SDO HMI 2014-11-30 03:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 19.32 | 0.00 | 11.20 | -23.89 | 92.36 | -19.49 | 144.04 | 0.5218 | -287.0 | -361.6 | |
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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 | 0.94 | 0.00 | 0.53 | -24.90 | 97.80 | -14.06 | 153.22 | 0.4910 | 715.0 | 571.2 | |
| 0.00 | 1.28 | 0.00 | 0.73 | -23.57 | 94.84 | -17.02 | 147.14 | 0.4965 | 775.0 | 681.3 | |
| 0.00 | 0.34 | 0.00 | 0.20 | -25.60 | 94.37 | -17.48 | 148.80 | 0.5251 | 588.0 | 609.2 | |
| 0.00 | 0.86 | 0.00 | 0.48 | -20.61 | 94.15 | -17.71 | 142.26 | 0.4671 | -661.0 | -527.5 | |
| 0.00 | 1.28 | 0.00 | 0.74 | -23.97 | 93.15 | -18.71 | 145.19 | 0.5155 | -939.0 | -755.7 | |
| 0.00 | 2.99 | 0.00 | 1.73 | -24.00 | 92.77 | -19.09 | 144.71 | 0.5192 | -779.0 | -608.9 | |
| 0.00 | 1.20 | 0.00 | 0.69 | -24.07 | 92.55 | -19.31 | 144.49 | 0.5218 | -812.0 | -675.4 | |
| 0.00 | 2.74 | 0.00 | 1.59 | -24.23 | 92.49 | -19.37 | 144.61 | 0.5243 | -579.0 | -577.7 | |
| 0.00 | 1.28 | 0.00 | 0.73 | -20.72 | 91.99 | -19.86 | 139.29 | 0.4893 | -541.0 | -530.3 | |
| 0.00 | 2.65 | 0.00 | 1.57 | -25.49 | 90.67 | -21.18 | 143.78 | 0.5542 | -798.0 | -615.1 | |
| 0.00 | 1.11 | 0.00 | 0.66 | -25.20 | 90.27 | -21.59 | 142.93 | 0.5544 | -827.0 | -593.5 | |
| 0.00 | 1.54 | 0.00 | 0.91 | -25.10 | 90.08 | -21.78 | 142.58 | 0.5551 | -635.0 | -418.4 | |
| 0.00 | 1.11 | 0.00 | 0.64 | -20.47 | 90.54 | -21.31 | 137.01 | 0.5014 | 762.0 | 636.5 | |
| 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. | |