SDO HMI 2014-11-29 02:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 11.28 | 34.72 | 6.57 | 20.07 | 16.98 | 152.66 | 27.08 | 302.30 | 0.5170 | 294.5 | 118.4 | |
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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 | 1.62 | 0.00 | 0.96 | 17.77 | 154.43 | 28.84 | 302.12 | 0.5446 | 249.0 | 368.6 | |
| 7.78 | 11.03 | 4.57 | 6.48 | 17.53 | 154.24 | 28.66 | 301.86 | 0.5406 | 914.2 | 592.8 | |
| 0.00 | 0.94 | 0.00 | 0.55 | 17.87 | 154.30 | 28.72 | 302.37 | 0.5436 | 732.0 | 564.5 | |
| 0.00 | 0.60 | 0.00 | 0.35 | 17.28 | 153.95 | 28.37 | 301.69 | 0.5353 | 174.0 | 160.7 | |
| 0.00 | 1.03 | 0.00 | 0.59 | 16.46 | 152.87 | 27.29 | 301.19 | 0.5161 | 585.0 | 423.7 | |
| 0.00 | 1.97 | 0.00 | 1.13 | 15.49 | 152.59 | 27.01 | 299.71 | 0.5059 | 360.0 | 369.3 | |
| 2.22 | 5.30 | 1.27 | 3.03 | 15.52 | 152.39 | 26.80 | 299.93 | 0.5034 | 816.1 | 741.9 | |
| 0.00 | 1.03 | 0.00 | 0.59 | 15.22 | 152.28 | 26.69 | 299.48 | 0.5000 | 807.0 | 700.2 | |
| 0.00 | 1.54 | 0.00 | 0.88 | 16.69 | 151.87 | 26.29 | 302.46 | 0.5048 | 735.0 | 583.4 | |
| 0.00 | 0.86 | 0.00 | 0.49 | 17.37 | 151.32 | 25.74 | 304.16 | 0.5028 | -683.0 | -599.1 | |
| 0.00 | 3.42 | 0.00 | 1.95 | 17.50 | 150.55 | 24.97 | 305.13 | 0.4942 | -759.0 | -662.0 | |
| 0.00 | 1.28 | 0.00 | 0.73 | 16.86 | 150.45 | 24.87 | 304.09 | 0.4880 | -751.0 | -636.1 | |
| 0.00 | 1.28 | 0.00 | 0.73 | 17.01 | 150.41 | 24.83 | 304.41 | 0.4886 | -886.0 | -701.3 | |
| 1.28 | 2.82 | 0.73 | 1.61 | 18.03 | 150.46 | 24.87 | 306.14 | 0.4973 | -826.9 | -685.6 | |
| 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. | |