SDO HMI 2014-04-15 00:00:34 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 60.38 | 394.94 | 32.63 | 213.39 | 11.80 | 274.99 | 15.82 | 318.01 | 0.4007 | -867.3 | -376.6 | |
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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 |
| 59.94 | 377.51 | 32.40 | 204.11 | 11.74 | 275.22 | 16.05 | 317.45 | 0.4020 | -1295.1 | -412.2 | |
| 0.00 | 1.15 | 0.00 | 0.63 | 14.96 | 274.54 | 15.37 | 323.69 | 0.4343 | -685.0 | -565.2 | |
| 0.00 | 1.33 | 0.00 | 0.70 | 9.97 | 273.57 | 14.40 | 317.36 | 0.3632 | -749.0 | -611.2 | |
| 0.00 | 1.06 | 0.00 | 0.57 | 13.91 | 272.07 | 12.90 | 326.88 | 0.3984 | -871.0 | -736.6 | |
| 0.00 | 1.15 | 0.00 | 0.60 | 9.18 | 271.78 | 12.61 | 319.62 | 0.3342 | -814.0 | -604.8 | |
| 0.00 | 1.24 | 0.00 | 0.66 | 13.14 | 270.29 | 11.12 | 329.60 | 0.3728 | 676.0 | 602.7 | |
| 0.00 | 0.88 | 0.00 | 0.47 | 13.08 | 270.13 | 10.96 | 329.87 | 0.3706 | 890.0 | 714.5 | |
| 0.00 | 1.33 | 0.00 | 0.71 | 13.48 | 269.80 | 10.63 | 331.17 | 0.3737 | 693.0 | 538.5 | |
| 0.00 | 1.86 | 0.00 | 0.99 | 13.07 | 269.75 | 10.58 | 330.72 | 0.3675 | 959.0 | 832.5 | |
| 0.00 | 1.33 | 0.00 | 0.71 | 14.59 | 269.13 | 9.96 | 334.07 | 0.3845 | 541.0 | 483.0 | |
| 0.00 | 0.44 | 0.00 | 0.24 | 14.46 | 269.06 | 9.89 | 334.08 | 0.3822 | 684.0 | 658.8 | |
| 0.00 | 3.27 | 0.00 | 1.75 | 14.78 | 268.88 | 9.72 | 334.84 | 0.3856 | 804.0 | 619.2 | |
| 0.44 | 2.39 | 0.23 | 1.25 | 11.88 | 266.09 | 6.93 | 338.55 | 0.3241 | 916.0 | 744.8 | |
| 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. | |