SDO HMI 2014-05-17 04:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 46.82 | 300.38 | 24.94 | 160.29 | -24.07 | 191.81 | -2.24 | 174.64 | 0.3727 | 779.5 | 351.5 | |
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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 | 1.80 | 0.00 | 0.93 | -19.67 | 195.25 | 1.19 | 183.79 | 0.2982 | -973.0 | -738.5 | |
| 13.84 | 277.18 | 7.36 | 147.66 | -23.78 | 192.53 | -1.53 | 176.17 | 0.3663 | 1419.3 | 434.4 | |
| 10.96 | -2.00 | 5.83 | -2.00 | -23.75 | 192.17 | -1.89 | 175.25 | 0.3662 | 1443.0 | 999999 | |
| 20.58 | -2.00 | 10.98 | -2.00 | -24.11 | 192.09 | -1.96 | 175.16 | 0.3722 | 1164.7 | 999999 | |
| 1.44 | -2.00 | 0.77 | -2.00 | -23.95 | 191.66 | -2.39 | 174.06 | 0.3702 | 884.6 | 999999 | |
| 0.00 | 1.17 | 0.00 | 0.62 | -22.74 | 191.13 | -2.93 | 172.27 | 0.3517 | 809.0 | 644.3 | |
| 0.00 | 1.71 | 0.00 | 0.91 | -23.88 | 190.70 | -3.35 | 171.68 | 0.3710 | 871.0 | 582.6 | |
| 0.00 | 1.08 | 0.00 | 0.57 | -22.35 | 190.02 | -4.04 | 169.18 | 0.3483 | 672.0 | 445.6 | |
| 0.00 | 2.79 | 0.00 | 1.51 | -25.36 | 186.11 | -7.95 | 162.23 | 0.4111 | -810.0 | -607.5 | |
| 0.00 | 1.53 | 0.00 | 0.84 | -27.55 | 185.81 | -8.24 | 163.34 | 0.4452 | -775.0 | -608.2 | |
| 0.00 | 1.26 | 0.00 | 0.70 | -27.69 | 185.77 | -8.29 | 163.35 | 0.4474 | -838.0 | -706.6 | |
| 0.00 | 6.11 | 0.00 | 3.37 | -27.15 | 185.67 | -8.38 | 162.77 | 0.4399 | -1101.0 | -721.9 | |
| 0.00 | 3.68 | 0.00 | 2.04 | -27.65 | 185.25 | -8.80 | 162.36 | 0.4492 | -840.0 | -612.3 | |
| 0.00 | 1.35 | 0.00 | 0.75 | -28.12 | 185.04 | -9.02 | 162.32 | 0.4571 | -761.0 | -596.1 | |
| 0.00 | 0.72 | 0.00 | 0.39 | -24.29 | 180.39 | -13.67 | 150.01 | 0.4328 | -567.0 | -464.0 | |
| 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. | |