SDO HMI 2014-04-19 09:00:34 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 23.82 | 0.00 | 12.18 | -16.83 | 201.39 | -0.02 | 186.64 | 0.2291 | -299.6 | -197.4 | |
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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 |
| 0.00 | 1.33 | 0.00 | 0.67 | -13.40 | 209.93 | 8.53 | 225.33 | 0.2037 | 821.0 | 609.9 | |
| 0.00 | 2.84 | 0.00 | 1.43 | -13.35 | 208.65 | 7.24 | 220.92 | 0.1881 | 656.0 | 759.2 | |
| 0.00 | 1.06 | 0.00 | 0.54 | -13.91 | 208.20 | 6.79 | 217.25 | 0.1905 | 799.0 | 622.6 | |
| 0.00 | 1.68 | 0.00 | 0.85 | -13.76 | 208.00 | 6.60 | 216.97 | 0.1865 | 1042.0 | 794.7 | |
| 0.00 | 1.15 | 0.00 | 0.58 | -13.60 | 207.78 | 6.38 | 216.54 | 0.1822 | 764.0 | 594.3 | |
| 0.00 | 1.15 | 0.00 | 0.58 | -15.77 | 203.14 | 1.73 | 189.07 | 0.1855 | -793.0 | -650.5 | |
| 0.00 | 3.19 | 0.00 | 1.60 | -13.54 | 203.03 | 1.63 | 190.84 | 0.1473 | -638.0 | -678.1 | |
| 0.00 | 1.24 | 0.00 | 0.63 | -15.64 | 202.11 | 0.70 | 183.74 | 0.1815 | -999.0 | -760.0 | |
| 0.00 | 1.06 | 0.00 | 0.55 | -20.02 | 201.35 | -0.06 | 179.79 | 0.2560 | -721.0 | -584.5 | |
| 0.00 | 1.68 | 0.00 | 0.86 | -19.77 | 198.72 | -2.68 | 170.04 | 0.2556 | -859.0 | -607.4 | |
| 0.00 | 1.06 | 0.00 | 0.55 | -19.83 | 198.47 | -2.94 | 169.16 | 0.2574 | -779.0 | -648.1 | |
| 0.00 | 1.06 | 0.00 | 0.55 | -20.95 | 197.70 | -3.70 | 167.43 | 0.2784 | -853.0 | -617.4 | |
| 0.00 | 1.06 | 0.00 | 0.56 | -22.92 | 196.40 | -5.00 | 165.18 | 0.3155 | -744.0 | -613.1 | |
| 0.00 | 1.15 | 0.00 | 0.61 | -23.72 | 194.68 | -6.72 | 161.34 | 0.3364 | -749.0 | -584.8 | |
| 0.00 | 0.89 | 0.00 | 0.46 | -18.34 | 190.53 | -10.87 | 141.85 | 0.2911 | -838.0 | -648.2 | |
| 0.00 | 2.22 | 0.00 | 1.16 | -19.84 | 188.11 | -13.30 | 139.59 | 0.3352 | -903.0 | -676.4 | |
| 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. | |