SDO HMI 2014-04-06 07:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 73.86 | 432.24 | 38.66 | 226.34 | 12.59 | 13.62 | -0.51 | 1.55 | 0.3246 | -1093.2 | -390.2 | |
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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 | 1.06 | 0.00 | 0.56 | 14.46 | 15.40 | 1.28 | 356.51 | 0.3557 | 783.0 | 596.4 | |
| 0.00 | 1.32 | 0.00 | 0.70 | 14.30 | 15.12 | 1.00 | 357.25 | 0.3528 | 701.0 | 513.9 | |
| 71.48 | 409.00 | 37.42 | 214.20 | 12.61 | 13.73 | -0.40 | 1.19 | 0.3247 | -1542.6 | -436.5 | |
| 1.32 | -3.00 | 0.69 | -3.00 | 13.16 | 13.61 | -0.52 | 1.52 | 0.3336 | -729.4 | 999999 | |
| 0.00 | 2.29 | 0.00 | 1.18 | 9.47 | 12.64 | -1.49 | 5.41 | 0.2732 | 950.0 | 698.3 | |
| 0.00 | 1.41 | 0.00 | 0.73 | 11.26 | 12.02 | -2.11 | 6.84 | 0.3042 | -815.0 | -674.9 | |
| 0.00 | 0.88 | 0.00 | 0.46 | 12.15 | 11.95 | -2.18 | 6.71 | 0.3189 | -650.0 | -475.6 | |
| 0.00 | 2.38 | 0.00 | 1.24 | 11.80 | 11.89 | -2.23 | 7.03 | 0.3133 | -784.0 | -681.4 | |
| 0.00 | 1.06 | 0.00 | 0.55 | 12.08 | 11.67 | -2.45 | 7.58 | 0.3185 | -586.0 | -386.6 | |
| 0.00 | 1.23 | 0.00 | 0.64 | 12.31 | 11.46 | -2.67 | 8.14 | 0.3226 | -648.0 | -485.5 | |
| 0.00 | 2.46 | 0.00 | 1.28 | 11.33 | 11.10 | -3.03 | 9.74 | 0.3075 | 775.0 | 722.5 | |
| 0.00 | 1.23 | 0.00 | 0.64 | 11.49 | 10.97 | -3.15 | 10.04 | 0.3105 | 694.0 | 600.5 | |
| 1.06 | 4.49 | 0.55 | 2.36 | 12.69 | 10.71 | -3.41 | 10.15 | 0.3309 | 1088.8 | 838.8 | |
| 0.00 | 1.32 | 0.00 | 0.69 | 11.93 | 10.57 | -3.56 | 11.02 | 0.3190 | 998.0 | 898.9 | |
| 0.00 | 2.11 | 0.00 | 1.11 | 13.05 | 9.60 | -4.53 | 13.11 | 0.3404 | 829.0 | 679.5 | |
| 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. | |