SDO HMI 2014-08-09 11:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 113.64 | 726.14 | 65.41 | 418.60 | 12.40 | 128.38 | -30.33 | 75.82 | 0.5106 | -227.3 | -36.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.08 | 0.00 | 0.60 | 16.34 | 132.96 | -25.76 | 66.13 | 0.4578 | -665.0 | -555.2 | |
| 0.27 | 387.74 | 0.15 | 217.04 | 14.50 | 131.87 | -26.84 | 70.62 | 0.4653 | -1061.7 | -386.0 | |
| 60.44 | -2.00 | 33.82 | -2.00 | 14.09 | 131.64 | -27.07 | 71.60 | 0.4671 | -1202.2 | 999999 | |
| 0.27 | -2.00 | 0.15 | -2.00 | 14.69 | 131.39 | -27.33 | 70.47 | 0.4731 | -736.7 | 999999 | |
| 1.90 | -2.00 | 1.07 | -2.00 | 14.50 | 131.13 | -27.59 | 71.01 | 0.4761 | -662.8 | 999999 | |
| 0.27 | -2.00 | 0.15 | -2.00 | 14.22 | 131.06 | -27.66 | 71.62 | 0.4761 | -703.0 | 999999 | |
| 2.35 | -2.00 | 1.32 | -2.00 | 13.93 | 130.85 | -27.87 | 72.30 | 0.4781 | -618.8 | 999999 | |
| 0.00 | 1.90 | 0.00 | 1.08 | 16.25 | 130.41 | -28.31 | 67.87 | 0.4934 | -795.0 | -533.2 | |
| 0.00 | 1.54 | 0.00 | 0.86 | 13.19 | 130.84 | -27.88 | 73.83 | 0.4759 | -559.0 | -377.5 | |
| 0.00 | 1.63 | 0.00 | 0.92 | 12.58 | 129.70 | -29.01 | 75.49 | 0.4909 | 165.0 | 232.5 | |
| 0.00 | 0.99 | 0.00 | 0.57 | 13.86 | 129.43 | -29.28 | 73.04 | 0.4985 | -642.0 | -470.7 | |
| 0.00 | 0.99 | 0.00 | 0.57 | 13.11 | 129.17 | -29.54 | 74.62 | 0.5000 | -743.0 | -617.5 | |
| 0.00 | 1.08 | 0.00 | 0.62 | 12.94 | 128.98 | -29.74 | 75.01 | 0.5024 | -687.0 | -552.8 | |
| 0.54 | 4.88 | 0.31 | 2.83 | 12.10 | 127.49 | -31.22 | 77.09 | 0.5220 | 980.5 | 767.6 | |
| 0.00 | 1.63 | 0.00 | 0.95 | 11.21 | 127.06 | -31.66 | 78.86 | 0.5267 | -607.0 | -453.7 | |
| 0.00 | 3.70 | 0.00 | 2.17 | 11.73 | 126.44 | -32.27 | 78.02 | 0.5365 | 589.0 | 693.6 | |
| 0.00 | 1.08 | 0.00 | 0.64 | 11.27 | 126.39 | -32.32 | 78.89 | 0.5364 | -476.0 | -289.2 | |
| 0.00 | 1.08 | 0.00 | 0.64 | 11.87 | 126.24 | -32.47 | 77.80 | 0.5396 | 518.0 | 447.5 | |
| 0.00 | 3.16 | 0.00 | 1.85 | 9.91 | 126.22 | -32.49 | 81.45 | 0.5372 | 836.0 | 670.8 | |
| 2.53 | 305.80 | 1.49 | 182.56 | 11.61 | 125.94 | -32.77 | 78.35 | 0.5434 | -523.5 | 349.0 | |
| 0.00 | 1.17 | 0.00 | 0.69 | 11.12 | 125.93 | -32.78 | 79.25 | 0.5429 | 841.0 | 684.1 | |
| 0.45 | -20.00 | 0.27 | -20.00 | 11.36 | 125.83 | -32.89 | 78.83 | 0.5447 | -387.0 | 999999 | |
| 0.00 | 1.36 | 0.00 | 0.80 | 11.93 | 125.60 | -33.11 | 77.84 | 0.5488 | 383.0 | 312.1 | |
| 0.00 | 2.08 | 0.00 | 1.23 | 9.68 | 125.33 | -33.39 | 81.98 | 0.5499 | 611.0 | 520.9 | |
| 0.27 | -20.00 | 0.16 | -20.00 | 10.37 | 125.17 | -33.54 | 80.74 | 0.5528 | 1130.3 | 999999 | |
| 0.00 | 0.63 | 0.00 | 0.38 | 11.37 | 125.01 | -33.71 | 78.96 | 0.5564 | 693.0 | 597.1 | |
| 7.77 | -20.00 | 4.62 | -20.00 | 10.57 | 125.00 | -33.71 | 80.39 | 0.5555 | 1188.0 | 999999 | |
| 0.90 | -20.00 | 0.54 | -20.00 | 9.94 | 125.04 | -33.68 | 81.54 | 0.5543 | 847.6 | 999999 | |
| 2.71 | -20.00 | 1.62 | -20.00 | 10.90 | 124.81 | -33.90 | 79.84 | 0.5586 | 887.3 | 999999 | |
| 1.08 | -20.00 | 0.65 | -20.00 | 10.11 | 124.83 | -33.88 | 81.26 | 0.5574 | 1023.0 | 999999 | |
| 3.34 | -20.00 | 2.00 | -20.00 | 10.68 | 124.65 | -34.06 | 80.26 | 0.5606 | 934.2 | 999999 | |
| 20.24 | -20.00 | 12.11 | -20.00 | 9.93 | 124.44 | -34.27 | 81.61 | 0.5628 | 929.6 | 999999 | |
| 8.31 | -20.00 | 4.98 | -20.00 | 10.60 | 124.32 | -34.39 | 80.45 | 0.5651 | 848.0 | 999999 | |
| 0.00 | 1.54 | 0.00 | 0.94 | 10.83 | 122.74 | -35.98 | 80.23 | 0.5877 | -802.0 | -667.6 | |
| 0.00 | 1.08 | 0.00 | 0.66 | 11.16 | 122.58 | -36.14 | 79.70 | 0.5903 | -645.0 | -548.8 | |
| 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. | |