SDO HMI 2011-10-21 06:59:01 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 4.70 | 31.19 | 2.71 | 17.88 | -15.37 | 5.08 | 22.17 | 226.16 | 0.5058 | 184.5 | 260.3 | |
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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 | 1.57 | 0.00 | 0.91 | -15.08 | 7.47 | 24.55 | 229.57 | 0.5292 | 707.0 | 580.2 | |
| 0.00 | 1.13 | 0.00 | 0.66 | -16.91 | 6.79 | 23.87 | 226.14 | 0.5391 | 798.0 | 543.8 | |
| 3.31 | 9.23 | 1.91 | 5.34 | -15.11 | 6.49 | 23.57 | 228.39 | 0.5184 | 857.2 | 714.6 | |
| 0.00 | 0.96 | 0.00 | 0.55 | -14.72 | 6.38 | 23.46 | 228.84 | 0.5135 | 550.0 | 587.2 | |
| 0.00 | 2.87 | 0.00 | 1.66 | -15.85 | 5.97 | 23.05 | 226.67 | 0.5199 | 963.0 | 717.7 | |
| 0.00 | 2.53 | 0.00 | 1.47 | -16.20 | 5.84 | 22.93 | 226.01 | 0.5220 | 725.0 | 664.1 | |
| 0.00 | 0.96 | 0.00 | 0.56 | -16.32 | 5.66 | 22.74 | 225.60 | 0.5212 | 610.0 | 458.5 | |
| 1.39 | 3.48 | 0.80 | 1.99 | -15.17 | 4.72 | 21.80 | 226.10 | 0.4995 | 786.6 | 716.4 | |
| 0.00 | 1.05 | 0.00 | 0.60 | -16.59 | 4.24 | 21.33 | 223.41 | 0.5092 | -981.0 | -723.5 | |
| 0.00 | 1.83 | 0.00 | 1.02 | -13.83 | 2.84 | 19.92 | 225.59 | 0.4650 | -856.0 | -614.5 | |
| 0.00 | 2.53 | 0.00 | 1.41 | -14.82 | 1.98 | 19.06 | 222.81 | 0.4664 | -732.0 | -617.0 | |
| 0.00 | 1.39 | 0.00 | 0.78 | -15.04 | 2.00 | 19.08 | 222.51 | 0.4691 | -726.0 | -541.3 | |
| 0.00 | 1.66 | 0.00 | 0.93 | -16.22 | 0.67 | 17.75 | 218.79 | 0.4692 | -795.0 | -683.6 | |
| 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. | |