SDO HMI 2014-09-13 02:00:35 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 29.63 | 140.17 | 16.01 | 75.74 | -15.80 | 66.07 | 4.86 | 191.78 | 0.4015 | 745.1 | 460.9 | |
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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 | 0.98 | 0.00 | 0.53 | -15.69 | 67.21 | 5.99 | 194.49 | 0.4035 | 209.0 | 149.6 | |
| 0.36 | 132.42 | 0.19 | 71.53 | -16.05 | 67.03 | 5.81 | 193.85 | 0.4083 | 827.2 | 514.3 | |
| 1.07 | -2.00 | 0.58 | -2.00 | -15.95 | 66.96 | 5.75 | 193.76 | 0.4065 | 919.1 | 999999 | |
| 6.85 | -2.00 | 3.71 | -2.00 | -15.91 | 66.61 | 5.40 | 192.98 | 0.4047 | 1015.3 | 999999 | |
| 5.43 | -2.00 | 2.93 | -2.00 | -15.78 | 66.39 | 5.18 | 192.53 | 0.4018 | 1190.8 | 999999 | |
| 5.07 | -2.00 | 2.74 | -2.00 | -15.74 | 66.17 | 4.95 | 192.03 | 0.4005 | 1182.4 | 999999 | |
| 6.32 | -2.00 | 3.41 | -2.00 | -15.51 | 66.01 | 4.79 | 191.77 | 0.3963 | 1394.9 | 999999 | |
| 0.53 | -2.00 | 0.29 | -2.00 | -15.87 | 65.92 | 4.71 | 191.38 | 0.4017 | 800.7 | 999999 | |
| 4.00 | -2.00 | 2.16 | -2.00 | -15.64 | 65.82 | 4.61 | 191.26 | 0.3977 | 1118.5 | 999999 | |
| 0.00 | 0.89 | 0.00 | 0.48 | -14.90 | 64.02 | 2.81 | 187.16 | 0.3814 | 787.0 | 619.1 | |
| 0.00 | 1.07 | 0.00 | 0.58 | -16.41 | 64.01 | 2.80 | 186.65 | 0.4055 | 706.0 | 579.5 | |
| 0.00 | 1.69 | 0.00 | 0.92 | -16.66 | 62.53 | 1.32 | 183.11 | 0.4075 | -852.0 | -726.8 | |
| 0.00 | 0.89 | 0.00 | 0.48 | -16.70 | 62.18 | 0.97 | 182.29 | 0.4078 | -812.0 | -647.8 | |
| 0.00 | 1.07 | 0.00 | 0.59 | -18.59 | 60.03 | -1.18 | 177.42 | 0.4380 | -875.0 | -683.8 | |
| 0.00 | 1.16 | 0.00 | 0.63 | -16.31 | 57.97 | -3.24 | 172.26 | 0.4047 | -747.0 | -568.9 | |
| 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. | |