SDO HMI 2014-10-11 05:00:31 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 67.39 | 432.88 | 44.34 | 285.15 | -20.55 | 18.19 | -31.85 | 131.30 | 0.6601 | 1026.8 | 297.5 | |
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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 | 2.10 | 0.00 | 1.36 | -21.30 | 20.59 | -29.45 | 134.38 | 0.6431 | -717.0 | -488.1 | |
| 0.00 | 1.31 | 0.00 | 0.83 | -18.82 | 20.38 | -29.66 | 131.12 | 0.6241 | 779.0 | 696.0 | |
| 0.00 | 1.84 | 0.00 | 1.17 | -19.34 | 19.98 | -30.06 | 131.41 | 0.6324 | 712.0 | 599.5 | |
| 0.44 | 3.33 | 0.28 | 2.11 | -18.55 | 19.92 | -30.12 | 130.36 | 0.6265 | 769.0 | 726.1 | |
| 1.31 | 412.91 | 0.85 | 272.12 | -20.37 | 19.31 | -30.72 | 132.08 | 0.6476 | 938.1 | 297.0 | |
| 0.00 | 0.88 | 0.00 | 0.57 | -20.03 | 19.39 | -30.65 | 131.74 | 0.6441 | 925.0 | 805.3 | |
| 0.00 | 0.96 | 0.00 | 0.65 | -22.84 | 18.53 | -31.51 | 134.31 | 0.6754 | -570.0 | -471.6 | |
| 0.00 | 2.02 | 0.00 | 1.27 | -17.39 | 19.67 | -30.37 | 128.62 | 0.6198 | 742.0 | 580.1 | |
| 1.93 | -5.00 | 1.25 | -5.00 | -20.32 | 18.99 | -31.05 | 131.74 | 0.6504 | 1193.0 | 999999 | |
| 0.00 | 1.66 | 0.00 | 1.06 | -18.46 | 19.20 | -30.83 | 129.60 | 0.6332 | 676.0 | 483.1 | |
| 0.00 | 1.84 | 0.00 | 1.23 | -22.04 | 18.35 | -31.68 | 133.23 | 0.6705 | -75.0 | -82.2 | |
| 0.00 | 1.40 | 0.00 | 0.88 | -16.83 | 19.26 | -30.78 | 127.51 | 0.6197 | 619.0 | 393.1 | |
| 63.71 | -5.00 | 41.96 | -5.00 | -20.58 | 18.11 | -31.93 | 131.27 | 0.6611 | 1216.6 | 999999 | |
| 0.00 | 1.58 | 0.00 | 1.11 | -24.15 | 15.70 | -34.33 | 133.45 | 0.7112 | 521.0 | 364.3 | |
| 0.00 | 1.05 | 0.00 | 0.79 | -25.42 | 11.74 | -38.30 | 131.92 | 0.7547 | -82.0 | -117.3 | |
| 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. | |