SDO HMI 2014-11-10 03:00:27 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 12.93 | 0.00 | 8.44 | -9.22 | 336.77 | -38.72 | 108.46 | 0.6529 | -107.4 | -119.9 | |
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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 | 0.78 | 0.00 | 0.48 | -9.59 | 341.45 | -34.04 | 111.30 | 0.5947 | 578.0 | 469.9 | |
| 0.00 | 0.95 | 0.00 | 0.60 | -11.81 | 339.90 | -35.59 | 113.86 | 0.6252 | 608.0 | 499.0 | |
| 0.00 | 1.55 | 0.00 | 0.96 | -6.94 | 339.89 | -35.60 | 106.31 | 0.6043 | 652.0 | 603.2 | |
| 0.00 | 1.47 | 0.00 | 0.91 | -6.98 | 339.66 | -35.82 | 106.27 | 0.6074 | 669.0 | 528.5 | |
| 0.00 | 1.03 | 0.00 | 0.69 | -11.75 | 335.80 | -39.69 | 111.66 | 0.6751 | -557.0 | -496.2 | |
| 0.00 | 0.26 | 0.00 | 0.17 | -6.20 | 336.37 | -39.11 | 103.79 | 0.6481 | -525.0 | -491.7 | |
| 0.00 | 2.93 | 0.00 | 1.95 | -9.74 | 335.49 | -40.00 | 108.67 | 0.6711 | -351.0 | -373.0 | |
| 0.00 | 0.43 | 0.00 | 0.29 | -8.88 | 334.90 | -40.59 | 107.21 | 0.6753 | -577.0 | -492.4 | |
| 0.00 | 0.60 | 0.00 | 0.41 | -10.99 | 334.09 | -41.40 | 109.85 | 0.6925 | -352.0 | -301.1 | |
| 0.00 | 1.90 | 0.00 | 1.28 | -9.30 | 334.32 | -41.17 | 107.58 | 0.6838 | -678.0 | -599.7 | |
| 0.00 | 1.03 | 0.00 | 0.70 | -8.48 | 334.27 | -41.21 | 106.40 | 0.6817 | -648.0 | -585.7 | |
| 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. | |