SDO HMI 2014-10-05 17:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 3.95 | 20.54 | 2.99 | 16.12 | -18.25 | 77.72 | -44.90 | 120.05 | 0.7756 | 358.2 | 322.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.97 | 0.00 | 0.72 | -20.94 | 82.21 | -40.40 | 125.73 | 0.7480 | 552.0 | 453.5 | |
| 0.00 | 1.05 | 0.00 | 0.76 | -15.45 | 80.78 | -41.84 | 118.27 | 0.7323 | 624.0 | 456.9 | |
| 3.95 | 7.55 | 2.99 | 5.72 | -18.23 | 79.62 | -43.00 | 121.01 | 0.7581 | 796.0 | 578.9 | |
| 0.00 | 0.79 | 0.00 | 0.60 | -17.98 | 79.43 | -43.18 | 120.61 | 0.7586 | 561.0 | 496.1 | |
| 0.00 | 0.44 | 0.00 | 0.33 | -16.05 | 79.69 | -42.92 | 118.42 | 0.7465 | 445.0 | 482.8 | |
| 0.00 | 0.79 | 0.00 | 0.66 | -23.65 | 76.74 | -45.87 | 125.59 | 0.8108 | 465.0 | 409.9 | |
| 0.00 | 2.11 | 0.00 | 1.56 | -15.42 | 79.47 | -43.14 | 117.54 | 0.7457 | 548.0 | 512.2 | |
| 0.00 | 1.32 | 0.00 | 1.04 | -16.81 | 76.70 | -45.92 | 117.80 | 0.7796 | 593.0 | 474.0 | |
| 0.00 | 1.05 | 0.00 | 0.86 | -19.03 | 75.84 | -46.77 | 119.97 | 0.7974 | 132.0 | 198.3 | |
| 0.00 | 1.05 | 0.00 | 0.85 | -17.21 | 75.47 | -47.14 | 117.68 | 0.7930 | 461.0 | 379.4 | |
| 0.00 | 1.23 | 0.00 | 1.02 | -17.57 | 74.60 | -48.02 | 117.70 | 0.8026 | 260.0 | 205.9 | |
| 0.00 | 0.26 | 0.00 | 0.25 | -22.82 | 71.14 | -51.47 | 121.98 | 0.8522 | -444.0 | -485.3 | |
| 0.00 | 0.88 | 0.00 | 0.79 | -20.21 | 71.92 | -50.70 | 119.47 | 0.8362 | -477.0 | -382.9 | |
| 0.00 | 1.05 | 0.00 | 0.96 | -20.07 | 71.22 | -51.40 | 119.02 | 0.8416 | -372.0 | -335.3 | |
| 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. | |