SDO HMI 2014-11-22 08:00:26 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.34 | 23.66 | 0.18 | 12.36 | -12.89 | 225.86 | 11.30 | 216.30 | 0.3218 | -44.3 | 161.5 | |
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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 | 1.03 | 0.00 | 0.54 | -13.40 | 228.35 | 13.78 | 221.24 | 0.3531 | 775.0 | 637.3 | |
| 0.00 | 1.46 | 0.00 | 0.77 | -12.51 | 228.17 | 13.61 | 222.65 | 0.3405 | 728.0 | 536.2 | |
| 0.34 | 7.89 | 0.18 | 4.16 | -13.49 | 227.66 | 13.10 | 219.65 | 0.3468 | 993.5 | 745.1 | |
| 0.00 | 1.89 | 0.00 | 0.99 | -13.18 | 227.58 | 13.02 | 220.07 | 0.3422 | 948.0 | 736.9 | |
| 0.00 | 0.94 | 0.00 | 0.49 | -12.14 | 227.34 | 12.78 | 221.65 | 0.3268 | 893.0 | 704.2 | |
| 0.00 | 1.20 | 0.00 | 0.63 | -13.20 | 226.81 | 12.24 | 218.32 | 0.3344 | 700.0 | 639.4 | |
| 0.00 | 1.20 | 0.00 | 0.62 | -11.99 | 223.64 | 9.07 | 212.62 | 0.2874 | -780.0 | -546.4 | |
| 0.00 | 0.94 | 0.00 | 0.49 | -11.98 | 223.42 | 8.86 | 212.01 | 0.2854 | -870.0 | -612.3 | |
| 0.00 | 0.94 | 0.00 | 0.48 | -10.55 | 223.29 | 8.72 | 214.53 | 0.2642 | -790.0 | -593.5 | |
| 0.00 | 1.11 | 0.00 | 0.58 | -14.19 | 223.35 | 8.78 | 208.01 | 0.3165 | -767.0 | -631.7 | |
| 0.00 | 1.54 | 0.00 | 0.80 | -12.13 | 222.81 | 8.25 | 209.94 | 0.2823 | -908.0 | -762.0 | |
| 0.00 | 2.49 | 0.00 | 1.28 | -12.01 | 222.57 | 8.00 | 209.41 | 0.2784 | -909.0 | -760.2 | |
| 0.00 | 1.03 | 0.00 | 0.53 | -13.79 | 222.59 | 8.03 | 206.54 | 0.3048 | -776.0 | -682.7 | |
| 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. | |