SDO HMI 2014-09-22 16:00:34 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 12.73 | 0.00 | 6.93 | -13.61 | 285.45 | -9.27 | 158.29 | 0.4021 | 733.3 | 597.4 | |
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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 | 1.15 | 0.00 | 0.60 | -10.35 | 299.75 | 5.04 | 196.14 | 0.3119 | 725.0 | 690.8 | |
| 0.00 | 1.15 | 0.00 | 0.60 | -9.84 | 299.53 | 4.81 | 195.92 | 0.3028 | 801.0 | 658.2 | |
| 0.00 | 0.97 | 0.00 | 0.51 | -13.05 | 295.56 | 0.85 | 182.40 | 0.3452 | 703.0 | 646.0 | |
| 0.00 | 1.15 | 0.00 | 0.60 | -7.30 | 283.88 | -10.84 | 142.77 | 0.3097 | 632.0 | 432.3 | |
| 0.00 | 1.24 | 0.00 | 0.65 | -8.12 | 283.39 | -11.33 | 143.12 | 0.3254 | 826.0 | 625.4 | |
| 0.00 | 0.88 | 0.00 | 0.49 | -17.40 | 282.17 | -12.55 | 153.23 | 0.4622 | 723.0 | 628.4 | |
| 0.00 | 1.15 | 0.00 | 0.63 | -13.67 | 281.58 | -13.14 | 147.78 | 0.4160 | 717.0 | 600.7 | |
| 0.00 | 1.42 | 0.00 | 0.76 | -10.96 | 281.72 | -13.00 | 144.18 | 0.3788 | 813.0 | 576.6 | |
| 0.00 | 0.88 | 0.00 | 0.53 | -24.13 | 280.12 | -14.60 | 155.89 | 0.5653 | 705.0 | 536.4 | |
| 0.00 | 0.97 | 0.00 | 0.58 | -24.14 | 279.81 | -14.91 | 155.45 | 0.5672 | 703.0 | 566.5 | |
| 0.00 | 1.77 | 0.00 | 0.98 | -13.93 | 278.39 | -16.33 | 142.30 | 0.4481 | 718.0 | 610.2 | |
| 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. | |