SDO HMI 2014-11-29 01:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 10.09 | 32.49 | 5.85 | 18.67 | 17.01 | 152.54 | 26.41 | 302.94 | 0.5087 | 302.4 | 187.8 | |
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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 | 2.82 | 0.00 | 1.65 | 17.85 | 154.35 | 28.22 | 302.74 | 0.5372 | 602.0 | 491.9 | |
| 7.44 | 9.58 | 4.35 | 5.60 | 17.54 | 154.19 | 28.06 | 302.37 | 0.5331 | 942.2 | 669.4 | |
| 0.00 | 1.71 | 0.00 | 0.98 | 15.53 | 152.52 | 26.39 | 300.29 | 0.4980 | 715.0 | 577.7 | |
| 1.03 | 4.87 | 0.58 | 2.77 | 15.53 | 152.28 | 26.15 | 300.50 | 0.4949 | 830.5 | 776.8 | |
| 0.00 | 1.03 | 0.00 | 0.58 | 15.26 | 152.25 | 26.11 | 300.04 | 0.4925 | 841.0 | 762.8 | |
| 0.00 | 1.45 | 0.00 | 0.83 | 16.82 | 152.20 | 26.06 | 302.88 | 0.5028 | 692.0 | 590.4 | |
| 0.00 | 1.28 | 0.00 | 0.73 | 16.76 | 151.91 | 25.78 | 303.04 | 0.4988 | 817.0 | 660.5 | |
| 0.00 | 1.54 | 0.00 | 0.88 | 17.44 | 151.36 | 25.23 | 304.76 | 0.4970 | -635.0 | -531.7 | |
| 0.00 | 1.20 | 0.00 | 0.68 | 16.81 | 150.55 | 24.42 | 304.44 | 0.4818 | -705.0 | -580.0 | |
| 0.00 | 3.16 | 0.00 | 1.79 | 17.45 | 150.58 | 24.44 | 305.56 | 0.4873 | -819.0 | -684.5 | |
| 1.62 | 2.74 | 0.92 | 1.55 | 18.04 | 150.46 | 24.32 | 306.71 | 0.4906 | -823.7 | -635.0 | |
| 0.00 | 1.11 | 0.00 | 0.63 | 16.96 | 150.23 | 24.10 | 305.04 | 0.4791 | -840.0 | -702.8 | |
| 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. | |