SDO HMI 2011-11-13 15:58:58 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 48.58 | 376.98 | 28.31 | 219.09 | 16.18 | 63.87 | 29.16 | 296.63 | 0.5256 | -831.3 | -362.9 | |
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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 | 0.67 | 18.61 | 65.43 | 30.72 | 299.61 | 0.5591 | -644.0 | -504.8 | |
| 0.00 | 0.77 | 0.00 | 0.46 | 18.78 | 64.77 | 30.07 | 300.35 | 0.5519 | -753.0 | -633.3 | |
| 48.58 | 357.62 | 28.31 | 208.25 | 16.03 | 64.21 | 29.50 | 296.03 | 0.5288 | -1349.6 | -398.1 | |
| 0.00 | 1.12 | 0.00 | 0.64 | 15.22 | 62.54 | 27.83 | 295.68 | 0.5019 | -743.0 | -561.7 | |
| 0.00 | 2.41 | 0.00 | 1.37 | 14.07 | 62.24 | 27.53 | 293.71 | 0.4918 | -918.0 | -755.4 | |
| 0.00 | 1.38 | 0.00 | 0.77 | 17.89 | 58.00 | 23.30 | 304.64 | 0.4594 | 744.0 | 591.7 | |
| 0.00 | 2.67 | 0.00 | 1.48 | 17.77 | 57.78 | 23.08 | 304.65 | 0.4557 | 918.0 | 698.3 | |
| 0.00 | 1.03 | 0.00 | 0.58 | 20.36 | 58.17 | 23.47 | 308.92 | 0.4819 | 631.0 | 505.5 | |
| 0.00 | 1.72 | 0.00 | 0.96 | 21.18 | 55.93 | 21.23 | 312.96 | 0.4633 | 771.0 | 665.2 | |
| 0.00 | 0.95 | 0.00 | 0.53 | 22.48 | 55.11 | 20.40 | 316.18 | 0.4671 | 831.0 | 593.4 | |
| 0.00 | 0.77 | 0.00 | 0.43 | 22.67 | 54.96 | 20.26 | 316.67 | 0.4676 | 819.0 | 659.0 | |
| 0.00 | 1.63 | 0.00 | 0.91 | 21.71 | 54.38 | 19.67 | 315.89 | 0.4513 | 773.0 | 697.4 | |
| 0.00 | 0.69 | 0.00 | 0.39 | 25.58 | 52.18 | 17.47 | 324.90 | 0.4729 | -857.0 | -719.8 | |
| 0.00 | 0.86 | 0.00 | 0.46 | 20.26 | 50.89 | 16.18 | 318.71 | 0.3980 | 688.0 | 581.8 | |
| 0.00 | 2.24 | 0.00 | 1.19 | 19.30 | 49.19 | 14.49 | 319.98 | 0.3688 | 775.0 | 651.0 | |
| 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. | |