| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 111.84 | 410.91 | 79.16 | 285.22 | 19.45 | 192.22 | -41.54 | 63.39 | 0.7003 | -124.4 | -192.4 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2011-11-25 20:58:57 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 | 0.86 | 0.00 | 0.54 | 17.83 | 197.90 | -35.86 | 62.97 | 0.6284 | -652.0 | -566.4 | |
| 2.14 | 215.55 | 1.43 | 143.37 | 19.08 | 194.74 | -39.02 | 62.76 | 0.6716 | -863.3 | -460.7 | |
| 13.61 | -2.00 | 9.06 | -2.00 | 18.71 | 194.68 | -39.08 | 63.32 | 0.6706 | -1148.5 | 999999 | |
| 19.85 | -2.00 | 13.22 | -2.00 | 18.21 | 194.50 | -39.26 | 64.11 | 0.6706 | -1083.2 | 999999 | |
| 0.00 | 0.26 | 0.00 | 0.17 | 15.54 | 194.96 | -38.80 | 67.76 | 0.6546 | -655.0 | -556.0 | |
| 2.22 | 76.93 | 1.51 | 52.74 | 19.19 | 193.57 | -40.19 | 63.16 | 0.6854 | -664.2 | -282.0 | |
| 11.04 | -6.00 | 7.49 | -6.00 | 18.81 | 193.39 | -40.37 | 63.76 | 0.6859 | -882.3 | 999999 | |
| 6.08 | -6.00 | 4.16 | -6.00 | 19.30 | 192.96 | -40.81 | 63.28 | 0.6929 | -682.8 | 999999 | |
| 2.74 | -6.00 | 1.87 | -6.00 | 18.68 | 193.02 | -40.74 | 64.11 | 0.6896 | -639.2 | 999999 | |
| 6.16 | -6.00 | 4.25 | -6.00 | 19.70 | 192.67 | -41.10 | 62.86 | 0.6978 | -640.1 | 999999 | |
| 1.28 | -6.00 | 0.88 | -6.00 | 18.93 | 192.90 | -40.86 | 63.82 | 0.6919 | -492.5 | 999999 | |
| 0.00 | 1.37 | 0.00 | 0.97 | 20.24 | 191.18 | -42.59 | 62.79 | 0.7163 | -449.0 | -194.2 | |
| 0.00 | 2.65 | 0.00 | 1.88 | 20.14 | 190.91 | -42.85 | 63.03 | 0.7188 | 620.0 | 561.5 | |
| 0.00 | 4.71 | 0.00 | 3.32 | 19.27 | 191.03 | -42.73 | 64.14 | 0.7142 | 762.0 | 566.1 | |
| 0.00 | 1.20 | 0.00 | 0.86 | 20.51 | 190.39 | -43.37 | 62.76 | 0.7258 | -277.0 | -213.4 | |
| 1.97 | 14.55 | 1.40 | 10.37 | 19.63 | 190.65 | -43.11 | 63.80 | 0.7198 | 757.4 | 503.5 | |
| 2.48 | -16.00 | 1.78 | -16.00 | 19.78 | 190.29 | -43.47 | 63.75 | 0.7242 | 763.6 | 999999 | |
| 1.20 | 28.15 | 0.86 | 20.44 | 20.28 | 190.08 | -43.69 | 63.18 | 0.7283 | 832.6 | 561.4 | |
| 1.28 | 2.22 | 0.92 | 1.60 | 19.87 | 189.91 | -43.85 | 63.78 | 0.7286 | 571.5 | 466.0 | |
| 14.89 | -18.00 | 10.83 | -18.00 | 20.30 | 189.50 | -44.27 | 63.38 | 0.7346 | 767.5 | 999999 | |
| 0.00 | 0.51 | 0.00 | 0.38 | 21.52 | 189.04 | -44.73 | 61.99 | 0.7439 | 709.0 | 654.3 | |
| 0.00 | 0.51 | 0.00 | 0.38 | 21.64 | 188.67 | -45.09 | 61.98 | 0.7480 | 543.0 | 571.7 | |
| 0.00 | 0.86 | 0.00 | 0.65 | 22.78 | 188.16 | -45.61 | 60.75 | 0.7574 | 605.0 | 534.4 | |
| 0.00 | 0.51 | 0.00 | 0.36 | 16.65 | 189.86 | -43.90 | 68.10 | 0.7184 | -396.0 | -391.3 | |
| 2.74 | 3.77 | 2.12 | 2.91 | 21.95 | 186.60 | -47.16 | 62.37 | 0.7700 | 817.9 | 712.5 | |
| 17.54 | 44.24 | 13.76 | 34.80 | 22.35 | 185.95 | -47.81 | 62.10 | 0.7777 | 791.2 | 479.5 | |
| 3.25 | 6.50 | 2.53 | 5.04 | 21.75 | 186.22 | -47.54 | 62.75 | 0.7731 | 629.1 | 537.5 | |
| 1.37 | -26.00 | 1.09 | -26.00 | 22.88 | 185.51 | -48.25 | 61.60 | 0.7837 | 520.7 | 999999 | |
| 0.00 | 1.03 | 0.00 | 0.82 | 23.16 | 185.03 | -48.73 | 61.43 | 0.7891 | 290.0 | 214.9 | |
| 0.00 | 1.88 | 0.00 | 1.49 | 21.99 | 185.30 | -48.46 | 62.77 | 0.7829 | 503.0 | 467.0 | |
| 0.00 | 1.37 | 0.00 | 1.10 | 22.68 | 184.92 | -48.84 | 62.05 | 0.7886 | 373.0 | 265.1 | |
| 0.00 | 1.28 | 0.00 | 1.03 | 22.46 | 184.79 | -48.97 | 62.37 | 0.7892 | 439.0 | 329.1 | |
| 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. | |