SDO HMI 2014-07-08 23:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 17.26 | 0.00 | 9.95 | -22.23 | 199.69 | -15.71 | 150.51 | 0.5107 | 160.3 | 45.6 | |
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See sunspots with tool (Click here to study sunspot positions and configurations with tool using white-light and magnetogram images and polarity drawing) (It is recommended to set high resolution on your display!) |
| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.27 | 0.00 | 0.70 | -20.97 | 206.56 | -8.84 | 161.00 | 0.4425 | 786.0 | 515.8 | |
| 0.00 | 1.09 | 0.00 | 0.61 | -21.73 | 204.81 | -10.58 | 158.29 | 0.4630 | 755.0 | 541.5 | |
| 0.00 | 1.27 | 0.00 | 0.71 | -21.65 | 203.18 | -12.22 | 155.26 | 0.4718 | 1059.0 | 888.5 | |
| 0.00 | 1.18 | 0.00 | 0.67 | -22.23 | 202.96 | -12.44 | 155.42 | 0.4812 | 558.0 | 478.8 | |
| 0.00 | 1.09 | 0.00 | 0.60 | -19.94 | 203.12 | -12.27 | 153.43 | 0.4486 | 690.0 | 464.5 | |
| 0.00 | 1.82 | 0.00 | 1.02 | -21.69 | 202.91 | -12.49 | 154.82 | 0.4741 | 823.0 | 670.5 | |
| 0.00 | 2.91 | 0.00 | 1.74 | -27.09 | 200.22 | -15.17 | 155.44 | 0.5627 | -738.0 | -635.2 | |
| 0.00 | 1.27 | 0.00 | 0.76 | -26.46 | 199.57 | -15.83 | 153.98 | 0.5588 | -885.0 | -659.5 | |
| 0.00 | 1.00 | 0.00 | 0.58 | -22.59 | 199.24 | -16.15 | 149.76 | 0.5120 | 902.0 | 656.8 | |
| 0.00 | 0.36 | 0.00 | 0.21 | -22.90 | 199.10 | -16.29 | 149.88 | 0.5170 | 649.0 | 563.2 | |
| 0.00 | 0.36 | 0.00 | 0.21 | -22.60 | 199.04 | -16.36 | 149.45 | 0.5136 | 544.0 | 664.2 | |
| 0.00 | 0.91 | 0.00 | 0.52 | -19.18 | 196.99 | -18.41 | 142.29 | 0.4895 | -715.0 | -582.6 | |
| 0.00 | 1.09 | 0.00 | 0.63 | -20.45 | 195.28 | -20.11 | 141.52 | 0.5199 | -682.0 | -545.7 | |
| 0.00 | 0.82 | 0.00 | 0.49 | -16.36 | 186.24 | -29.15 | 125.63 | 0.5773 | -696.0 | -555.1 | |
| 0.00 | 0.82 | 0.00 | 0.50 | -16.24 | 184.72 | -30.68 | 124.16 | 0.5941 | -645.0 | -532.3 | |
| 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. | |