SDO HMI 2014-07-10 05:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 10.63 | 0.00 | 6.49 | -20.91 | 221.77 | 22.91 | 219.04 | 0.5772 | -331.8 | -280.5 | |
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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 | 0.82 | 0.00 | 0.59 | -16.61 | 241.53 | 42.67 | 242.90 | 0.7318 | 509.0 | 385.6 | |
| 0.00 | 1.27 | 0.00 | 0.86 | -14.28 | 237.74 | 38.88 | 244.01 | 0.6791 | 632.0 | 529.2 | |
| 0.00 | 1.18 | 0.00 | 0.75 | -17.66 | 232.07 | 33.21 | 235.70 | 0.6340 | -692.0 | -577.2 | |
| 0.00 | 0.36 | 0.00 | 0.23 | -17.03 | 231.00 | 32.14 | 235.74 | 0.6176 | -484.0 | -482.5 | |
| 0.00 | 1.36 | 0.00 | 0.79 | -21.59 | 216.87 | 18.01 | 213.99 | 0.5163 | -670.0 | -583.2 | |
| 0.00 | 0.73 | 0.00 | 0.42 | -22.05 | 216.34 | 17.48 | 212.70 | 0.5175 | -692.0 | -630.1 | |
| 0.00 | 1.09 | 0.00 | 0.63 | -22.14 | 215.67 | 16.81 | 211.60 | 0.5132 | -126.0 | -247.5 | |
| 0.00 | 0.64 | 0.00 | 0.36 | -19.66 | 214.51 | 15.65 | 212.65 | 0.4728 | 3.0 | -23.3 | |
| 0.00 | 1.00 | 0.00 | 0.58 | -25.23 | 211.92 | 13.06 | 202.89 | 0.5277 | -708.0 | -605.5 | |
| 0.00 | 1.27 | 0.00 | 0.74 | -25.74 | 211.08 | 12.22 | 201.17 | 0.5299 | -679.0 | -482.4 | |
| 0.00 | 0.91 | 0.00 | 0.54 | -28.65 | 205.09 | 6.23 | 190.07 | 0.5473 | -743.0 | -664.1 | |
| 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. | |