SDO HMI 2014-11-04 06:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 18.92 | 0.00 | 11.02 | -21.87 | 75.96 | -17.00 | 149.59 | 0.5134 | 525.9 | 382.8 | |
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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 | 0.78 | -15.13 | 86.33 | -6.63 | 161.25 | 0.3482 | 840.0 | 705.2 | |
| 0.00 | 1.64 | 0.00 | 0.89 | -17.95 | 84.24 | -8.72 | 158.91 | 0.4025 | 917.0 | 699.8 | |
| 0.00 | 1.21 | 0.00 | 0.67 | -20.62 | 83.19 | -9.77 | 159.13 | 0.4477 | 336.0 | 313.1 | |
| 0.00 | 0.95 | 0.00 | 0.53 | -20.32 | 79.03 | -13.93 | 151.21 | 0.4707 | 663.0 | 533.4 | |
| 0.00 | 1.47 | 0.00 | 0.83 | -20.49 | 78.65 | -14.31 | 150.75 | 0.4757 | 589.0 | 457.2 | |
| 0.00 | 1.21 | 0.00 | 0.68 | -20.69 | 78.17 | -14.79 | 150.17 | 0.4821 | 826.0 | 613.8 | |
| 0.00 | 0.78 | 0.00 | 0.45 | -22.72 | 77.52 | -15.44 | 151.28 | 0.5131 | 676.0 | 538.7 | |
| 0.00 | 2.25 | 0.00 | 1.30 | -22.81 | 76.40 | -16.56 | 149.68 | 0.5225 | 715.0 | 395.8 | |
| 0.00 | 1.82 | 0.00 | 1.03 | -20.53 | 76.51 | -16.45 | 147.31 | 0.4932 | 877.0 | 632.2 | |
| 0.00 | 1.21 | 0.00 | 0.69 | -20.99 | 76.45 | -16.51 | 147.76 | 0.4993 | 603.0 | 419.4 | |
| 0.00 | 0.86 | 0.00 | 0.51 | -22.23 | 73.70 | -19.26 | 145.20 | 0.5371 | 693.0 | 514.3 | |
| 0.00 | 0.86 | 0.00 | 0.52 | -24.66 | 72.98 | -19.98 | 146.92 | 0.5712 | 641.0 | 523.7 | |
| 0.00 | 0.86 | 0.00 | 0.51 | -22.14 | 73.27 | -19.69 | 144.52 | 0.5397 | 666.0 | 548.6 | |
| 0.00 | 1.12 | 0.00 | 0.77 | -28.32 | 63.00 | -29.96 | 140.18 | 0.6887 | -641.0 | -601.1 | |
| 0.00 | 1.21 | 0.00 | 0.86 | -28.79 | 59.98 | -32.98 | 138.14 | 0.7172 | -513.0 | -347.3 | |
| 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. | |