SDO HMI 2014-04-03 05:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 21.53 | 0.00 | 12.28 | 4.21 | 27.09 | -27.71 | 69.70 | 0.4962 | -698.8 | -619.3 | |
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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 | 1.67 | 0.00 | 0.94 | 3.89 | 28.14 | -26.67 | 69.51 | 0.4800 | -927.0 | -758.0 | |
| 0.00 | 1.32 | 0.00 | 0.75 | 4.41 | 28.09 | -26.72 | 68.54 | 0.4837 | -755.0 | -569.9 | |
| 0.00 | 0.79 | 0.00 | 0.44 | 2.34 | 28.08 | -26.73 | 72.62 | 0.4728 | -726.0 | -628.3 | |
| 0.00 | 1.58 | 0.00 | 0.89 | 3.78 | 27.87 | -26.93 | 69.92 | 0.4832 | -870.0 | -725.3 | |
| 0.00 | 1.76 | 0.00 | 1.00 | 4.06 | 27.76 | -27.04 | 69.46 | 0.4863 | -653.0 | -547.3 | |
| 0.00 | 1.58 | 0.00 | 0.89 | 3.64 | 27.74 | -27.06 | 70.29 | 0.4843 | -980.0 | -768.2 | |
| 0.00 | 1.85 | 0.00 | 1.05 | 3.89 | 27.60 | -27.21 | 69.91 | 0.4877 | -902.0 | -716.8 | |
| 0.00 | 1.14 | 0.00 | 0.65 | 4.11 | 27.39 | -27.42 | 69.64 | 0.4919 | -596.0 | -562.8 | |
| 0.00 | 1.14 | 0.00 | 0.65 | 3.51 | 27.37 | -27.43 | 70.81 | 0.4889 | -622.0 | -525.9 | |
| 0.00 | 3.78 | 0.00 | 2.15 | 3.87 | 27.33 | -27.48 | 70.14 | 0.4915 | -1000.0 | -801.3 | |
| 0.00 | 2.81 | 0.00 | 1.60 | 4.01 | 27.08 | -27.72 | 70.05 | 0.4956 | -653.0 | -570.9 | |
| 0.00 | 1.14 | 0.00 | 0.65 | 5.51 | 27.02 | -27.78 | 67.30 | 0.5050 | -625.0 | -522.4 | |
| 0.00 | 0.97 | 0.00 | 0.62 | 9.13 | 18.31 | -36.49 | 67.21 | 0.6392 | 224.0 | 198.7 | |
| 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. | |