SDO HMI 2014-03-30 07:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 18.60 | 0.00 | 11.24 | 4.09 | 139.72 | 33.24 | 287.02 | 0.5740 | -9.3 | -81.4 | |
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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 | 1.05 | 0.00 | 0.66 | 3.97 | 142.40 | 35.93 | 285.49 | 0.6096 | -643.0 | -508.9 | |
| 0.00 | 0.88 | 0.00 | 0.55 | 4.69 | 142.22 | 35.74 | 286.71 | 0.6101 | -700.0 | -496.5 | |
| 0.00 | 3.16 | 0.00 | 1.97 | 5.05 | 142.17 | 35.69 | 287.30 | 0.6110 | -657.0 | -561.7 | |
| 0.00 | 0.79 | 0.00 | 0.49 | 4.93 | 141.24 | 34.76 | 287.58 | 0.5981 | -529.0 | -514.6 | |
| 0.00 | 1.23 | 0.00 | 0.76 | 4.68 | 141.08 | 34.60 | 287.26 | 0.5949 | -819.0 | -680.5 | |
| 0.00 | 1.14 | 0.00 | 0.69 | 1.16 | 140.69 | 34.22 | 281.63 | 0.5762 | -82.0 | -86.3 | |
| 0.00 | 1.14 | 0.00 | 0.71 | 7.02 | 140.88 | 34.40 | 291.07 | 0.6032 | -683.0 | -550.2 | |
| 0.00 | 1.23 | 0.00 | 0.74 | 3.62 | 140.22 | 33.75 | 285.96 | 0.5788 | -594.0 | -490.1 | |
| 0.00 | 1.23 | 0.00 | 0.73 | 3.00 | 138.73 | 32.25 | 285.69 | 0.5557 | 727.0 | 442.1 | |
| 0.00 | 1.05 | 0.00 | 0.62 | 4.71 | 137.82 | 31.34 | 289.16 | 0.5508 | 584.0 | 471.5 | |
| 0.00 | 0.88 | 0.00 | 0.51 | 2.29 | 137.51 | 31.03 | 285.07 | 0.5356 | 714.0 | 656.3 | |
| 0.00 | 1.05 | 0.00 | 0.62 | 4.38 | 137.41 | 30.93 | 288.83 | 0.5437 | 853.0 | 719.2 | |
| 0.00 | 0.96 | 0.00 | 0.57 | 3.85 | 137.11 | 30.63 | 288.08 | 0.5368 | 818.0 | 598.8 | |
| 0.00 | 0.79 | 0.00 | 0.45 | -1.28 | 136.82 | 30.34 | 278.73 | 0.5130 | 539.0 | 435.2 | |
| 0.00 | 2.02 | 0.00 | 1.17 | 4.97 | 136.01 | 29.53 | 290.78 | 0.5273 | 332.0 | 373.3 | |
| 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. | |