 25.32 | 296.35 | 0.4632 | 750.0 | 580.0 | |
| 0.00 | 1.18 | 0.00 | 0.66 | 16.63 | 349.30 | 25.53 | 299.71 | 0.4773 | 724.0 | 647.6 | |
| 0.00 | 3.36 | 0.00 | 1.89 | 17.60 | 348.35 | 24.58 | 302.40 | 0.4714 | 778.0 | 677.0 | |
| 0.00 | 2.36 | 0.00 | 1.32 | 17.42 | 347.80 | 24.02 | 302.60 | 0.4629 | 792.0 | 674.1 | |
| 0.00 | 2.81 | 0.00 | 1.57 | 17.72 | 347.39 | 23.61 | 303.57 | 0.4597 | 861.0 | 634.2 | |
| 0.00 | 1.54 | 0.00 | 0.86 | 17.63 | 347.16 | 23.39 | 303.62 | 0.4562 | 900.0 | 674.1 | |
| 0.00 | 1.27 | 0.00 | 0.70 | 17.35 | 346.71 | 22.93 | 303.56 | 0.4482 | 740.0 | 600.1 | |
| 0.00 | 1.54 | 0.00 | 0.85 | 17.02 | 346.18 | 22.41 | 303.46 | 0.4387 | 861.0 | 703.0 | |
| 0.00 | 1.09 | 0.00 | 0.61 | 19.16 | 346.47 | 22.70 | 307.24 | 0.4597 | 543.0 | 470.2 | |
| 0.00 | 2.36 | 0.00 | 1.30 | 17.09 | 345.95 | 22.17 | 303.85 | 0.4362 | 918.0 | 784.5 | |
| 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. | |