| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 72.17 | 315.23 | 55.37 | 239.21 | 19.48 | 192.36 | -46.91 | 65.40 | 0.7579 | -194.2 | -126.0 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2011-11-25 10:58:57 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 |
| 2.31 | 201.28 | 1.68 | 145.88 | 19.13 | 194.70 | -44.57 | 65.05 | 0.7336 | -725.2 | -363.2 | |
| 9.33 | -1.00 | 6.76 | -1.00 | 18.79 | 194.77 | -44.50 | 65.47 | 0.7317 | -950.6 | 999999 | |
| 22.00 | -1.00 | 15.97 | -1.00 | 18.35 | 194.48 | -44.79 | 66.15 | 0.7334 | -974.1 | 999999 | |
| 3.42 | 4.45 | 2.54 | 3.30 | 19.11 | 193.42 | -45.85 | 65.53 | 0.7473 | -612.6 | -389.4 | |
| 3.17 | 11.30 | 2.35 | 8.41 | 18.64 | 193.31 | -45.96 | 66.17 | 0.7469 | -546.2 | -447.7 | |
| 0.51 | -5.00 | 0.38 | -5.00 | 19.13 | 193.09 | -46.18 | 65.61 | 0.7508 | -432.2 | 999999 | |
| 4.37 | -5.00 | 3.26 | -5.00 | 18.85 | 193.10 | -46.17 | 65.97 | 0.7498 | -547.2 | 999999 | |
| 0.00 | 2.23 | 0.00 | 1.68 | 19.59 | 192.51 | -46.76 | 65.22 | 0.7583 | -316.0 | -334.0 | |
| 1.71 | 6.25 | 1.29 | 4.70 | 18.63 | 192.68 | -46.59 | 66.40 | 0.7536 | -506.0 | -214.1 | |
| 0.00 | 0.60 | 0.00 | 0.46 | 19.68 | 192.20 | -47.07 | 65.21 | 0.7617 | -351.0 | -302.6 | |
| 0.00 | 1.37 | 0.00 | 1.04 | 19.14 | 192.08 | -47.19 | 65.93 | 0.7614 | -357.0 | -200.9 | |
| 0.00 | 1.11 | 0.00 | 0.86 | 19.95 | 191.62 | -47.65 | 65.06 | 0.7684 | -203.0 | -195.3 | |
| 0.00 | 0.68 | 0.00 | 0.52 | 18.46 | 192.05 | -47.22 | 66.81 | 0.7597 | -300.0 | -256.0 | |
| 2.05 | 3.60 | 1.60 | 2.80 | 20.35 | 191.18 | -48.09 | 64.70 | 0.7741 | -425.5 | -301.3 | |
| 0.00 | 0.77 | 0.00 | 0.60 | 20.66 | 191.05 | -48.22 | 64.36 | 0.7763 | -383.0 | -317.4 | |
| 0.00 | 2.74 | 0.00 | 2.12 | 19.60 | 191.39 | -47.88 | 65.57 | 0.7698 | 479.0 | 444.7 | |
| 0.00 | 0.77 | 0.00 | 0.60 | 19.75 | 191.33 | -47.94 | 65.40 | 0.7709 | 473.0 | 482.1 | |
| 0.00 | 0.51 | 0.00 | 0.40 | 20.53 | 190.72 | -48.55 | 64.63 | 0.7792 | -203.0 | -157.2 | |
| 1.63 | 7.71 | 1.27 | 6.01 | 19.71 | 190.92 | -48.35 | 65.58 | 0.7749 | 612.5 | 508.9 | |
| 2.23 | -19.00 | 1.74 | -19.00 | 19.56 | 190.84 | -48.43 | 65.80 | 0.7753 | 714.9 | 999999 | |
| 1.11 | 1.63 | 0.88 | 1.28 | 20.05 | 190.49 | -48.78 | 65.29 | 0.7801 | 604.0 | 695.7 | |
| 0.00 | 1.11 | 0.00 | 0.87 | 19.86 | 190.57 | -48.70 | 65.50 | 0.7788 | 280.0 | 290.2 | |
| 1.63 | 2.40 | 1.29 | 1.90 | 19.92 | 190.16 | -49.11 | 65.56 | 0.7830 | 460.2 | 458.0 | |
| 2.91 | 5.99 | 2.33 | 4.79 | 20.38 | 189.91 | -49.36 | 65.06 | 0.7867 | 731.9 | 571.7 | |
| 0.00 | 5.05 | 0.00 | 4.14 | 21.56 | 189.03 | -50.24 | 63.88 | 0.7985 | 761.0 | 576.4 | |
| 0.00 | 5.65 | 0.00 | 4.82 | 21.56 | 187.09 | -52.18 | 64.46 | 0.8165 | 799.0 | 596.8 | |
| 10.62 | 42.64 | 9.24 | 37.22 | 22.27 | 186.40 | -52.87 | 63.80 | 0.8245 | 849.3 | 519.8 | |
| 2.14 | -27.00 | 1.88 | -27.00 | 22.49 | 186.01 | -53.26 | 63.66 | 0.8284 | 678.7 | 999999 | |
| 1.03 | 1.71 | 0.91 | 1.52 | 22.77 | 185.64 | -53.63 | 63.43 | 0.8324 | 353.2 | 356.1 | |
| 0.00 | 0.94 | 0.00 | 0.84 | 22.66 | 185.37 | -53.90 | 63.63 | 0.8344 | 294.0 | 176.6 | |
| 0.00 | 0.77 | 0.00 | 0.68 | 22.16 | 185.65 | -53.62 | 64.14 | 0.8308 | 372.0 | 308.0 | |
| 0.00 | 1.97 | 0.00 | 1.77 | 22.18 | 184.93 | -54.34 | 64.31 | 0.8371 | 250.0 | 290.5 | |
| 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. | |