SDO HMI 2014-03-05 10:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 12.97 | 0.00 | 8.90 | 10.60 | 113.94 | 39.54 | 294.55 | 0.6833 | -67.0 | -47.6 | |
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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 | 0.86 | 0.00 | 0.79 | 8.97 | 129.26 | 54.87 | 285.65 | 0.8411 | -229.0 | -280.1 | |
| 0.00 | 0.78 | 0.00 | 0.62 | 11.76 | 122.58 | 48.18 | 291.30 | 0.7854 | -584.0 | -430.7 | |
| 0.00 | 0.69 | 0.00 | 0.53 | 13.10 | 119.81 | 45.42 | 294.15 | 0.7626 | -581.0 | -472.4 | |
| 0.00 | 1.30 | 0.00 | 0.97 | 13.39 | 118.89 | 44.49 | 294.96 | 0.7543 | -605.0 | -489.8 | |
| 0.00 | 1.47 | 0.00 | 1.02 | 11.70 | 115.01 | 40.61 | 294.83 | 0.7046 | -577.0 | -446.9 | |
| 0.00 | 0.78 | 0.00 | 0.55 | 12.86 | 114.90 | 40.51 | 296.39 | 0.7092 | -622.0 | -505.9 | |
| 0.00 | 1.04 | 0.00 | 0.69 | 8.91 | 113.51 | 39.11 | 291.88 | 0.6739 | 473.0 | 356.9 | |
| 0.00 | 0.69 | 0.00 | 0.47 | 11.57 | 113.44 | 39.04 | 295.54 | 0.6863 | -555.0 | -446.4 | |
| 0.00 | 1.90 | 0.00 | 1.20 | 6.00 | 110.47 | 36.08 | 289.30 | 0.6228 | 690.0 | 437.2 | |
| 0.00 | 1.38 | 0.00 | 0.83 | 11.04 | 103.48 | 29.09 | 301.99 | 0.5648 | 650.0 | 441.0 | |
| 0.00 | 1.04 | 0.00 | 0.62 | 10.90 | 103.19 | 28.79 | 302.04 | 0.5601 | 583.0 | 462.8 | |
| 0.00 | 1.04 | 0.00 | 0.61 | 10.36 | 102.55 | 28.15 | 301.79 | 0.5482 | 553.0 | 501.5 | |
| 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. | |