SDO HMI 2014-08-02 02:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 27.87 | 104.21 | 16.04 | 59.81 | -18.76 | 238.34 | -17.87 | 144.94 | 0.5065 | 118.9 | 39.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.72 | 0.00 | 0.40 | -16.11 | 244.54 | -11.68 | 152.40 | 0.4215 | 738.0 | 524.9 | |
| 0.00 | 1.45 | 0.00 | 0.81 | -17.93 | 243.04 | -13.17 | 151.58 | 0.4574 | 796.0 | 607.7 | |
| 0.00 | 1.09 | 0.00 | 0.61 | -18.07 | 242.60 | -13.61 | 150.95 | 0.4626 | 635.0 | 526.1 | |
| 0.00 | 1.90 | 0.00 | 1.06 | -17.84 | 242.36 | -13.86 | 150.26 | 0.4615 | 884.0 | 737.0 | |
| 0.81 | 3.17 | 0.45 | 1.76 | -17.45 | 242.06 | -14.15 | 149.29 | 0.4586 | 1021.3 | 807.9 | |
| 0.00 | 0.91 | 0.00 | 0.51 | -18.69 | 241.96 | -14.26 | 150.50 | 0.4757 | 872.0 | 666.4 | |
| 0.00 | 1.72 | 0.00 | 0.97 | -18.46 | 241.75 | -14.47 | 149.89 | 0.4743 | 687.0 | 471.6 | |
| 0.63 | 10.14 | 0.36 | 5.75 | -18.63 | 240.23 | -15.98 | 147.58 | 0.4886 | 929.3 | 762.8 | |
| 0.00 | 3.35 | 0.00 | 1.90 | -18.40 | 240.19 | -16.03 | 147.23 | 0.4860 | 1085.0 | 852.1 | |
| 0.91 | -8.00 | 0.51 | -8.00 | -18.70 | 240.06 | -16.16 | 147.38 | 0.4909 | 894.2 | 999999 | |
| 0.00 | 1.36 | 0.00 | 0.77 | -19.04 | 239.96 | -16.26 | 147.61 | 0.4960 | 688.0 | 533.3 | |
| 0.00 | 1.45 | 0.00 | 0.82 | -18.88 | 239.84 | -16.38 | 147.23 | 0.4949 | 710.0 | 592.5 | |
| 1.09 | 4.80 | 0.62 | 2.73 | -18.68 | 239.76 | -16.46 | 146.88 | 0.4931 | 982.3 | 719.3 | |
| 0.00 | 1.18 | 0.00 | 0.67 | -19.36 | 239.45 | -16.76 | 147.18 | 0.5040 | 648.0 | 545.3 | |
| 1.72 | 23.62 | 0.98 | 13.48 | -18.59 | 239.33 | -16.88 | 146.10 | 0.4955 | 1101.2 | 693.6 | |
| 7.78 | -15.00 | 4.44 | -15.00 | -18.70 | 239.12 | -17.10 | 145.90 | 0.4987 | 839.9 | 999999 | |
| 2.08 | -15.00 | 1.19 | -15.00 | -18.44 | 238.95 | -17.27 | 145.32 | 0.4969 | 1032.3 | 999999 | |
| 2.17 | -15.00 | 1.24 | -15.00 | -18.44 | 238.74 | -17.47 | 145.02 | 0.4988 | 765.8 | 999999 | |
| 0.91 | 2.08 | 0.52 | 1.20 | -19.66 | 238.47 | -17.74 | 146.04 | 0.5158 | -925.6 | -775.4 | |
| 0.00 | 1.00 | 0.00 | 0.57 | -17.90 | 237.89 | -18.32 | 143.07 | 0.4999 | 642.0 | 549.8 | |
| 0.72 | 2.99 | 0.42 | 1.72 | -18.98 | 237.67 | -18.55 | 144.07 | 0.5145 | -974.8 | -614.1 | |
| 2.08 | 18.55 | 1.21 | 10.76 | -19.13 | 237.04 | -19.18 | 143.35 | 0.5219 | -972.7 | -742.3 | |
| 1.72 | -22.00 | 1.00 | -22.00 | -18.88 | 236.73 | -19.49 | 142.60 | 0.5217 | -982.1 | 999999 | |
| 0.00 | 0.81 | 0.00 | 0.47 | -18.62 | 236.55 | -19.66 | 142.03 | 0.5203 | -754.0 | -650.8 | |
| 0.00 | 1.09 | 0.00 | 0.63 | -19.09 | 236.26 | -19.96 | 142.21 | 0.5285 | -834.0 | -650.2 | |
| 0.00 | 1.00 | 0.00 | 0.58 | -18.73 | 236.16 | -20.05 | 141.64 | 0.5252 | -853.0 | -686.5 | |
| 0.00 | 1.45 | 0.00 | 0.85 | -19.34 | 236.05 | -20.16 | 142.23 | 0.5331 | -743.0 | -709.2 | |
| 0.00 | 3.89 | 0.00 | 2.29 | -19.79 | 235.75 | -20.46 | 142.37 | 0.5408 | -934.0 | -784.9 | |
| 0.00 | 0.81 | 0.00 | 0.47 | -17.02 | 235.69 | -20.52 | 138.77 | 0.5107 | -593.0 | -473.0 | |
| 5.25 | 8.33 | 3.10 | 4.92 | -19.84 | 235.26 | -20.95 | 141.78 | 0.5458 | -885.3 | -547.7 | |
| 0.00 | 1.18 | 0.00 | 0.67 | -15.68 | 235.54 | -20.68 | 136.70 | 0.4977 | -611.0 | -541.1 | |
| 0.00 | 1.90 | 0.00 | 1.11 | -18.25 | 234.68 | -21.53 | 139.05 | 0.5339 | -859.0 | -666.0 | |
| 0.00 | 1.18 | 0.00 | 0.69 | -18.65 | 234.59 | -21.62 | 139.45 | 0.5391 | -828.0 | -651.8 | |
| 0.00 | 1.09 | 0.00 | 0.64 | -18.80 | 234.33 | -21.88 | 139.30 | 0.5431 | -644.0 | -481.2 | |
| 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. | |