SDO HMI 2014-11-24 17:00:26 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.51 | 20.72 | 0.37 | 14.54 | -13.08 | 226.16 | 42.89 | 249.48 | 0.7096 | 129.1 | 97.8 | |
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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 | 1.11 | 0.00 | 0.81 | -13.04 | 228.62 | 45.35 | 250.46 | 0.7378 | 461.0 | 415.5 | |
| 0.00 | 1.37 | 0.00 | 1.00 | -13.28 | 228.46 | 45.19 | 250.09 | 0.7367 | 508.0 | 366.6 | |
| 0.00 | 2.40 | 0.00 | 1.73 | -12.60 | 228.09 | 44.82 | 250.86 | 0.7305 | 627.0 | 492.9 | |
| 0.00 | 0.94 | 0.00 | 0.68 | -12.78 | 228.04 | 44.77 | 250.60 | 0.7305 | 594.0 | 475.8 | |
| 0.51 | 2.40 | 0.37 | 1.73 | -12.96 | 227.91 | 44.64 | 250.32 | 0.7296 | 745.2 | 626.6 | |
| 0.00 | 1.28 | 0.00 | 0.93 | -13.58 | 227.93 | 44.66 | 249.51 | 0.7317 | 571.0 | 452.5 | |
| 0.00 | 0.86 | 0.00 | 0.61 | -12.95 | 227.48 | 44.21 | 250.18 | 0.7247 | 687.0 | 637.5 | |
| 0.00 | 1.03 | 0.00 | 0.74 | -13.41 | 227.50 | 44.23 | 249.58 | 0.7264 | 704.0 | 563.4 | |
| 0.00 | 0.86 | 0.00 | 0.62 | -14.12 | 227.59 | 44.31 | 248.67 | 0.7297 | 617.0 | 549.9 | |
| 0.00 | 0.94 | 0.00 | 0.63 | -10.47 | 223.81 | 40.54 | 252.30 | 0.6733 | -630.0 | -422.3 | |
| 0.00 | 1.11 | 0.00 | 0.75 | -11.75 | 224.02 | 40.75 | 250.55 | 0.6802 | -576.0 | -502.5 | |
| 0.00 | 2.57 | 0.00 | 1.73 | -13.48 | 223.51 | 40.24 | 247.90 | 0.6804 | -671.0 | -500.4 | |
| 0.00 | 1.28 | 0.00 | 0.86 | -12.74 | 223.17 | 39.90 | 248.80 | 0.6734 | -696.0 | -591.4 | |
| 0.00 | 1.37 | 0.00 | 0.92 | -13.13 | 223.13 | 39.86 | 248.21 | 0.6745 | -665.0 | -583.7 | |
| 0.00 | 1.20 | 0.00 | 0.80 | -15.51 | 222.08 | 38.81 | 244.37 | 0.6721 | -567.0 | -454.9 | |
| 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. | |