SDO HMI 2014-04-22 06:00:35 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 22.46 | 0.00 | 11.52 | -17.11 | 165.42 | 1.99 | 190.09 | 0.2413 | -687.1 | -575.9 | |
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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 | 0.59 | -5.55 | 177.14 | 13.72 | 267.12 | 0.2375 | 932.0 | 717.3 | |
| 0.00 | 1.15 | 0.00 | 0.58 | -11.69 | 173.25 | 9.82 | 234.89 | 0.2052 | -837.0 | -673.8 | |
| 0.00 | 3.29 | 0.00 | 1.66 | -12.29 | 171.36 | 7.94 | 226.65 | 0.1865 | -985.0 | -704.2 | |
| 0.00 | 1.69 | 0.00 | 0.87 | -20.56 | 167.94 | 4.52 | 195.39 | 0.2795 | -744.0 | -490.4 | |
| 0.00 | 1.95 | 0.00 | 1.01 | -20.38 | 167.71 | 4.29 | 194.82 | 0.2755 | -705.0 | -609.3 | |
| 0.00 | 1.42 | 0.00 | 0.74 | -23.50 | 167.54 | 4.12 | 191.73 | 0.3254 | -769.0 | -486.4 | |
| 0.00 | 1.51 | 0.00 | 0.81 | -27.49 | 167.17 | 3.74 | 188.61 | 0.3885 | -606.0 | -465.4 | |
| 0.00 | 1.24 | 0.00 | 0.62 | -9.42 | 162.75 | -0.68 | 171.37 | 0.0780 | -868.0 | -710.9 | |
| 0.00 | 0.80 | 0.00 | 0.40 | -8.54 | 162.66 | -0.77 | 167.88 | 0.0632 | -923.0 | -771.1 | |
| 0.00 | 1.69 | 0.00 | 0.86 | -19.54 | 162.12 | -1.30 | 175.14 | 0.2529 | -689.0 | -458.1 | |
| 0.00 | 1.33 | 0.00 | 0.68 | -17.85 | 159.92 | -3.50 | 165.36 | 0.2309 | -831.0 | -700.1 | |
| 0.00 | 1.15 | 0.00 | 0.58 | -10.10 | 159.50 | -3.93 | 142.80 | 0.1120 | -935.0 | -695.5 | |
| 0.00 | 3.02 | 0.00 | 1.58 | -23.35 | 158.14 | -5.28 | 164.98 | 0.3275 | -947.0 | -886.1 | |
| 0.00 | 1.07 | 0.00 | 0.54 | -14.02 | 156.97 | -6.45 | 145.24 | 0.1921 | -712.0 | -549.7 | |
| 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. | |