SDO HMI 2014-05-14 05:00:37 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 42.73 | 250.02 | 28.92 | 170.62 | -23.81 | 193.93 | -39.26 | 122.53 | 0.6884 | 629.0 | 277.2 | |
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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 |
| 4.58 | 238.15 | 3.08 | 161.38 | -23.79 | 194.90 | -38.28 | 123.00 | 0.6783 | 1073.3 | 324.3 | |
| 37.25 | -1.00 | 25.23 | -1.00 | -23.68 | 194.31 | -38.88 | 122.53 | 0.6841 | 1003.1 | 999999 | |
| 0.90 | -1.00 | 0.61 | -1.00 | -23.46 | 193.66 | -39.53 | 121.90 | 0.6900 | 460.3 | 999999 | |
| 0.00 | 0.90 | 0.00 | 0.62 | -23.22 | 192.27 | -40.92 | 120.90 | 0.7038 | 328.0 | 309.2 | |
| 0.00 | 0.54 | 0.00 | 0.38 | -23.30 | 191.45 | -41.74 | 120.62 | 0.7128 | -307.0 | -354.8 | |
| 0.00 | 1.26 | 0.00 | 0.96 | -25.94 | 187.74 | -45.44 | 122.38 | 0.7610 | -610.0 | -446.9 | |
| 0.00 | 0.90 | 0.00 | 0.69 | -25.76 | 187.45 | -45.74 | 122.04 | 0.7632 | -685.0 | -597.0 | |
| 0.00 | 1.08 | 0.00 | 0.84 | -26.44 | 186.66 | -46.53 | 122.55 | 0.7732 | -567.0 | -534.8 | |
| 0.00 | 0.81 | 0.00 | 0.63 | -26.00 | 186.50 | -46.69 | 121.95 | 0.7731 | -595.0 | -532.0 | |
| 0.00 | 2.78 | 0.00 | 2.20 | -26.27 | 185.75 | -47.43 | 122.00 | 0.7810 | -416.0 | -364.5 | |
| 0.00 | 0.99 | 0.00 | 0.78 | -25.97 | 185.76 | -47.42 | 121.64 | 0.7799 | -455.0 | -467.4 | |
| 0.00 | 1.53 | 0.00 | 1.25 | -27.88 | 184.58 | -48.61 | 123.49 | 0.7974 | -691.0 | -576.8 | |
| 0.00 | 1.08 | 0.00 | 0.89 | -24.90 | 182.76 | -50.43 | 119.32 | 0.8041 | -419.0 | -270.9 | |
| 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. | |