SDO HMI 2014-11-03 09:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 18.43 | 52.85 | 10.99 | 31.90 | 5.73 | 69.65 | -34.85 | 85.91 | 0.5713 | -42.7 | 39.6 | |
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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 | 1.12 | 0.00 | 0.65 | 5.96 | 73.17 | -31.33 | 85.34 | 0.5210 | -367.0 | -359.7 | |
| 3.29 | 26.56 | 1.91 | 15.44 | 5.63 | 73.02 | -31.49 | 85.98 | 0.5232 | -1109.0 | -675.1 | |
| 6.40 | -2.00 | 3.72 | -2.00 | 5.80 | 72.87 | -31.64 | 85.66 | 0.5255 | -995.6 | 999999 | |
| 0.00 | 1.21 | 0.00 | 0.70 | 5.23 | 72.76 | -31.75 | 86.75 | 0.5269 | -666.0 | -489.0 | |
| 3.55 | -2.00 | 2.07 | -2.00 | 5.50 | 72.61 | -31.90 | 86.26 | 0.5293 | -832.7 | 999999 | |
| 0.00 | 0.87 | 0.00 | 0.51 | 5.09 | 71.24 | -33.26 | 87.04 | 0.5492 | -752.0 | -558.7 | |
| 0.00 | 1.30 | 0.00 | 0.81 | 6.05 | 67.03 | -37.48 | 85.46 | 0.6093 | 813.0 | 694.8 | |
| 0.00 | 1.47 | 0.00 | 0.92 | 6.25 | 66.82 | -37.69 | 85.14 | 0.6122 | 682.0 | 614.5 | |
| 0.00 | 0.69 | 0.00 | 0.43 | 6.11 | 66.41 | -38.09 | 85.38 | 0.6177 | 681.0 | 635.8 | |
| 0.00 | 4.15 | 0.00 | 2.62 | 6.07 | 66.11 | -38.39 | 85.46 | 0.6218 | 529.0 | 537.4 | |
| 0.00 | 1.38 | 0.00 | 0.87 | 6.96 | 66.03 | -38.47 | 84.02 | 0.6232 | 739.0 | 651.4 | |
| 4.50 | 7.53 | 2.84 | 4.75 | 5.62 | 66.03 | -38.47 | 86.18 | 0.6228 | 821.9 | 566.3 | |
| 0.00 | 0.52 | 0.00 | 0.33 | 6.95 | 65.84 | -38.67 | 84.05 | 0.6258 | 592.0 | 507.5 | |
| 0.00 | 2.42 | 0.00 | 1.53 | 5.07 | 65.84 | -38.66 | 87.06 | 0.6254 | 807.0 | 656.0 | |
| 0.69 | 3.63 | 0.45 | 2.34 | 5.56 | 64.69 | -39.82 | 86.29 | 0.6410 | 837.9 | 679.0 | |
| 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. | |