SDO HMI 2014-11-24 19:00:26 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 8.04 | 33.81 | 4.39 | 18.46 | 4.51 | 157.41 | -24.76 | 82.93 | 0.4224 | 6.4 | 152.2 | |
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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 |
| 3.25 | 4.71 | 1.75 | 2.53 | 4.02 | 159.68 | -22.48 | 83.61 | 0.3855 | -1068.8 | -810.2 | |
| 0.00 | 2.48 | 0.00 | 1.34 | 4.38 | 159.32 | -22.85 | 82.79 | 0.3919 | -1021.0 | -811.7 | |
| 0.00 | 0.94 | 0.00 | 0.51 | 3.96 | 159.20 | -22.96 | 83.88 | 0.3931 | -876.0 | -688.6 | |
| 0.00 | 1.54 | 0.00 | 0.83 | 3.78 | 159.14 | -23.02 | 84.35 | 0.3939 | -841.0 | -534.2 | |
| 0.00 | 1.37 | 0.00 | 0.74 | 4.14 | 158.97 | -23.19 | 83.49 | 0.3971 | -835.0 | -694.7 | |
| 0.00 | 2.14 | 0.00 | 1.16 | 5.02 | 158.20 | -23.97 | 81.52 | 0.4109 | -645.0 | -572.4 | |
| 0.00 | 2.14 | 0.00 | 1.17 | 5.18 | 157.08 | -25.09 | 81.45 | 0.4288 | 128.0 | 112.2 | |
| 0.00 | 1.28 | 0.00 | 0.70 | 5.00 | 156.79 | -25.38 | 81.95 | 0.4330 | 806.0 | 654.4 | |
| 1.37 | 6.42 | 0.75 | 3.53 | 5.53 | 156.67 | -25.50 | 80.77 | 0.4359 | 901.8 | 805.1 | |
| 0.00 | 2.31 | 0.00 | 1.27 | 3.84 | 156.20 | -25.96 | 84.74 | 0.4405 | 1039.0 | 833.2 | |
| 0.00 | 1.80 | 0.00 | 0.99 | 4.28 | 155.83 | -26.34 | 83.81 | 0.4469 | 928.0 | 802.0 | |
| 3.42 | 5.82 | 1.89 | 3.22 | 4.07 | 155.77 | -26.40 | 84.29 | 0.4476 | 1022.8 | 686.4 | |
| 0.00 | 0.86 | 0.00 | 0.47 | 4.13 | 155.50 | -26.67 | 84.21 | 0.4518 | 670.0 | 489.3 | |
| 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. | |