SDO HMI 2014-09-07 06:00:36 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 69.03 | 267.63 | 45.11 | 174.88 | -19.74 | 107.22 | -31.03 | 132.01 | 0.6553 | 639.6 | 395.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.77 | 0.00 | 1.77 | -20.50 | 109.84 | -28.41 | 135.36 | 0.6366 | 838.0 | 683.4 | |
| 0.00 | 0.80 | 0.00 | 0.53 | -22.84 | 108.61 | -29.65 | 136.85 | 0.6688 | 484.0 | 522.1 | |
| 0.00 | 0.54 | 0.00 | 0.36 | -23.13 | 108.50 | -29.75 | 137.06 | 0.6722 | 296.0 | 299.7 | |
| 5.18 | 8.93 | 3.45 | 5.95 | -22.82 | 108.38 | -29.87 | 136.62 | 0.6706 | 835.2 | 725.3 | |
| 0.00 | 0.98 | 0.00 | 0.66 | -23.19 | 108.14 | -30.11 | 136.79 | 0.6759 | 523.0 | 470.9 | |
| 0.00 | 0.80 | 0.00 | 0.54 | -23.76 | 107.92 | -30.33 | 137.21 | 0.6828 | 482.0 | 350.0 | |
| 0.00 | 1.25 | 0.00 | 0.84 | -23.49 | 107.84 | -30.42 | 136.84 | 0.6811 | 649.0 | 473.1 | |
| 0.54 | 1.70 | 0.36 | 1.14 | -22.92 | 107.94 | -30.31 | 136.32 | 0.6753 | 594.3 | 513.8 | |
| 9.02 | 89.56 | 5.77 | 57.24 | -18.76 | 108.49 | -29.76 | 131.98 | 0.6344 | 1223.4 | 534.6 | |
| 6.16 | -9.00 | 3.95 | -9.00 | -19.00 | 108.37 | -29.88 | 132.16 | 0.6377 | 860.7 | 999999 | |
| 0.00 | 1.07 | 0.00 | 0.72 | -22.64 | 107.44 | -30.81 | 135.55 | 0.6774 | 250.0 | 338.8 | |
| 6.34 | -9.00 | 4.06 | -9.00 | -18.71 | 108.21 | -30.04 | 131.65 | 0.6369 | 932.5 | 999999 | |
| 0.00 | 1.34 | 0.00 | 0.90 | -22.39 | 107.04 | -31.21 | 134.92 | 0.6789 | 486.0 | 490.9 | |
| 0.00 | 0.89 | 0.00 | 0.58 | -19.80 | 107.54 | -30.71 | 132.35 | 0.6526 | 777.0 | 624.4 | |
| 0.00 | 1.96 | 0.00 | 1.32 | -22.20 | 106.82 | -31.43 | 134.51 | 0.6793 | 714.0 | 628.3 | |
| 12.23 | 50.27 | 8.07 | 33.13 | -20.51 | 107.08 | -31.17 | 132.78 | 0.6629 | 817.8 | 334.1 | |
| 0.00 | 1.25 | 0.00 | 0.83 | -20.54 | 106.66 | -31.60 | 132.44 | 0.6672 | 313.0 | 393.7 | |
| 26.43 | 74.65 | 17.39 | 49.06 | -19.79 | 106.71 | -31.54 | 131.60 | 0.6605 | 1032.4 | 471.7 | |
| 0.00 | 1.79 | 0.00 | 1.19 | -20.26 | 106.30 | -31.95 | 131.80 | 0.6683 | -191.0 | -170.0 | |
| 0.00 | 1.34 | 0.00 | 0.90 | -21.40 | 105.99 | -32.26 | 132.87 | 0.6804 | 666.0 | 448.3 | |
| 0.00 | 1.43 | 0.00 | 0.93 | -18.63 | 106.51 | -31.74 | 130.02 | 0.6532 | 711.0 | 637.9 | |
| 0.00 | 0.63 | 0.00 | 0.41 | -19.63 | 106.07 | -32.18 | 130.85 | 0.6656 | 331.0 | 279.1 | |
| 3.13 | 7.23 | 2.06 | 4.78 | -19.30 | 106.03 | -32.22 | 130.42 | 0.6633 | 671.4 | 79.9 | |
| 0.00 | 1.07 | 0.00 | 0.73 | -21.09 | 104.63 | -33.62 | 131.38 | 0.6907 | 613.0 | 542.4 | |
| 0.00 | 1.70 | 0.00 | 1.15 | -20.39 | 104.50 | -33.75 | 130.45 | 0.6866 | 345.0 | 344.7 | |
| 0.00 | 1.88 | 0.00 | 1.26 | -19.41 | 104.43 | -33.82 | 129.23 | 0.6800 | -248.0 | -261.7 | |
| 0.00 | 1.52 | 0.00 | 1.03 | -18.48 | 103.49 | -34.76 | 127.35 | 0.6826 | -558.0 | -478.9 | |
| 0.00 | 1.43 | 0.00 | 0.95 | -16.81 | 103.71 | -34.54 | 125.44 | 0.6686 | -639.0 | -518.4 | |
| 0.00 | 0.27 | 0.00 | 0.18 | -16.62 | 103.59 | -34.66 | 125.11 | 0.6684 | -640.0 | -594.7 | |
| 0.00 | 1.52 | 0.00 | 1.02 | -17.30 | 103.21 | -35.04 | 125.69 | 0.6772 | -517.0 | -443.0 | |
| 0.00 | 1.52 | 0.00 | 1.04 | -19.06 | 102.80 | -35.45 | 127.54 | 0.6936 | -423.0 | -328.7 | |
| 0.00 | 2.77 | 0.00 | 1.85 | -16.61 | 103.29 | -34.96 | 124.87 | 0.6716 | -609.0 | -471.3 | |
| 0.00 | 0.54 | 0.00 | 0.36 | -16.82 | 103.13 | -35.12 | 125.01 | 0.6747 | -296.0 | -199.8 | |
| 0.00 | 1.25 | 0.00 | 0.86 | -18.59 | 102.41 | -35.85 | 126.67 | 0.6943 | -737.0 | -554.9 | |
| 0.00 | 0.98 | 0.00 | 0.67 | -17.78 | 102.13 | -36.12 | 125.48 | 0.6916 | -725.0 | -666.5 | |
| 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. | |