SDO HMI 2014-03-03 01:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 18.57 | 0.00 | 10.63 | -11.80 | 75.64 | -30.02 | 101.01 | 0.5006 | 55.9 | -164.8 | |
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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 | 0.95 | 0.00 | 0.50 | -8.60 | 85.11 | -20.55 | 95.19 | 0.3501 | -3.0 | -1.6 | |
| 0.00 | 2.42 | 0.00 | 1.32 | -13.39 | 81.18 | -24.49 | 106.32 | 0.4220 | 818.0 | 629.7 | |
| 0.00 | 1.12 | 0.00 | 0.61 | -7.77 | 81.46 | -24.21 | 92.82 | 0.4085 | 725.0 | 505.6 | |
| 0.00 | 0.78 | 0.00 | 0.44 | -11.37 | 75.68 | -29.98 | 100.23 | 0.4999 | 896.0 | 776.4 | |
| 0.00 | 1.04 | 0.00 | 0.59 | -11.15 | 75.60 | -30.06 | 99.79 | 0.5008 | 640.0 | 604.2 | |
| 0.00 | 0.86 | 0.00 | 0.49 | -11.42 | 75.50 | -30.16 | 100.29 | 0.5026 | 655.0 | 480.7 | |
| 0.00 | 0.86 | 0.00 | 0.50 | -11.80 | 74.96 | -30.70 | 100.95 | 0.5111 | 640.0 | 482.0 | |
| 0.00 | 1.99 | 0.00 | 1.16 | -12.21 | 73.88 | -31.79 | 101.52 | 0.5276 | -786.0 | -663.9 | |
| 0.00 | 4.75 | 0.00 | 2.77 | -11.85 | 73.49 | -32.17 | 100.78 | 0.5326 | -802.0 | -737.8 | |
| 0.00 | 1.81 | 0.00 | 1.06 | -11.55 | 73.39 | -32.28 | 100.19 | 0.5337 | -777.0 | -577.2 | |
| 0.00 | 0.95 | 0.00 | 0.56 | -10.86 | 73.34 | -32.33 | 98.89 | 0.5337 | -663.0 | -524.2 | |
| 0.00 | 1.04 | 0.00 | 0.63 | -16.37 | 70.09 | -35.57 | 107.99 | 0.5891 | -672.0 | -555.4 | |
| 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. | |