SDO HMI 2014-04-19 13:00:34 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.44 | 19.76 | 0.23 | 10.11 | -17.24 | 198.98 | -0.23 | 184.77 | 0.2436 | -499.3 | -485.4 | |
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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 |
| 0.44 | 1.68 | 0.23 | 0.86 | -13.42 | 209.84 | 10.63 | 231.32 | 0.2309 | 926.0 | 772.5 | |
| 0.00 | 1.24 | 0.00 | 0.63 | -13.31 | 208.61 | 9.40 | 228.32 | 0.2138 | 821.0 | 702.7 | |
| 0.00 | 0.89 | 0.00 | 0.45 | -12.18 | 207.20 | 7.99 | 228.18 | 0.1831 | -924.0 | -806.4 | |
| 0.00 | 2.39 | 0.00 | 1.21 | -14.58 | 203.96 | 4.75 | 206.25 | 0.1820 | -1007.0 | -816.8 | |
| 0.00 | 0.44 | 0.00 | 0.22 | -13.55 | 203.13 | 3.92 | 204.70 | 0.1598 | -295.0 | -468.2 | |
| 0.00 | 1.86 | 0.00 | 0.94 | -15.59 | 202.07 | 2.86 | 194.97 | 0.1869 | -903.0 | -729.2 | |
| 0.00 | 1.33 | 0.00 | 0.68 | -20.63 | 201.86 | 2.65 | 189.25 | 0.2701 | -904.0 | -692.8 | |
| 0.00 | 0.97 | 0.00 | 0.49 | -15.14 | 201.07 | 1.86 | 190.31 | 0.1755 | -868.0 | -704.0 | |
| 0.00 | 1.42 | 0.00 | 0.73 | -20.88 | 200.96 | 1.75 | 186.04 | 0.2723 | -910.0 | -668.2 | |
| 0.00 | 0.71 | 0.00 | 0.37 | -23.14 | 197.32 | -1.89 | 174.36 | 0.3102 | 48.0 | 135.0 | |
| 0.00 | 0.35 | 0.00 | 0.18 | -18.40 | 193.60 | -5.61 | 157.85 | 0.2472 | -641.0 | -598.2 | |
| 0.00 | 1.24 | 0.00 | 0.64 | -19.23 | 193.12 | -6.09 | 157.52 | 0.2632 | -716.0 | -573.4 | |
| 0.00 | 1.42 | 0.00 | 0.73 | -18.33 | 190.44 | -8.77 | 147.50 | 0.2707 | -837.0 | -637.3 | |
| 0.00 | 2.22 | 0.00 | 1.15 | -19.78 | 188.09 | -11.13 | 144.28 | 0.3124 | -761.0 | -686.0 | |
| 0.00 | 1.60 | 0.00 | 0.83 | -19.96 | 187.84 | -11.37 | 144.07 | 0.3171 | -847.0 | -727.4 | |
| 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. | |