SDO HMI 2014-05-19 22:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 38.85 | 215.49 | 24.76 | 137.01 | -24.71 | 190.40 | 32.72 | 231.57 | 0.6290 | 636.1 | 321.9 | |
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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 |
| 37.14 | 197.76 | 23.67 | 125.99 | -24.51 | 190.73 | 33.05 | 232.12 | 0.6309 | 1095.8 | 375.1 | |
| 1.71 | -1.00 | 1.09 | -1.00 | -25.00 | 190.68 | 32.99 | 231.40 | 0.6338 | 738.8 | 999999 | |
| 0.00 | 2.25 | 0.00 | 1.45 | -26.33 | 190.69 | 33.01 | 229.62 | 0.6432 | 687.0 | 416.1 | |
| 0.00 | 0.54 | 0.00 | 0.34 | -22.86 | 189.64 | 31.96 | 233.64 | 0.6078 | 662.0 | 640.2 | |
| 0.00 | 1.89 | 0.00 | 1.22 | -26.57 | 190.49 | 32.80 | 229.16 | 0.6427 | 695.0 | 585.9 | |
| 0.00 | 1.08 | 0.00 | 0.69 | -25.57 | 190.17 | 32.49 | 230.25 | 0.6324 | 467.0 | 260.2 | |
| 0.00 | 1.08 | 0.00 | 0.66 | -25.84 | 186.29 | 28.61 | 226.71 | 0.5943 | -726.0 | -581.2 | |
| 0.00 | 2.07 | 0.00 | 1.27 | -26.38 | 185.86 | 28.18 | 225.58 | 0.5944 | -609.0 | -587.7 | |
| 0.00 | 0.99 | 0.00 | 0.61 | -26.68 | 185.75 | 28.06 | 225.08 | 0.5959 | -533.0 | -525.4 | |
| 0.00 | 1.44 | 0.00 | 0.89 | -27.02 | 185.68 | 28.00 | 224.57 | 0.5982 | -611.0 | -428.6 | |
| 0.00 | 0.81 | 0.00 | 0.50 | -27.36 | 185.35 | 27.67 | 223.81 | 0.5979 | -670.0 | -515.4 | |
| 0.00 | 0.90 | 0.00 | 0.55 | -27.50 | 185.04 | 27.36 | 223.34 | 0.5961 | -652.0 | -609.9 | |
| 0.00 | 0.99 | 0.00 | 0.61 | -28.61 | 185.00 | 27.32 | 221.87 | 0.6058 | -481.0 | -432.4 | |
| 0.00 | 1.62 | 0.00 | 1.00 | -28.42 | 184.52 | 26.83 | 221.66 | 0.5995 | -407.0 | -395.6 | |
| 0.00 | 2.07 | 0.00 | 1.23 | -27.02 | 180.92 | 23.24 | 219.70 | 0.5523 | -545.0 | -374.0 | |
| 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. | |