SDO HMI 2014-04-22 12:00:35 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 17.14 | 0.00 | 8.78 | -18.83 | 161.49 | 1.35 | 185.01 | 0.2502 | -763.9 | -631.9 | |
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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 | 0.98 | 0.00 | 0.50 | -12.27 | 171.59 | 11.45 | 236.47 | 0.2337 | -828.0 | -680.9 | |
| 0.00 | 0.98 | 0.00 | 0.51 | -20.35 | 167.92 | 7.79 | 205.55 | 0.2958 | -712.0 | -579.7 | |
| 0.00 | 0.44 | 0.00 | 0.23 | -24.27 | 167.18 | 7.04 | 198.65 | 0.3508 | -317.0 | -395.8 | |
| 0.00 | 0.98 | 0.00 | 0.49 | -12.84 | 163.13 | 2.99 | 200.43 | 0.1466 | -808.0 | -515.6 | |
| 0.00 | 1.33 | 0.00 | 0.69 | -22.55 | 163.09 | 2.95 | 188.96 | 0.3069 | -771.0 | -576.1 | |
| 0.00 | 0.89 | 0.00 | 0.45 | -18.61 | 161.43 | 1.29 | 185.18 | 0.2376 | -781.0 | -702.0 | |
| 0.00 | 2.04 | 0.00 | 1.07 | -23.73 | 161.24 | 1.10 | 183.13 | 0.3232 | -831.0 | -662.5 | |
| 0.00 | 1.24 | 0.00 | 0.64 | -19.57 | 160.96 | 0.82 | 183.06 | 0.2533 | -884.0 | -637.5 | |
| 0.00 | 2.31 | 0.00 | 1.17 | -17.90 | 159.94 | -0.20 | 179.15 | 0.2245 | -971.0 | -755.8 | |
| 0.00 | 1.24 | 0.00 | 0.63 | -18.61 | 159.55 | -0.58 | 177.65 | 0.2368 | -769.0 | -618.5 | |
| 0.00 | 2.04 | 0.00 | 1.04 | -18.42 | 159.52 | -0.61 | 177.49 | 0.2336 | -853.0 | -685.5 | |
| 0.00 | 0.98 | 0.00 | 0.51 | -22.26 | 157.58 | -2.56 | 172.09 | 0.3012 | -698.0 | -479.2 | |
| 0.00 | 1.69 | 0.00 | 0.85 | -13.99 | 156.93 | -3.20 | 160.89 | 0.1665 | -708.0 | -595.8 | |
| 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. | |