SDO HMI 2014-11-14 06:00:27 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 14.11 | 42.93 | 9.48 | 29.16 | 8.55 | 4.08 | 42.97 | 279.39 | 0.6854 | -73.6 | -278.8 | |
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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 | 1.20 | 0.00 | 0.84 | 8.40 | 5.94 | 44.83 | 278.94 | 0.7084 | -405.0 | -305.6 | |
| 5.77 | 15.23 | 4.00 | 10.59 | 8.12 | 5.52 | 44.41 | 278.58 | 0.7030 | -938.0 | -535.4 | |
| 0.00 | 1.20 | 0.00 | 0.84 | 8.47 | 5.57 | 44.46 | 279.09 | 0.7039 | -590.0 | -469.9 | |
| 0.00 | 2.07 | 0.00 | 1.43 | 8.22 | 5.20 | 44.09 | 278.76 | 0.6991 | -873.0 | -761.9 | |
| 0.00 | 1.89 | 0.00 | 1.30 | 8.08 | 4.97 | 43.86 | 278.58 | 0.6961 | -875.0 | -771.1 | |
| 0.00 | 1.29 | 0.00 | 0.88 | 8.14 | 4.77 | 43.66 | 278.70 | 0.6937 | -696.0 | -563.3 | |
| 0.00 | 3.70 | 0.00 | 2.52 | 8.13 | 4.44 | 43.33 | 278.71 | 0.6895 | -762.0 | -720.3 | |
| 0.00 | 1.72 | 0.00 | 1.15 | 9.74 | 2.75 | 41.64 | 281.31 | 0.6702 | 563.0 | 459.9 | |
| 0.34 | 1.64 | 0.23 | 1.08 | 10.12 | 2.21 | 41.10 | 281.97 | 0.6638 | 860.5 | 747.1 | |
| 0.00 | 1.03 | 0.00 | 0.68 | 10.30 | 2.20 | 41.08 | 282.25 | 0.6640 | 600.0 | 516.8 | |
| 6.54 | 9.21 | 4.29 | 6.04 | 8.72 | 1.84 | 40.73 | 279.93 | 0.6571 | 854.0 | 582.3 | |
| 1.46 | 2.75 | 0.96 | 1.81 | 9.59 | 1.93 | 40.81 | 281.23 | 0.6594 | 738.1 | 662.6 | |
| 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. | |