SDO HMI 2014-11-10 10:00:27 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 23.02 | 0.00 | 12.74 | -23.26 | 9.31 | -2.35 | 175.24 | 0.4519 | 663.1 | 572.8 | |
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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 | 2.24 | 0.00 | 1.22 | -21.41 | 10.16 | -1.50 | 176.67 | 0.4219 | 894.0 | 707.4 | |
| 0.00 | 0.95 | 0.00 | 0.51 | -20.53 | 10.17 | -1.49 | 176.56 | 0.4079 | 741.0 | 732.6 | |
| 0.00 | 2.93 | 0.00 | 1.61 | -22.53 | 10.09 | -1.58 | 176.67 | 0.4397 | 642.0 | 585.2 | |
| 0.00 | 2.07 | 0.00 | 1.14 | -22.56 | 9.80 | -1.87 | 176.06 | 0.4405 | 754.0 | 588.6 | |
| 0.00 | 2.50 | 0.00 | 1.37 | -21.84 | 9.42 | -2.24 | 175.13 | 0.4295 | 290.0 | 367.2 | |
| 0.00 | 2.07 | 0.00 | 1.15 | -23.66 | 9.26 | -2.40 | 175.17 | 0.4582 | 581.0 | 556.5 | |
| 0.00 | 0.69 | 0.00 | 0.38 | -24.00 | 9.25 | -2.41 | 175.22 | 0.4634 | 614.0 | 525.8 | |
| 0.00 | 1.81 | 0.00 | 1.01 | -24.40 | 9.11 | -2.55 | 175.03 | 0.4698 | 747.0 | 635.1 | |
| 0.00 | 1.98 | 0.00 | 1.11 | -24.73 | 8.98 | -2.69 | 174.83 | 0.4752 | 844.0 | 718.3 | |
| 0.00 | 1.03 | 0.00 | 0.58 | -24.23 | 8.92 | -2.74 | 174.62 | 0.4675 | 799.0 | 633.5 | |
| 0.00 | 1.38 | 0.00 | 0.78 | -25.17 | 8.54 | -3.13 | 174.11 | 0.4825 | 557.0 | 425.9 | |
| 0.00 | 1.38 | 0.00 | 0.77 | -24.00 | 8.37 | -3.29 | 173.50 | 0.4648 | 801.0 | 638.4 | |
| 0.00 | 0.78 | 0.00 | 0.43 | -24.20 | 8.30 | -3.36 | 173.41 | 0.4680 | 530.0 | 438.3 | |
| 0.00 | 1.21 | 0.00 | 0.68 | -24.77 | 8.16 | -3.51 | 173.28 | 0.4770 | 489.0 | 417.9 | |
| 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. | |