SDO HMI 2014-04-03 14:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 18.27 | 60.00 | 12.00 | 39.46 | -8.25 | 8.47 | -41.41 | 95.28 | 0.6590 | 298.1 | 249.9 | |
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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 | 0.97 | 0.00 | 0.62 | -8.89 | 10.47 | -39.40 | 96.22 | 0.6332 | 260.0 | 246.0 | |
| 7.38 | 34.61 | 4.73 | 22.20 | -8.41 | 10.18 | -39.70 | 95.47 | 0.6371 | 963.7 | 442.3 | |
| 6.85 | -2.00 | 4.41 | -2.00 | -8.60 | 9.91 | -39.96 | 95.77 | 0.6406 | 861.4 | 999999 | |
| 0.00 | 1.93 | 0.00 | 1.25 | -8.86 | 9.64 | -40.23 | 96.16 | 0.6442 | 487.0 | 445.5 | |
| 0.00 | 3.60 | 0.00 | 2.33 | -8.58 | 9.56 | -40.32 | 95.73 | 0.6453 | 680.0 | 485.5 | |
| 0.00 | 4.04 | 0.00 | 2.63 | -8.61 | 9.16 | -40.72 | 95.78 | 0.6506 | 476.0 | 440.3 | |
| 0.00 | 1.23 | 0.00 | 0.81 | -8.14 | 8.45 | -41.42 | 95.05 | 0.6598 | 539.0 | 508.4 | |
| 0.00 | 1.14 | 0.00 | 0.75 | -8.70 | 8.30 | -41.58 | 95.91 | 0.6618 | 441.0 | 322.7 | |
| 0.00 | 0.70 | 0.00 | 0.50 | -6.21 | 4.21 | -45.67 | 92.42 | 0.7141 | -418.0 | -273.0 | |
| 4.04 | 6.41 | 2.86 | 4.54 | -7.52 | 3.96 | -45.92 | 94.27 | 0.7165 | -749.1 | -543.7 | |
| 0.00 | 0.97 | 0.00 | 0.69 | -7.35 | 3.72 | -46.16 | 94.04 | 0.7195 | -445.0 | -411.9 | |
| 0.00 | 1.67 | 0.00 | 1.19 | -7.15 | 3.52 | -46.35 | 93.78 | 0.7219 | -408.0 | -368.8 | |
| 0.00 | 1.32 | 0.00 | 0.94 | -7.13 | 3.22 | -46.66 | 93.76 | 0.7255 | -481.0 | -423.5 | |
| 0.00 | 1.41 | 0.00 | 1.01 | -6.97 | 3.11 | -46.77 | 93.54 | 0.7269 | -490.0 | -391.2 | |
| 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. | |