SDO HMI 2014-04-10 21:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 19.41 | 0.00 | 10.14 | -15.32 | 298.98 | -14.66 | 125.80 | 0.3002 | -155.8 | -173.5 | |
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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 | 1.41 | 0.00 | 0.70 | -12.12 | 310.43 | -3.21 | 153.08 | 0.1213 | 893.0 | 671.6 | |
| 0.00 | 1.50 | 0.00 | 0.75 | -11.60 | 309.27 | -4.37 | 142.94 | 0.1243 | 744.0 | 572.9 | |
| 0.00 | 0.62 | 0.00 | 0.31 | -17.97 | 307.92 | -5.71 | 155.62 | 0.2302 | 870.0 | 710.3 | |
| 0.00 | 1.15 | 0.00 | 0.58 | -17.50 | 307.59 | -6.04 | 153.45 | 0.2256 | 745.0 | 614.7 | |
| 0.00 | 2.12 | 0.00 | 1.06 | -6.62 | 305.87 | -7.76 | 95.43 | 0.1354 | 1040.0 | 828.8 | |
| 0.00 | 1.23 | 0.00 | 0.65 | -14.13 | 296.69 | -16.95 | 117.43 | 0.3199 | -875.0 | -683.1 | |
| 0.00 | 0.44 | 0.00 | 0.23 | -16.59 | 296.34 | -17.29 | 123.59 | 0.3434 | -878.0 | -712.0 | |
| 0.00 | 1.23 | 0.00 | 0.65 | -14.49 | 296.49 | -17.14 | 118.20 | 0.3252 | -789.0 | -653.4 | |
| 0.00 | 1.68 | 0.00 | 0.88 | -16.86 | 296.15 | -17.48 | 124.00 | 0.3483 | -801.0 | -683.2 | |
| 0.00 | 1.50 | 0.00 | 0.79 | -14.36 | 296.34 | -17.29 | 117.66 | 0.3265 | -706.0 | -577.9 | |
| 0.00 | 1.15 | 0.00 | 0.61 | -17.05 | 295.47 | -18.16 | 123.54 | 0.3590 | -871.0 | -723.4 | |
| 0.00 | 1.59 | 0.00 | 0.85 | -17.46 | 293.13 | -20.50 | 121.64 | 0.3942 | -777.0 | -537.3 | |
| 0.00 | 3.79 | 0.00 | 2.08 | -19.97 | 291.57 | -22.07 | 125.23 | 0.4341 | -620.0 | -544.6 | |
| 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. | |