SDO HMI 2014-04-19 21:00:34 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 20.02 | 0.00 | 10.24 | -14.60 | 201.14 | 6.34 | 216.12 | 0.2446 | -313.5 | -334.9 | |
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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 | 1.60 | 0.00 | 0.83 | -13.40 | 209.58 | 14.78 | 239.74 | 0.2886 | 662.0 | 576.3 | |
| 0.00 | 1.06 | 0.00 | 0.55 | -13.34 | 209.42 | 14.62 | 239.66 | 0.2858 | 769.0 | 607.8 | |
| 0.00 | 1.24 | 0.00 | 0.63 | -12.16 | 207.35 | 12.56 | 240.00 | 0.2465 | -729.0 | -620.4 | |
| 0.00 | 1.24 | 0.00 | 0.64 | -15.03 | 207.38 | 12.58 | 230.72 | 0.2730 | 711.0 | 565.6 | |
| 0.00 | 2.22 | 0.00 | 1.12 | -3.77 | 205.81 | 11.01 | 277.15 | 0.1930 | -714.0 | -579.2 | |
| 0.00 | 1.33 | 0.00 | 0.67 | -3.43 | 204.79 | 10.00 | 279.89 | 0.1767 | 807.0 | 599.7 | |
| 0.00 | 1.77 | 0.00 | 0.90 | -15.61 | 203.37 | 8.58 | 218.45 | 0.2320 | -853.0 | -701.9 | |
| 0.00 | 1.15 | 0.00 | 0.59 | -19.34 | 203.29 | 8.49 | 209.68 | 0.2827 | -825.0 | -702.2 | |
| 0.00 | 1.33 | 0.00 | 0.68 | -16.44 | 202.33 | 7.53 | 212.81 | 0.2331 | -781.0 | -622.7 | |
| 0.00 | 1.15 | 0.00 | 0.60 | -24.31 | 194.14 | -0.66 | 178.17 | 0.3284 | -855.0 | -666.2 | |
| 0.00 | 2.92 | 0.00 | 1.49 | -18.73 | 193.19 | -1.61 | 173.49 | 0.2358 | -667.0 | -709.4 | |
| 0.00 | 1.15 | 0.00 | 0.59 | -18.14 | 192.75 | -2.05 | 171.35 | 0.2268 | -845.0 | -679.4 | |
| 0.00 | 1.86 | 0.00 | 0.95 | -18.34 | 190.36 | -4.43 | 162.08 | 0.2395 | -756.0 | -662.5 | |
| 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. | |