SDO HMI 2014-03-10 13:00:29 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 17.78 | 0.00 | 8.90 | -11.27 | 13.71 | 6.84 | 233.67 | 0.1454 | 369.2 | 326.7 | |
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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 | 1.39 | 0.00 | 0.70 | -9.25 | 18.44 | 11.57 | 259.13 | 0.2025 | 805.0 | 690.6 | |
| 0.00 | 1.13 | 0.00 | 0.57 | -10.76 | 16.43 | 9.56 | 248.75 | 0.1758 | 782.0 | 714.3 | |
| 0.00 | 1.99 | 0.00 | 1.00 | -10.83 | 15.85 | 8.97 | 247.18 | 0.1670 | 971.0 | 795.0 | |
| 0.00 | 1.21 | 0.00 | 0.61 | -10.80 | 15.63 | 8.76 | 246.86 | 0.1634 | 1042.0 | 928.5 | |
| 0.00 | 1.13 | 0.00 | 0.57 | -11.22 | 15.49 | 8.62 | 244.15 | 0.1641 | 929.0 | 686.1 | |
| 0.00 | 1.13 | 0.00 | 0.57 | -11.37 | 15.46 | 8.59 | 243.26 | 0.1648 | 916.0 | 702.0 | |
| 0.00 | 1.13 | 0.00 | 0.57 | -10.75 | 15.42 | 8.54 | 246.69 | 0.1597 | 983.0 | 782.5 | |
| 0.00 | 1.82 | 0.00 | 0.91 | -11.00 | 14.60 | 7.72 | 243.07 | 0.1487 | 1016.0 | 825.3 | |
| 0.00 | 1.39 | 0.00 | 0.69 | -10.74 | 13.89 | 7.01 | 242.55 | 0.1358 | 884.0 | 775.9 | |
| 0.00 | 1.99 | 0.00 | 0.99 | -12.12 | 10.43 | 3.56 | 215.35 | 0.1055 | -904.0 | -712.3 | |
| 0.00 | 1.21 | 0.00 | 0.60 | -13.32 | 8.98 | 2.11 | 198.59 | 0.1128 | -789.0 | -623.6 | |
| 0.00 | 1.13 | 0.00 | 0.56 | -12.31 | 8.82 | 1.95 | 200.52 | 0.0952 | -955.0 | -755.4 | |
| 0.00 | 1.13 | 0.00 | 0.56 | -12.49 | 7.94 | 1.06 | 191.18 | 0.0940 | -881.0 | -631.2 | |
| 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. | |