SDO HMI 2014-04-04 09:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.97 | 17.15 | 0.50 | 9.03 | 5.90 | 25.09 | -14.33 | 48.32 | 0.3293 | -202.9 | -40.4 | |
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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 | 1.67 | 0.00 | 0.86 | 9.55 | 34.99 | -4.43 | 15.55 | 0.2854 | 830.0 | 646.5 | |
| 0.00 | 0.79 | 0.00 | 0.41 | 6.23 | 29.61 | -9.81 | 38.06 | 0.2760 | -896.0 | -744.4 | |
| 0.97 | 2.99 | 0.50 | 1.53 | 3.56 | 28.73 | -10.69 | 47.39 | 0.2527 | -1199.6 | -974.2 | |
| 0.00 | 1.67 | 0.00 | 0.86 | 4.06 | 28.45 | -10.97 | 46.73 | 0.2618 | -975.0 | -740.7 | |
| 0.00 | 1.23 | 0.00 | 0.63 | 2.99 | 27.08 | -12.34 | 53.16 | 0.2678 | -938.0 | -745.7 | |
| 0.00 | 1.32 | 0.00 | 0.68 | 3.37 | 26.74 | -12.68 | 52.83 | 0.2762 | -803.0 | -642.6 | |
| 0.00 | 0.88 | 0.00 | 0.45 | 1.70 | 25.52 | -13.90 | 60.32 | 0.2776 | -757.0 | -676.9 | |
| 0.00 | 2.55 | 0.00 | 1.38 | 9.13 | 21.21 | -18.21 | 49.72 | 0.4062 | 807.0 | 567.3 | |
| 0.00 | 1.32 | 0.00 | 0.73 | 8.65 | 18.43 | -20.99 | 54.60 | 0.4363 | 809.0 | 611.9 | |
| 0.00 | 0.62 | 0.00 | 0.34 | 6.89 | 18.46 | -20.96 | 58.01 | 0.4206 | 621.0 | 499.4 | |
| 0.00 | 2.11 | 0.00 | 1.16 | 6.38 | 17.41 | -22.01 | 60.30 | 0.4306 | 768.0 | 746.8 | |
| 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. | |