SDO HMI 2014-03-24 14:00:31 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 11.00 | 36.32 | 7.62 | 25.64 | 3.16 | 137.43 | -44.34 | 78.60 | 0.7141 | -83.4 | 98.4 | |
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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 | 1.40 | 0.00 | 0.95 | 6.19 | 140.50 | -41.28 | 73.31 | 0.6870 | -514.0 | -462.5 | |
| 2.88 | 4.45 | 1.98 | 3.06 | 3.44 | 139.08 | -42.69 | 77.70 | 0.6951 | -740.2 | -555.0 | |
| 2.27 | 4.45 | 1.56 | 3.06 | 3.14 | 139.10 | -42.68 | 78.12 | 0.6940 | -638.2 | -419.4 | |
| 0.96 | 2.18 | 0.66 | 1.50 | 2.80 | 138.83 | -42.95 | 78.69 | 0.6963 | -481.8 | -331.6 | |
| 4.02 | 6.46 | 2.80 | 4.50 | 3.89 | 138.40 | -43.38 | 77.30 | 0.7047 | -657.0 | -562.9 | |
| 0.00 | 1.31 | 0.00 | 0.94 | 3.81 | 136.85 | -44.92 | 77.92 | 0.7229 | -585.0 | -485.3 | |
| 0.87 | 1.75 | 0.62 | 1.25 | 2.77 | 136.61 | -45.16 | 79.41 | 0.7229 | 524.8 | 475.4 | |
| 0.00 | 0.79 | 0.00 | 0.57 | 5.44 | 136.38 | -45.40 | 75.91 | 0.7331 | -457.0 | -381.9 | |
| 0.00 | 3.84 | 0.00 | 2.75 | 2.25 | 136.34 | -45.44 | 80.19 | 0.7248 | 788.0 | 670.3 | |
| 0.00 | 0.87 | 0.00 | 0.63 | 2.41 | 136.24 | -45.53 | 80.00 | 0.7263 | 302.0 | 378.2 | |
| 0.00 | 1.57 | 0.00 | 1.14 | 2.65 | 135.63 | -46.15 | 79.86 | 0.7341 | 418.0 | 323.6 | |
| 0.00 | 0.96 | 0.00 | 0.70 | 2.21 | 135.48 | -46.30 | 80.49 | 0.7348 | 698.0 | 585.0 | |
| 0.00 | 2.36 | 0.00 | 1.72 | 2.43 | 135.38 | -46.40 | 80.22 | 0.7365 | 638.0 | 591.3 | |
| 0.00 | 0.96 | 0.00 | 0.70 | 2.13 | 135.35 | -46.43 | 80.63 | 0.7361 | 391.0 | 415.8 | |
| 0.00 | 1.40 | 0.00 | 1.02 | 2.24 | 135.13 | -46.65 | 80.54 | 0.7390 | 496.0 | 398.2 | |
| 0.00 | 1.57 | 0.00 | 1.15 | 2.49 | 135.03 | -46.75 | 80.24 | 0.7407 | 566.0 | 409.6 | |
| 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. | |