SDO HMI 2014-10-05 10:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 18.64 | 0.00 | 11.53 | -20.68 | 102.27 | -24.20 | 139.95 | 0.5928 | 51.2 | 18.4 | |
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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 | 0.97 | 0.00 | 0.57 | -22.96 | 112.37 | -14.09 | 155.35 | 0.5396 | 497.0 | 453.9 | |
| 0.00 | 1.41 | 0.00 | 0.78 | -15.28 | 111.14 | -15.32 | 145.22 | 0.4487 | 812.0 | 619.1 | |
| 0.00 | 0.53 | 0.00 | 0.30 | -20.09 | 110.54 | -15.92 | 149.84 | 0.5149 | 532.0 | 410.0 | |
| 0.00 | 2.99 | 0.00 | 1.82 | -24.33 | 108.65 | -17.81 | 151.22 | 0.5811 | 601.0 | 498.6 | |
| 0.00 | 1.23 | 0.00 | 0.71 | -17.31 | 105.95 | -20.51 | 139.87 | 0.5211 | 816.0 | 660.9 | |
| 0.00 | 1.14 | 0.00 | 0.65 | -14.95 | 105.91 | -20.55 | 136.59 | 0.4955 | 826.0 | 711.8 | |
| 0.00 | 1.93 | 0.00 | 1.12 | -17.39 | 105.64 | -20.82 | 139.54 | 0.5249 | 522.0 | 462.7 | |
| 0.00 | 1.58 | 0.00 | 1.16 | -30.50 | 95.32 | -31.14 | 142.83 | 0.7398 | -610.0 | -443.7 | |
| 0.00 | 1.14 | 0.00 | 0.71 | -17.61 | 98.38 | -28.09 | 131.41 | 0.6005 | -608.0 | -518.6 | |
| 0.00 | 0.79 | 0.00 | 0.49 | -17.18 | 98.41 | -28.05 | 130.88 | 0.5964 | -816.0 | -627.9 | |
| 0.00 | 1.58 | 0.00 | 0.99 | -18.26 | 97.33 | -29.14 | 131.22 | 0.6170 | -614.0 | -545.3 | |
| 0.00 | 0.62 | 0.00 | 0.38 | -16.26 | 96.27 | -30.19 | 127.62 | 0.6118 | -624.0 | -518.6 | |
| 0.00 | 2.73 | 0.00 | 1.85 | -22.22 | 93.79 | -32.67 | 132.86 | 0.6842 | -669.0 | -587.5 | |
| 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. | |