SDO HMI 2014-04-12 02:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 24.62 | 0.00 | 13.93 | -21.40 | 321.04 | 23.36 | 230.71 | 0.4751 | -144.8 | -189.5 | |
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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 | 0.79 | 0.00 | 0.51 | -14.82 | 336.74 | 39.07 | 253.72 | 0.6370 | 478.0 | 444.7 | |
| 0.00 | 1.59 | 0.00 | 0.97 | -15.73 | 332.78 | 35.11 | 251.12 | 0.5872 | 732.0 | 576.7 | |
| 0.00 | 1.41 | 0.00 | 0.87 | -21.03 | 332.22 | 34.55 | 242.25 | 0.6004 | 474.0 | 443.1 | |
| 0.00 | 1.77 | 0.00 | 1.06 | -17.03 | 331.02 | 33.35 | 248.25 | 0.5682 | 667.0 | 539.0 | |
| 0.00 | 1.59 | 0.00 | 0.96 | -18.85 | 330.96 | 33.28 | 245.13 | 0.5746 | 573.0 | 334.9 | |
| 0.00 | 1.59 | 0.00 | 0.91 | -18.88 | 325.39 | 27.71 | 241.76 | 0.5015 | 738.0 | 438.8 | |
| 0.00 | 1.59 | 0.00 | 0.89 | -22.67 | 320.33 | 22.66 | 230.16 | 0.4649 | -757.0 | -586.1 | |
| 0.00 | 1.32 | 0.00 | 0.73 | -23.67 | 317.03 | 19.35 | 224.29 | 0.4365 | -715.0 | -570.6 | |
| 0.00 | 5.21 | 0.00 | 2.83 | -22.06 | 316.07 | 18.40 | 225.86 | 0.4093 | -900.0 | -712.8 | |
| 0.00 | 1.41 | 0.00 | 0.77 | -24.14 | 315.99 | 18.31 | 222.00 | 0.4303 | -855.0 | -670.2 | |
| 0.00 | 1.94 | 0.00 | 1.06 | -24.67 | 314.33 | 16.66 | 218.60 | 0.4193 | -448.0 | -296.3 | |
| 0.00 | 1.41 | 0.00 | 0.77 | -25.11 | 314.29 | 16.62 | 217.81 | 0.4241 | -843.0 | -773.2 | |
| 0.00 | 1.59 | 0.00 | 0.85 | -24.31 | 310.60 | 12.93 | 212.59 | 0.3801 | -445.0 | -339.1 | |
| 0.00 | 1.41 | 0.00 | 0.75 | -25.36 | 307.01 | 9.34 | 203.64 | 0.3673 | -726.0 | -581.5 | |
| 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. | |