SDO HMI 2014-11-29 11:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 20.44 | 0.00 | 12.47 | -23.10 | 93.73 | -26.94 | 134.51 | 0.5863 | -180.4 | -23.8 | |
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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 | 1.45 | 0.00 | 0.84 | -24.10 | 101.22 | -19.45 | 144.41 | 0.5244 | 696.0 | 539.0 | |
| 0.00 | 1.28 | 0.00 | 0.76 | -22.25 | 96.86 | -23.81 | 136.57 | 0.5457 | 753.0 | 596.3 | |
| 0.00 | 0.60 | 0.00 | 0.35 | -21.54 | 96.57 | -24.10 | 135.26 | 0.5418 | -487.0 | -403.6 | |
| 0.00 | 4.79 | 0.00 | 2.91 | -23.69 | 94.84 | -25.83 | 136.29 | 0.5797 | 792.0 | 703.2 | |
| 0.00 | 1.03 | 0.00 | 0.61 | -22.23 | 94.96 | -25.71 | 134.47 | 0.5649 | -637.0 | -457.1 | |
| 0.00 | 1.28 | 0.00 | 0.79 | -24.06 | 93.56 | -27.11 | 135.48 | 0.5957 | -763.0 | -578.1 | |
| 0.00 | 1.62 | 0.00 | 1.01 | -24.23 | 92.79 | -27.88 | 134.95 | 0.6049 | -752.0 | -600.8 | |
| 0.00 | 0.86 | 0.00 | 0.53 | -24.16 | 92.51 | -28.16 | 134.60 | 0.6071 | -529.0 | -419.0 | |
| 0.00 | 2.57 | 0.00 | 1.60 | -23.78 | 91.94 | -28.73 | 133.57 | 0.6094 | -804.0 | -557.3 | |
| 0.00 | 1.03 | 0.00 | 0.64 | -23.39 | 91.26 | -29.41 | 132.45 | 0.6131 | -466.0 | -388.5 | |
| 0.00 | 1.62 | 0.00 | 0.99 | -19.90 | 91.35 | -29.32 | 127.71 | 0.5842 | -519.0 | -468.4 | |
| 0.00 | 0.94 | 0.00 | 0.60 | -24.75 | 89.97 | -30.70 | 133.07 | 0.6371 | -584.0 | -499.3 | |
| 0.00 | 0.94 | 0.00 | 0.58 | -20.35 | 90.27 | -30.40 | 127.44 | 0.5997 | 733.0 | 590.2 | |
| 0.00 | 0.43 | 0.00 | 0.26 | -19.94 | 90.29 | -30.38 | 126.86 | 0.5965 | 42.0 | 90.2 | |
| 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. | |