SDO HMI 2014-11-08 11:00:27 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 2.50 | 23.66 | 1.35 | 13.03 | -14.86 | 19.37 | -18.12 | 136.79 | 0.4364 | -254.2 | -162.8 | |
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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 | 1.47 | 0.00 | 0.77 | -13.61 | 26.54 | -10.94 | 147.96 | 0.3493 | -1.0 | 7.3 | |
| 0.00 | 1.04 | 0.00 | 0.55 | -13.72 | 25.20 | -12.29 | 145.09 | 0.3630 | 669.0 | 545.8 | |
| 0.00 | 1.47 | 0.00 | 0.78 | -13.71 | 23.56 | -13.92 | 141.68 | 0.3787 | 802.0 | 588.4 | |
| 0.00 | 1.64 | 0.00 | 0.88 | -13.45 | 22.03 | -15.45 | 138.33 | 0.3915 | 914.0 | 709.9 | |
| 1.64 | 4.92 | 0.88 | 2.64 | -13.24 | 21.89 | -15.60 | 137.69 | 0.3905 | 840.5 | 716.2 | |
| 0.86 | 3.97 | 0.47 | 2.17 | -14.08 | 19.98 | -17.51 | 135.88 | 0.4210 | -970.6 | -792.4 | |
| 0.00 | 2.76 | 0.00 | 1.57 | -16.27 | 15.87 | -21.62 | 133.51 | 0.4896 | -830.0 | -754.6 | |
| 0.00 | 0.95 | 0.00 | 0.54 | -15.76 | 15.93 | -21.56 | 132.79 | 0.4839 | -696.0 | -552.2 | |
| 0.00 | 0.95 | 0.00 | 0.54 | -16.55 | 15.74 | -21.75 | 133.78 | 0.4939 | -783.0 | -665.2 | |
| 0.00 | 1.04 | 0.00 | 0.60 | -17.87 | 15.07 | -22.42 | 134.89 | 0.5145 | -755.0 | -574.7 | |
| 0.00 | 1.38 | 0.00 | 0.80 | -17.64 | 14.28 | -23.20 | 133.59 | 0.5205 | -671.0 | -486.8 | |
| 0.00 | 1.12 | 0.00 | 0.65 | -17.48 | 13.97 | -23.52 | 132.99 | 0.5225 | -598.0 | -414.2 | |
| 0.00 | 0.95 | 0.00 | 0.54 | -15.46 | 14.06 | -23.43 | 130.01 | 0.5023 | -757.0 | -691.6 | |
| 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. | |