SDO HMI 2014-07-08 18:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 53.02 | 253.47 | 36.91 | 174.82 | 14.67 | 261.35 | 43.18 | 287.45 | 0.6956 | -492.6 | -240.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.45 | 0.00 | 1.09 | 13.61 | 266.69 | 48.52 | 284.89 | 0.7557 | -422.0 | -448.2 | |
| 0.00 | 2.45 | 0.00 | 1.75 | 13.34 | 263.71 | 45.54 | 285.05 | 0.7214 | -480.0 | -427.3 | |
| 4.09 | 9.44 | 2.90 | 6.70 | 12.98 | 263.44 | 45.28 | 284.60 | 0.7177 | -836.7 | -668.2 | |
| 1.72 | -3.00 | 1.22 | -3.00 | 13.17 | 263.44 | 45.27 | 284.86 | 0.7180 | -804.7 | 999999 | |
| 0.00 | 2.00 | 0.00 | 1.44 | 15.67 | 264.02 | 45.85 | 288.16 | 0.7294 | 531.0 | 392.3 | |
| 0.00 | 1.82 | 0.00 | 1.27 | 11.82 | 262.97 | 44.80 | 283.07 | 0.7103 | -723.0 | -683.8 | |
| 0.00 | 1.00 | 0.00 | 0.70 | 11.64 | 262.93 | 44.76 | 282.82 | 0.7095 | -637.0 | -545.8 | |
| 0.00 | 1.00 | 0.00 | 0.71 | 15.66 | 262.93 | 44.76 | 288.40 | 0.7168 | -455.0 | -424.0 | |
| 0.00 | 1.63 | 0.00 | 1.16 | 16.85 | 262.83 | 44.66 | 290.07 | 0.7185 | 550.0 | 383.8 | |
| 0.00 | 0.27 | 0.00 | 0.19 | 12.32 | 261.63 | 43.46 | 284.00 | 0.6949 | 480.0 | 450.0 | |
| 22.70 | 204.18 | 15.79 | 142.03 | 14.66 | 262.04 | 43.87 | 287.23 | 0.7043 | -981.0 | -292.1 | |
| 21.06 | -11.00 | 14.63 | -11.00 | 15.14 | 261.86 | 43.69 | 287.95 | 0.7032 | -1030.9 | 999999 | |
| 0.00 | 1.27 | 0.00 | 0.87 | 12.96 | 261.08 | 42.91 | 285.03 | 0.6893 | -739.0 | -490.4 | |
| 3.45 | -11.00 | 2.37 | -11.00 | 14.92 | 261.11 | 42.94 | 287.83 | 0.6937 | -841.4 | 999999 | |
| 0.00 | 1.09 | 0.00 | 0.74 | 13.42 | 260.62 | 42.45 | 285.79 | 0.6846 | -661.0 | -570.7 | |
| 0.00 | 1.63 | 0.00 | 1.11 | 14.81 | 260.69 | 42.52 | 287.79 | 0.6885 | -678.0 | -642.7 | |
| 0.00 | 1.27 | 0.00 | 0.86 | 14.85 | 260.53 | 42.36 | 287.88 | 0.6866 | -592.0 | -620.9 | |
| 0.00 | 1.27 | 0.00 | 0.86 | 13.65 | 260.17 | 42.00 | 286.24 | 0.6795 | -760.0 | -613.6 | |
| 0.00 | 1.82 | 0.00 | 1.23 | 14.86 | 260.32 | 42.15 | 287.95 | 0.6841 | -649.0 | -623.7 | |
| 0.00 | 1.27 | 0.00 | 0.85 | 14.58 | 259.53 | 41.36 | 287.76 | 0.6738 | -687.0 | -589.4 | |
| 0.00 | 0.27 | 0.00 | 0.18 | 14.68 | 258.76 | 40.59 | 288.11 | 0.6645 | -619.0 | -649.3 | |
| 0.00 | 0.73 | 0.00 | 0.48 | 16.68 | 258.08 | 39.91 | 291.29 | 0.6618 | 569.0 | 468.9 | |
| 0.00 | 1.18 | 0.00 | 0.71 | 10.27 | 252.74 | 34.57 | 282.73 | 0.5746 | 732.0 | 598.2 | |
| 0.00 | 1.36 | 0.00 | 0.83 | 14.10 | 252.94 | 34.77 | 289.15 | 0.5877 | 577.0 | 399.0 | |
| 0.00 | 1.27 | 0.00 | 0.78 | 14.35 | 252.76 | 34.59 | 289.65 | 0.5861 | 733.0 | 557.8 | |
| 0.00 | 1.36 | 0.00 | 0.83 | 14.20 | 252.73 | 34.56 | 289.40 | 0.5852 | 754.0 | 679.1 | |
| 0.00 | 2.27 | 0.00 | 1.38 | 14.57 | 252.68 | 34.51 | 290.05 | 0.5859 | 673.0 | 619.2 | |
| 0.00 | 1.63 | 0.00 | 0.98 | 10.49 | 251.79 | 33.62 | 283.36 | 0.5618 | 663.0 | 578.8 | |
| 0.00 | 1.72 | 0.00 | 1.03 | 10.80 | 251.80 | 33.63 | 283.90 | 0.5625 | 789.0 | 475.5 | |
| 0.00 | 0.91 | 0.00 | 0.54 | 12.78 | 251.44 | 33.27 | 287.50 | 0.5631 | 638.0 | 546.6 | |
| 0.00 | 2.81 | 0.00 | 1.68 | 12.40 | 251.08 | 32.91 | 286.95 | 0.5569 | 785.0 | 506.3 | |
| 0.00 | 0.64 | 0.00 | 0.39 | 18.56 | 251.84 | 33.67 | 296.94 | 0.5917 | 606.0 | 553.0 | |
| 0.00 | 0.82 | 0.00 | 0.49 | 15.01 | 250.83 | 32.66 | 291.61 | 0.5627 | 656.0 | 569.8 | |
| 0.00 | 0.91 | 0.00 | 0.54 | 15.51 | 249.90 | 31.73 | 292.94 | 0.5524 | 727.0 | 593.9 | |
| 0.00 | 0.73 | 0.00 | 0.42 | 18.84 | 244.99 | 26.82 | 302.14 | 0.5063 | 654.0 | 613.2 | |
| 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. | |