SDO HMI 2013-01-06 22:58:54 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 49.09 | 300.35 | 25.99 | 159.18 | -24.34 | 250.40 | 1.82 | 184.72 | 0.3560 | 742.4 | 329.2 | |
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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 | 1.44 | 0.00 | 0.76 | -22.33 | 251.97 | 3.39 | 189.71 | 0.3255 | -817.0 | -687.6 | |
| 49.09 | 282.63 | 25.99 | 149.74 | -24.34 | 250.76 | 2.18 | 185.61 | 0.3556 | 1458.5 | 408.2 | |
| 0.00 | 1.27 | 0.00 | 0.68 | -26.02 | 249.38 | 0.79 | 181.88 | 0.3815 | -768.0 | -539.3 | |
| 0.00 | 1.10 | 0.00 | 0.58 | -23.61 | 245.79 | -2.79 | 172.54 | 0.3448 | -819.0 | -677.5 | |
| 0.00 | 2.12 | 0.00 | 1.12 | -23.64 | 245.47 | -3.11 | 171.70 | 0.3461 | -948.0 | -850.4 | |
| 0.00 | 0.76 | 0.00 | 0.41 | -24.93 | 245.44 | -3.15 | 172.17 | 0.3670 | -730.0 | -650.9 | |
| 0.00 | 0.93 | 0.00 | 0.50 | -24.77 | 245.15 | -3.43 | 171.39 | 0.3651 | -730.0 | -624.0 | |
| 0.00 | 3.65 | 0.00 | 1.93 | -23.89 | 244.98 | -3.60 | 170.54 | 0.3513 | -721.0 | -751.0 | |
| 0.00 | 1.87 | 0.00 | 0.99 | -23.63 | 244.18 | -4.40 | 168.35 | 0.3496 | -888.0 | -792.1 | |
| 0.00 | 0.93 | 0.00 | 0.50 | -25.64 | 242.17 | -6.41 | 164.92 | 0.3888 | -803.0 | -700.9 | |
| 0.00 | 1.10 | 0.00 | 0.58 | -22.36 | 241.05 | -7.53 | 159.27 | 0.3439 | -771.0 | -609.1 | |
| 0.00 | 1.02 | 0.00 | 0.54 | -22.17 | 240.94 | -7.65 | 158.76 | 0.3418 | -891.0 | -689.9 | |
| 0.00 | 1.53 | 0.00 | 0.85 | -28.83 | 239.19 | -9.39 | 161.42 | 0.4505 | -816.0 | -648.5 | |
| 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. | |