SDO HMI 2014-06-04 11:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 16.73 | 35.62 | 9.37 | 19.98 | -19.73 | 332.31 | 20.24 | 224.17 | 0.4685 | 690.6 | 486.7 | |
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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 | 0.81 | 0.00 | 0.48 | -20.27 | 339.29 | 27.23 | 231.40 | 0.5512 | 482.0 | 382.6 | |
| 0.00 | 0.90 | 0.00 | 0.52 | -21.21 | 334.83 | 22.76 | 225.22 | 0.5100 | 696.0 | 653.8 | |
| 2.62 | 4.88 | 1.51 | 2.81 | -21.51 | 334.66 | 22.59 | 224.59 | 0.5112 | 860.1 | 649.4 | |
| 0.00 | 1.81 | 0.00 | 1.04 | -21.25 | 334.55 | 22.48 | 224.84 | 0.5074 | 868.0 | 782.1 | |
| 0.00 | 0.99 | 0.00 | 0.55 | -17.35 | 333.51 | 21.44 | 229.88 | 0.4582 | 892.0 | 715.5 | |
| 1.99 | 20.08 | 1.11 | 11.18 | -18.72 | 332.41 | 20.35 | 226.10 | 0.4589 | 907.1 | 748.8 | |
| 12.12 | -6.00 | 6.75 | -6.00 | -18.85 | 332.19 | 20.12 | 225.59 | 0.4577 | 1016.1 | 999999 | |
| 0.00 | 1.27 | 0.00 | 0.72 | -23.84 | 331.08 | 19.01 | 216.66 | 0.5009 | 743.0 | 611.3 | |
| 0.00 | 2.08 | 0.00 | 1.17 | -22.00 | 329.98 | 17.91 | 217.59 | 0.4694 | 729.0 | 550.5 | |
| 0.00 | 0.90 | 0.00 | 0.49 | -18.66 | 326.88 | 14.81 | 217.50 | 0.3996 | -686.0 | -539.7 | |
| 0.00 | 1.90 | 0.00 | 1.02 | -18.40 | 325.37 | 13.30 | 215.04 | 0.3819 | -892.0 | -709.2 | |
| 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. | |