| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 33.14 | 184.34 | 26.65 | 150.86 | -20.04 | 20.15 | -50.20 | 114.86 | 0.7975 | 228.2 | 259.3 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2011-05-31 11:59:10 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 |
| 0.00 | 1.45 | 0.00 | 1.11 | -19.41 | 22.99 | -47.36 | 115.01 | 0.7678 | -597.0 | -517.1 | |
| 5.33 | 7.68 | 4.02 | 5.78 | -17.53 | 23.63 | -46.73 | 112.83 | 0.7556 | -652.8 | -691.6 | |
| 3.07 | 3.70 | 2.33 | 2.81 | -17.81 | 23.39 | -46.96 | 113.12 | 0.7589 | -527.8 | -361.7 | |
| 0.00 | 0.81 | 0.00 | 0.63 | -19.37 | 22.72 | -47.63 | 114.87 | 0.7705 | -507.0 | -427.0 | |
| 0.00 | 1.17 | 0.00 | 0.92 | -19.30 | 22.07 | -48.28 | 114.57 | 0.7768 | -427.0 | -400.2 | |
| 0.00 | 1.17 | 0.00 | 0.91 | -18.73 | 22.25 | -48.11 | 113.91 | 0.7734 | -474.0 | -398.2 | |
| 0.00 | 0.99 | 0.00 | 0.76 | -17.71 | 22.57 | -47.78 | 112.73 | 0.7671 | -402.0 | -280.5 | |
| 3.97 | 14.54 | 3.13 | 11.51 | -18.56 | 21.53 | -48.82 | 113.48 | 0.7801 | -589.2 | -125.0 | |
| 0.00 | 1.08 | 0.00 | 0.87 | -18.87 | 20.77 | -49.59 | 113.63 | 0.7886 | 541.0 | 435.5 | |
| 0.00 | 1.72 | 0.00 | 1.38 | -18.68 | 20.74 | -49.61 | 113.39 | 0.7883 | 327.0 | 225.9 | |
| 17.61 | 146.23 | 14.52 | 120.93 | -20.35 | 19.83 | -50.52 | 115.14 | 0.8016 | 956.9 | 342.0 | |
| 3.16 | -11.00 | 2.65 | -11.00 | -20.70 | 19.26 | -51.10 | 115.39 | 0.8080 | 592.3 | 999999 | |
| 0.00 | 1.45 | 0.00 | 1.25 | -22.02 | 18.01 | -52.34 | 116.59 | 0.8228 | 337.0 | 288.7 | |
| 0.00 | 1.45 | 0.00 | 1.22 | -19.66 | 18.49 | -51.87 | 113.92 | 0.8125 | 327.0 | 231.8 | |
| 0.00 | 0.90 | 0.00 | 0.78 | -19.75 | 17.60 | -52.76 | 113.78 | 0.8209 | -528.0 | -479.6 | |
| 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. | |