SDO HMI 2014-11-21 15:00:26 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 31.98 | 0.00 | 16.41 | -12.71 | 224.56 | 0.65 | 182.29 | 0.2612 | -535.5 | -488.0 | |
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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 | 0.86 | 0.00 | 0.44 | -10.24 | 232.11 | 8.20 | 213.38 | 0.2563 | -907.0 | -774.0 | |
| 0.00 | 1.29 | 0.00 | 0.66 | -9.87 | 231.20 | 7.28 | 211.12 | 0.2427 | -980.0 | -832.7 | |
| 0.00 | 1.03 | 0.00 | 0.54 | -15.19 | 231.25 | 7.33 | 202.55 | 0.3227 | -818.0 | -593.6 | |
| 0.00 | 0.77 | 0.00 | 0.40 | -12.99 | 227.52 | 3.60 | 193.26 | 0.2683 | 819.0 | 656.2 | |
| 0.00 | 1.20 | 0.00 | 0.62 | -12.56 | 227.18 | 3.26 | 192.40 | 0.2599 | 1163.0 | 944.9 | |
| 0.00 | 3.26 | 0.00 | 1.68 | -13.32 | 227.16 | 3.24 | 191.71 | 0.2725 | 956.0 | 876.3 | |
| 0.00 | 1.11 | 0.00 | 0.59 | -19.57 | 226.06 | 2.15 | 185.46 | 0.3723 | -709.0 | -497.2 | |
| 0.00 | 3.17 | 0.00 | 1.62 | -12.43 | 223.27 | -0.65 | 177.47 | 0.2519 | -919.0 | -746.9 | |
| 0.00 | 1.46 | 0.00 | 0.74 | -10.63 | 223.27 | -0.64 | 177.13 | 0.2213 | -1105.0 | -897.5 | |
| 0.00 | 3.17 | 0.00 | 1.62 | -12.03 | 223.15 | -0.77 | 176.92 | 0.2453 | -959.0 | -774.1 | |
| 0.00 | 6.60 | 0.00 | 3.37 | -12.21 | 223.05 | -0.86 | 176.60 | 0.2485 | -1203.0 | -884.1 | |
| 0.00 | 1.63 | 0.00 | 0.83 | -11.45 | 223.03 | -0.89 | 176.29 | 0.2356 | -936.0 | -704.8 | |
| 0.00 | 1.46 | 0.00 | 0.74 | -12.06 | 222.69 | -1.22 | 175.11 | 0.2463 | -843.0 | -734.5 | |
| 0.00 | 3.00 | 0.00 | 1.55 | -14.21 | 222.40 | -1.51 | 174.79 | 0.2829 | -926.0 | -618.8 | |
| 0.00 | 1.97 | 0.00 | 1.01 | -13.19 | 221.68 | -2.23 | 171.80 | 0.2674 | -666.0 | -605.8 | |
| 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. | |