SDO HMI 2014-11-22 10:00:26 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 24.28 | 0.00 | 12.79 | -13.73 | 225.58 | 12.11 | 216.73 | 0.3409 | -395.7 | -66.3 | |
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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 | 0.77 | 0.00 | 0.42 | -15.40 | 231.37 | 17.90 | 224.93 | 0.4213 | -740.0 | -624.9 | |
| 0.00 | 1.29 | 0.00 | 0.68 | -12.35 | 228.54 | 15.07 | 225.87 | 0.3553 | 679.0 | 461.9 | |
| 0.00 | 6.95 | 0.00 | 3.68 | -13.60 | 227.64 | 14.17 | 221.65 | 0.3595 | 483.0 | 758.6 | |
| 0.00 | 0.94 | 0.00 | 0.50 | -13.04 | 227.23 | 13.76 | 221.91 | 0.3484 | 845.0 | 707.7 | |
| 0.00 | 1.29 | 0.00 | 0.71 | -19.47 | 227.50 | 14.03 | 212.07 | 0.4322 | -738.0 | -584.9 | |
| 0.00 | 1.46 | 0.00 | 0.77 | -13.10 | 226.99 | 13.51 | 221.28 | 0.3464 | 934.0 | 798.2 | |
| 0.00 | 1.20 | 0.00 | 0.62 | -11.97 | 223.43 | 9.96 | 215.12 | 0.2954 | -948.0 | -673.4 | |
| 0.00 | 1.72 | 0.00 | 0.90 | -13.96 | 223.36 | 9.88 | 211.29 | 0.3222 | -864.0 | -746.4 | |
| 0.00 | 1.20 | 0.00 | 0.63 | -14.15 | 223.37 | 9.89 | 211.00 | 0.3248 | -695.0 | -523.3 | |
| 0.00 | 0.86 | 0.00 | 0.45 | -13.41 | 223.18 | 9.70 | 211.77 | 0.3128 | -781.0 | -577.3 | |
| 0.00 | 1.20 | 0.00 | 0.63 | -15.35 | 223.17 | 9.70 | 208.64 | 0.3403 | -833.0 | -661.7 | |
| 0.00 | 0.86 | 0.00 | 0.44 | -12.09 | 222.82 | 9.35 | 213.22 | 0.2912 | -959.0 | -779.0 | |
| 0.00 | 2.14 | 0.00 | 1.12 | -13.77 | 222.79 | 9.32 | 210.13 | 0.3147 | -889.0 | -751.5 | |
| 0.00 | 2.40 | 0.00 | 1.24 | -12.00 | 222.64 | 9.16 | 212.87 | 0.2882 | -1034.0 | -779.7 | |
| 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. | |