SDO HMI 2014-11-12 13:00:27 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 19.54 | 0.00 | 9.92 | -8.44 | 341.07 | -2.59 | 171.53 | 0.2180 | 117.4 | 301.7 | |
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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 | 2.50 | 0.00 | 1.25 | -4.94 | 347.45 | 3.79 | 205.11 | 0.1560 | 824.0 | 736.3 | |
| 0.00 | 1.46 | 0.00 | 0.73 | -4.24 | 345.12 | 1.47 | 191.23 | 0.1318 | 794.0 | 562.0 | |
| 0.00 | 3.01 | 0.00 | 1.51 | -6.61 | 343.27 | -0.38 | 177.77 | 0.1704 | 616.0 | 588.1 | |
| 0.00 | 3.27 | 0.00 | 1.66 | -9.51 | 342.27 | -1.38 | 173.82 | 0.2215 | 773.0 | 706.2 | |
| 0.00 | 1.12 | 0.00 | 0.57 | -9.82 | 342.06 | -1.59 | 173.04 | 0.2271 | 771.0 | 604.1 | |
| 0.00 | 2.24 | 0.00 | 1.14 | -10.98 | 341.48 | -2.17 | 171.32 | 0.2480 | 891.0 | 693.3 | |
| 0.00 | 0.86 | 0.00 | 0.44 | -11.13 | 340.09 | -3.57 | 166.09 | 0.2552 | 712.0 | 527.7 | |
| 0.00 | 0.60 | 0.00 | 0.31 | -12.19 | 336.93 | -6.72 | 156.58 | 0.2892 | -798.0 | -601.1 | |
| 0.00 | 0.95 | 0.00 | 0.49 | -9.92 | 336.68 | -6.97 | 152.11 | 0.2567 | -874.0 | -746.0 | |
| 0.00 | 1.29 | 0.00 | 0.66 | -10.05 | 336.38 | -7.28 | 151.31 | 0.2610 | -882.0 | -751.1 | |
| 0.00 | 1.64 | 0.00 | 0.84 | -8.01 | 333.33 | -10.32 | 137.34 | 0.2631 | -716.0 | -658.9 | |
| 0.00 | 0.60 | 0.00 | 0.32 | -11.40 | 329.03 | -14.62 | 135.24 | 0.3530 | -702.0 | -534.6 | |
| 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. | |