| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 32.15 | 180.52 | 25.62 | 145.85 | -20.01 | 20.20 | -49.61 | 115.02 | 0.7917 | 223.6 | 254.0 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2011-05-31 12:59:10 UT
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 |
| 4.61 | 12.46 | 3.44 | 9.31 | -17.53 | 23.64 | -46.16 | 113.03 | 0.7497 | -672.0 | -586.6 | |
| 0.00 | 1.63 | 0.00 | 1.24 | -19.41 | 22.97 | -46.83 | 115.20 | 0.7625 | -573.0 | -528.8 | |
| 2.89 | -1.00 | 2.17 | -1.00 | -17.82 | 23.40 | -46.40 | 113.31 | 0.7530 | -601.9 | 999999 | |
| 0.00 | 0.81 | 0.00 | 0.62 | -19.38 | 22.75 | -47.06 | 115.08 | 0.7647 | -479.0 | -445.8 | |
| 0.00 | 0.63 | 0.00 | 0.49 | -19.22 | 22.38 | -47.42 | 114.75 | 0.7679 | -505.0 | -438.3 | |
| 0.00 | 1.17 | 0.00 | 0.91 | -19.31 | 22.10 | -47.70 | 114.77 | 0.7710 | -457.0 | -407.3 | |
| 0.00 | 0.99 | 0.00 | 0.76 | -18.76 | 22.26 | -47.54 | 114.14 | 0.7677 | -501.0 | -446.1 | |
| 0.00 | 0.45 | 0.00 | 0.34 | -17.71 | 22.55 | -47.25 | 112.90 | 0.7617 | -456.0 | -343.8 | |
| 3.70 | 13.46 | 2.89 | 10.52 | -18.57 | 21.52 | -48.28 | 113.65 | 0.7747 | -618.6 | -237.7 | |
| 0.00 | 3.52 | 0.00 | 2.79 | -18.91 | 20.85 | -48.95 | 113.87 | 0.7824 | 552.0 | 446.6 | |
| 0.00 | 1.17 | 0.00 | 0.93 | -18.69 | 20.74 | -49.06 | 113.56 | 0.7829 | 301.0 | 267.1 | |
| 17.52 | 142.07 | 14.28 | 116.13 | -20.35 | 19.85 | -49.96 | 115.33 | 0.7963 | 970.8 | 352.3 | |
| 3.43 | -12.00 | 2.84 | -12.00 | -20.67 | 19.14 | -50.66 | 115.49 | 0.8039 | 526.4 | 999999 | |
| 0.00 | 0.81 | 0.00 | 0.68 | -20.63 | 18.69 | -51.11 | 115.31 | 0.8080 | -258.0 | -219.3 | |
| 0.00 | 1.35 | 0.00 | 1.13 | -19.69 | 18.45 | -51.35 | 114.11 | 0.8078 | 387.0 | 248.3 | |
| Proj. U | - Projected umbra area in millionths of solar disc, negative values indicate | |
|
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. |
||
| Proj. WS | - Projected whole spot area in millionths of solar disc, negative values indicate | |
|
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. |
||
| 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. | |