SDO HMI 2014-09-18 03:00:35 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 11.10 | 42.24 | 8.77 | 33.02 | -20.93 | 311.66 | -42.99 | 124.66 | 0.7759 | 7.2 | -30.1 | |
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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 |
| 1.07 | 2.31 | 0.79 | 1.70 | -20.77 | 315.13 | -39.53 | 126.60 | 0.7435 | 776.5 | 627.5 | |
| 0.00 | 1.95 | 0.00 | 1.45 | -20.92 | 314.62 | -40.03 | 126.43 | 0.7491 | 702.0 | 526.7 | |
| 1.33 | 2.84 | 0.99 | 2.11 | -20.66 | 314.49 | -40.16 | 126.05 | 0.7487 | 738.6 | 588.4 | |
| 1.07 | 5.59 | 0.80 | 4.19 | -20.62 | 314.12 | -40.53 | 125.77 | 0.7519 | 665.8 | 472.9 | |
| 0.00 | 1.86 | 0.00 | 1.42 | -20.19 | 312.89 | -41.76 | 124.51 | 0.7609 | 549.0 | 493.3 | |
| 0.00 | 2.22 | 0.00 | 1.70 | -20.31 | 312.63 | -42.02 | 124.50 | 0.7640 | 635.0 | 483.2 | |
| 0.00 | 1.24 | 0.00 | 0.96 | -20.32 | 312.15 | -42.50 | 124.22 | 0.7684 | 547.0 | 393.6 | |
| 0.00 | 1.51 | 0.00 | 1.17 | -20.62 | 311.87 | -42.78 | 124.39 | 0.7726 | -287.0 | -183.1 | |
| 0.00 | 0.44 | 0.00 | 0.34 | -20.03 | 311.64 | -43.02 | 123.58 | 0.7716 | 368.0 | 322.8 | |
| 0.00 | 1.07 | 0.00 | 0.85 | -21.60 | 310.75 | -43.90 | 124.84 | 0.7878 | -631.0 | -519.8 | |
| 4.08 | 15.71 | 3.32 | 12.73 | -21.51 | 309.83 | -44.82 | 124.23 | 0.7954 | -585.2 | -488.0 | |
| 0.71 | 5.50 | 0.57 | 4.40 | -20.78 | 310.12 | -44.54 | 123.56 | 0.7892 | -712.1 | -579.3 | |
| 2.84 | -11.00 | 2.30 | -11.00 | -21.20 | 309.91 | -44.74 | 123.92 | 0.7932 | -564.4 | 999999 | |
| 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. | |