SDO HMI 2014-09-06 01:00:36 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 16.53 | 0.00 | 9.14 | 11.17 | 178.14 | 23.94 | 285.18 | 0.4127 | -174.9 | -30.6 | |
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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 | 0.27 | 0.00 | 0.16 | 7.01 | 188.60 | 34.40 | 271.80 | 0.5631 | -641.0 | -613.7 | |
| 0.00 | 1.52 | 0.00 | 0.91 | 10.95 | 188.70 | 34.50 | 278.82 | 0.5648 | -555.0 | -420.5 | |
| 0.00 | 1.34 | 0.00 | 0.80 | 12.68 | 187.86 | 33.66 | 282.03 | 0.5550 | -669.0 | -596.3 | |
| 0.00 | 1.61 | 0.00 | 0.95 | 10.88 | 187.46 | 33.26 | 278.82 | 0.5471 | -636.0 | -548.7 | |
| 0.00 | 0.45 | 0.00 | 0.26 | 11.13 | 187.49 | 33.29 | 279.26 | 0.5478 | -635.0 | -593.4 | |
| 0.00 | 1.16 | 0.00 | 0.68 | 10.94 | 187.14 | 32.94 | 278.96 | 0.5425 | -740.0 | -620.1 | |
| 0.00 | 0.45 | 0.00 | 0.26 | 11.55 | 187.11 | 32.91 | 280.09 | 0.5427 | -530.0 | -523.0 | |
| 0.00 | 1.52 | 0.00 | 0.89 | 10.86 | 186.51 | 32.30 | 278.88 | 0.5333 | -813.0 | -696.3 | |
| 0.00 | 0.89 | 0.00 | 0.51 | 13.21 | 184.57 | 30.37 | 283.77 | 0.5087 | -539.0 | -361.4 | |
| 0.00 | 1.96 | 0.00 | 1.01 | 2.45 | 169.20 | 15.00 | 252.90 | 0.2718 | 894.0 | 735.1 | |
| 0.00 | 2.86 | 0.00 | 1.44 | 11.96 | 164.57 | 10.36 | 295.51 | 0.1959 | 1009.0 | 870.7 | |
| 0.00 | 0.98 | 0.00 | 0.50 | 17.40 | 162.24 | 8.04 | 323.05 | 0.2230 | 698.0 | 451.8 | |
| 0.00 | 1.52 | 0.00 | 0.77 | 16.04 | 161.26 | 7.06 | 322.46 | 0.1947 | 883.0 | 642.6 | |
| 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. | |