SDO HMI 2014-04-19 11:00:34 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 19.49 | 0.00 | 9.92 | -15.73 | 201.22 | 0.91 | 190.67 | 0.2152 | -370.2 | -358.9 | |
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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 | 1.15 | 0.00 | 0.58 | -13.44 | 209.90 | 9.59 | 228.45 | 0.2176 | 916.0 | 695.9 | |
| 0.00 | 0.89 | 0.00 | 0.45 | -13.27 | 208.64 | 8.33 | 225.12 | 0.2000 | 879.0 | 691.4 | |
| 0.00 | 1.06 | 0.00 | 0.54 | -14.86 | 208.39 | 8.08 | 218.98 | 0.2168 | 744.0 | 532.7 | |
| 0.00 | 1.77 | 0.00 | 0.90 | -13.67 | 208.03 | 7.72 | 221.55 | 0.1977 | 1030.0 | 932.0 | |
| 0.00 | 0.62 | 0.00 | 0.31 | -12.19 | 207.09 | 6.78 | 223.51 | 0.1683 | -824.0 | -634.9 | |
| 0.00 | 2.48 | 0.00 | 1.25 | -14.59 | 203.90 | 3.59 | 200.48 | 0.1742 | -1125.0 | -901.6 | |
| 0.00 | 1.24 | 0.00 | 0.62 | -13.31 | 203.42 | 3.11 | 200.62 | 0.1507 | -939.0 | -695.5 | |
| 0.00 | 1.42 | 0.00 | 0.72 | -15.78 | 203.01 | 2.70 | 193.94 | 0.1893 | -883.0 | -682.4 | |
| 0.00 | 2.30 | 0.00 | 1.16 | -15.60 | 202.11 | 1.80 | 189.53 | 0.1831 | -977.0 | -739.6 | |
| 0.00 | 2.13 | 0.00 | 1.07 | -14.69 | 201.29 | 0.98 | 185.76 | 0.1655 | -785.0 | -596.4 | |
| 0.00 | 0.62 | 0.00 | 0.33 | -23.47 | 194.69 | -5.62 | 164.00 | 0.3271 | -616.0 | -648.1 | |
| 0.00 | 0.98 | 0.00 | 0.50 | -18.35 | 190.50 | -9.81 | 144.65 | 0.2806 | -895.0 | -708.6 | |
| 0.00 | 1.77 | 0.00 | 0.93 | -19.86 | 188.13 | -12.18 | 142.01 | 0.3238 | -990.0 | -813.5 | |
| 0.00 | 1.06 | 0.00 | 0.56 | -19.91 | 187.60 | -12.71 | 140.96 | 0.3299 | -718.0 | -597.8 | |
| 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. | |