SDO HMI 2014-04-14 04:00:34 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 66.93 | 410.47 | 34.85 | 213.85 | 11.66 | 274.90 | 4.73 | 344.78 | 0.3108 | -956.2 | -405.8 | |
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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 | 0.74 | 9.30 | 280.52 | 10.35 | 325.42 | 0.3137 | -850.0 | -598.1 | |
| 66.93 | 394.04 | 34.85 | 205.19 | 11.58 | 275.08 | 4.91 | 344.20 | 0.3097 | -1470.5 | -444.4 | |
| 0.00 | 1.06 | 0.00 | 0.56 | 13.76 | 273.33 | 3.16 | 350.86 | 0.3387 | -735.0 | -538.3 | |
| 0.00 | 1.41 | 0.00 | 0.74 | 13.66 | 273.11 | 2.94 | 351.44 | 0.3365 | -858.0 | -690.6 | |
| 0.00 | 0.88 | 0.00 | 0.46 | 12.80 | 270.94 | 0.77 | 357.63 | 0.3189 | 811.0 | 620.3 | |
| 0.00 | 0.97 | 0.00 | 0.52 | 15.39 | 270.36 | 0.19 | 359.49 | 0.3613 | 584.0 | 385.7 | |
| 0.00 | 1.86 | 0.00 | 0.97 | 12.90 | 269.61 | -0.56 | 1.70 | 0.3203 | 984.0 | 816.6 | |
| 0.00 | 1.06 | 0.00 | 0.56 | 13.75 | 269.55 | -0.62 | 1.80 | 0.3346 | 820.0 | 695.4 | |
| 0.00 | 0.97 | 0.00 | 0.51 | 12.83 | 269.12 | -1.05 | 3.21 | 0.3197 | 893.0 | 734.7 | |
| 0.00 | 0.97 | 0.00 | 0.51 | 14.30 | 268.28 | -1.89 | 5.34 | 0.3449 | 704.0 | 505.1 | |
| 0.00 | 1.15 | 0.00 | 0.61 | 13.98 | 268.16 | -2.01 | 5.78 | 0.3399 | 527.0 | 334.1 | |
| 0.00 | 1.41 | 0.00 | 0.76 | 16.76 | 268.07 | -2.10 | 5.25 | 0.3851 | 804.0 | 637.2 | |
| 0.00 | 1.95 | 0.00 | 1.02 | 13.06 | 268.07 | -2.10 | 6.33 | 0.3249 | 1015.0 | 856.9 | |
| 0.00 | 1.33 | 0.00 | 0.70 | 13.92 | 267.82 | -2.35 | 6.77 | 0.3395 | 794.0 | 646.9 | |
| 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. | |