SDO HMI 2014-11-22 16:00:26 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 22.97 | 0.00 | 12.24 | -12.55 | 225.97 | 15.79 | 226.41 | 0.3676 | -63.5 | 9.4 | |
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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 | 0.56 | -10.29 | 232.09 | 21.91 | 240.27 | 0.4246 | -750.0 | -610.5 | |
| 0.00 | 5.23 | 0.00 | 2.81 | -12.03 | 228.39 | 18.21 | 231.85 | 0.3903 | 790.0 | 649.0 | |
| 0.00 | 1.46 | 0.00 | 0.78 | -12.42 | 227.75 | 17.57 | 230.06 | 0.3861 | 882.0 | 687.5 | |
| 0.00 | 0.94 | 0.00 | 0.51 | -12.72 | 227.71 | 17.52 | 229.38 | 0.3886 | 787.0 | 650.3 | |
| 0.00 | 1.46 | 0.00 | 0.79 | -13.64 | 227.68 | 17.49 | 227.53 | 0.3978 | 795.0 | 681.2 | |
| 0.00 | 0.86 | 0.00 | 0.46 | -12.38 | 227.05 | 16.86 | 229.01 | 0.3770 | 841.0 | 673.1 | |
| 0.00 | 0.60 | 0.00 | 0.32 | -13.24 | 227.01 | 16.83 | 227.23 | 0.3856 | 738.0 | 588.7 | |
| 0.00 | 1.11 | 0.00 | 0.60 | -12.62 | 226.91 | 16.72 | 228.28 | 0.3778 | 976.0 | 809.4 | |
| 0.00 | 1.71 | 0.00 | 0.90 | -11.46 | 223.52 | 13.33 | 224.35 | 0.3247 | -869.0 | -686.5 | |
| 0.00 | 0.69 | 0.00 | 0.36 | -11.98 | 223.54 | 13.36 | 223.29 | 0.3311 | -841.0 | -680.1 | |
| 0.00 | 1.97 | 0.00 | 1.04 | -13.91 | 223.39 | 13.21 | 219.15 | 0.3529 | -775.0 | -644.0 | |
| 0.00 | 0.77 | 0.00 | 0.41 | -13.50 | 223.09 | 12.91 | 219.26 | 0.3448 | -930.0 | -779.9 | |
| 0.00 | 1.37 | 0.00 | 0.72 | -12.80 | 222.96 | 12.78 | 220.35 | 0.3346 | -829.0 | -673.4 | |
| 0.00 | 2.14 | 0.00 | 1.13 | -13.75 | 222.95 | 12.76 | 218.49 | 0.3464 | -815.0 | -623.6 | |
| 0.00 | 1.63 | 0.00 | 0.85 | -12.06 | 222.83 | 12.65 | 221.56 | 0.3242 | -952.0 | -830.5 | |
| 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. | |