SDO HMI 2014-08-01 19:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 14.66 | 90.34 | 8.78 | 53.15 | -18.75 | 238.27 | -21.81 | 139.43 | 0.5415 | 153.9 | 94.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.45 | 0.00 | 0.26 | -17.70 | 242.88 | -17.20 | 144.49 | 0.4869 | 655.0 | 567.4 | |
| 0.00 | 1.00 | 0.00 | 0.57 | -18.28 | 242.62 | -17.46 | 144.79 | 0.4961 | 678.0 | 629.4 | |
| 0.00 | 1.99 | 0.00 | 1.13 | -18.15 | 242.50 | -17.58 | 144.45 | 0.4956 | 847.0 | 738.4 | |
| 0.00 | 1.00 | 0.00 | 0.56 | -16.57 | 242.33 | -17.75 | 142.15 | 0.4783 | 726.0 | 657.9 | |
| 0.00 | 1.27 | 0.00 | 0.72 | -17.83 | 242.13 | -17.95 | 143.49 | 0.4951 | 799.0 | 598.7 | |
| 0.00 | 1.54 | 0.00 | 0.87 | -17.66 | 242.08 | -18.00 | 143.21 | 0.4936 | 900.0 | 632.3 | |
| 0.00 | 1.45 | 0.00 | 0.83 | -18.80 | 241.79 | -18.29 | 144.19 | 0.5098 | 826.0 | 588.1 | |
| 0.00 | 2.53 | 0.00 | 1.44 | -17.74 | 241.84 | -18.24 | 142.94 | 0.4967 | 708.0 | 694.5 | |
| 0.00 | 1.00 | 0.00 | 0.57 | -18.67 | 241.67 | -18.41 | 143.85 | 0.5093 | 674.0 | 594.5 | |
| 0.00 | 1.54 | 0.00 | 0.87 | -15.74 | 241.44 | -18.64 | 139.66 | 0.4772 | 703.0 | 561.4 | |
| 0.00 | 1.00 | 0.00 | 0.56 | -16.10 | 241.40 | -18.68 | 140.11 | 0.4817 | 699.0 | 557.6 | |
| 1.00 | 5.34 | 0.58 | 3.09 | -18.26 | 240.19 | -19.89 | 141.22 | 0.5179 | 983.7 | 796.2 | |
| 0.81 | 6.33 | 0.47 | 3.67 | -18.50 | 239.95 | -20.13 | 141.20 | 0.5228 | 1015.8 | 753.8 | |
| 0.00 | 3.17 | 0.00 | 1.84 | -18.57 | 239.77 | -20.31 | 141.05 | 0.5253 | 847.0 | 638.4 | |
| 1.18 | 4.25 | 0.69 | 2.48 | -18.65 | 239.42 | -20.66 | 140.67 | 0.5295 | 744.8 | 567.6 | |
| 0.90 | 7.87 | 0.53 | 4.60 | -18.53 | 239.16 | -20.92 | 140.17 | 0.5306 | 947.3 | 366.1 | |
| 0.54 | -16.00 | 0.32 | -16.00 | -18.50 | 239.03 | -21.05 | 139.95 | 0.5316 | 910.0 | 999999 | |
| 0.00 | 2.44 | 0.00 | 1.43 | -18.30 | 238.92 | -21.17 | 139.56 | 0.5305 | 868.0 | 667.6 | |
| 0.00 | 1.09 | 0.00 | 0.63 | -18.47 | 238.86 | -21.22 | 139.70 | 0.5329 | 707.0 | 549.7 | |
| 0.00 | 1.36 | 0.00 | 0.79 | -18.45 | 238.69 | -21.39 | 139.44 | 0.5342 | 393.0 | 371.9 | |
| 0.00 | 1.00 | 0.00 | 0.58 | -18.59 | 238.50 | -21.58 | 139.37 | 0.5375 | 526.0 | 401.2 | |
| 0.00 | 1.90 | 0.00 | 1.11 | -18.35 | 238.46 | -21.62 | 139.03 | 0.5354 | 634.0 | 577.5 | |
| 0.00 | 1.18 | 0.00 | 0.70 | -18.95 | 237.82 | -22.26 | 138.97 | 0.5478 | -270.0 | -257.2 | |
| 0.00 | 0.81 | 0.00 | 0.48 | -18.63 | 237.42 | -22.66 | 138.06 | 0.5484 | -579.0 | -413.4 | |
| 0.00 | 2.35 | 0.00 | 1.40 | -19.10 | 237.28 | -22.80 | 138.49 | 0.5547 | -699.0 | -515.5 | |
| 0.00 | 1.18 | 0.00 | 0.70 | -18.64 | 237.21 | -22.87 | 137.81 | 0.5506 | -280.0 | -366.5 | |
| 1.00 | 2.62 | 0.59 | 1.56 | -18.99 | 236.84 | -23.24 | 137.82 | 0.5577 | -933.6 | -781.7 | |
| 1.63 | 9.50 | 0.98 | 5.70 | -19.45 | 236.17 | -23.91 | 137.61 | 0.5690 | -910.1 | -750.5 | |
| 0.00 | 3.53 | 0.00 | 2.11 | -18.68 | 236.26 | -23.82 | 136.72 | 0.5603 | -861.0 | -750.1 | |
| 0.00 | 1.00 | 0.00 | 0.60 | -19.65 | 236.10 | -23.98 | 137.78 | 0.5717 | -646.0 | -645.3 | |
| 0.00 | 3.08 | 0.00 | 1.86 | -19.79 | 236.05 | -24.03 | 137.89 | 0.5736 | -689.0 | -611.2 | |
| 1.45 | 4.16 | 0.88 | 2.52 | -19.87 | 235.78 | -24.30 | 137.68 | 0.5769 | -765.1 | -602.0 | |
| 6.15 | 8.69 | 3.74 | 5.28 | -19.86 | 235.32 | -24.76 | 137.14 | 0.5812 | -853.4 | -546.6 | |
| 0.00 | 1.54 | 0.00 | 0.93 | -18.38 | 234.64 | -25.44 | 134.50 | 0.5736 | -773.0 | -660.3 | |
| 0.00 | 1.18 | 0.00 | 0.71 | -18.55 | 234.54 | -25.54 | 134.61 | 0.5763 | -707.0 | -568.1 | |
| 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. | |