SDO HMI 2014-08-13 05:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 65.51 | 382.93 | 36.03 | 210.24 | 15.01 | 133.63 | 24.51 | 291.38 | 0.4319 | -837.6 | -375.6 | |
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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 | 0.90 | 0.00 | 0.51 | 17.01 | 135.39 | 26.27 | 294.51 | 0.4670 | 662.0 | 536.9 | |
| 64.07 | 360.41 | 35.29 | 198.42 | 15.16 | 134.01 | 24.89 | 291.51 | 0.4384 | -1436.3 | -432.2 | |
| 0.00 | 1.35 | 0.00 | 0.74 | 15.83 | 132.95 | 23.83 | 293.71 | 0.4263 | -701.0 | -560.9 | |
| 0.00 | 1.89 | 0.00 | 1.03 | 16.50 | 131.76 | 22.64 | 296.16 | 0.4129 | -778.0 | -668.4 | |
| 0.00 | 2.08 | 0.00 | 1.09 | 12.80 | 127.33 | 18.21 | 290.60 | 0.3270 | 777.0 | 585.4 | |
| 0.00 | 1.17 | 0.00 | 0.61 | 12.56 | 127.31 | 18.19 | 289.90 | 0.3255 | 710.0 | 514.8 | |
| 0.00 | 1.26 | 0.00 | 0.66 | 12.54 | 127.05 | 17.93 | 290.07 | 0.3214 | 871.0 | 756.6 | |
| 0.00 | 1.08 | 0.00 | 0.57 | 12.84 | 127.07 | 17.95 | 290.95 | 0.3232 | 705.0 | 588.1 | |
| 0.00 | 1.17 | 0.00 | 0.61 | 12.27 | 126.90 | 17.78 | 289.39 | 0.3177 | 754.0 | 684.2 | |
| 0.00 | 1.44 | 0.00 | 0.75 | 12.13 | 126.43 | 17.31 | 289.38 | 0.3098 | 835.0 | 608.4 | |
| 0.00 | 0.54 | 0.00 | 0.28 | 10.11 | 125.82 | 16.70 | 283.29 | 0.2920 | 709.0 | 501.2 | |
| 0.00 | 0.81 | 0.00 | 0.42 | 9.36 | 125.59 | 16.47 | 280.85 | 0.2861 | 741.0 | 552.3 | |
| 0.00 | 1.08 | 0.00 | 0.56 | 10.02 | 125.63 | 16.51 | 283.13 | 0.2886 | 908.0 | 633.7 | |
| 0.00 | 1.08 | 0.00 | 0.56 | 14.27 | 125.55 | 16.43 | 296.89 | 0.3086 | 748.0 | 508.2 | |
| 0.00 | 1.80 | 0.00 | 0.93 | 10.80 | 125.06 | 15.94 | 286.23 | 0.2822 | 1054.0 | 821.3 | |
| 1.44 | 4.87 | 0.74 | 2.50 | 10.28 | 124.23 | 15.11 | 285.06 | 0.2668 | 1068.5 | 831.7 | |
| 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. | |