SDO HMI 2011-11-19 08:58:57 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!)
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 28.69 | 215.26 | 16.09 | 121.21 | -18.77 | 337.71 | 18.26 | 219.28 | 0.4767 | 244.4 | 225.3 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2011-11-19 08:58:57 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 | 1.20 | 0.00 | 0.69 | -16.70 | 343.79 | 24.34 | 230.69 | 0.5123 | 661.0 | 534.3 | |
| 0.00 | 3.26 | 0.00 | 1.87 | -16.57 | 343.60 | 24.15 | 230.69 | 0.5089 | 730.0 | 605.8 | |
| 0.00 | 1.20 | 0.00 | 0.70 | -18.01 | 343.32 | 23.88 | 228.14 | 0.5190 | 653.0 | 551.6 | |
| 0.52 | 2.40 | 0.30 | 1.39 | -17.76 | 343.19 | 23.74 | 228.37 | 0.5150 | 959.2 | 742.5 | |
| 0.00 | 1.97 | 0.00 | 1.17 | -20.95 | 343.34 | 23.89 | 223.94 | 0.5473 | 561.0 | 481.7 | |
| 0.00 | 1.46 | 0.00 | 0.84 | -17.12 | 342.69 | 23.24 | 228.78 | 0.5035 | 916.0 | 738.7 | |
| 0.00 | 0.86 | 0.00 | 0.49 | -17.75 | 342.68 | 23.23 | 227.79 | 0.5092 | 524.0 | 516.6 | |
| 0.00 | 0.94 | 0.00 | 0.54 | -17.91 | 342.66 | 23.22 | 227.53 | 0.5106 | 609.0 | 554.0 | |
| 0.00 | 1.80 | 0.00 | 1.03 | -16.83 | 342.28 | 22.84 | 228.75 | 0.4961 | 949.0 | 727.4 | |
| 0.00 | 1.97 | 0.00 | 1.17 | -21.33 | 342.85 | 23.40 | 222.86 | 0.5461 | 547.0 | 519.5 | |
| 1.29 | 6.01 | 0.73 | 3.43 | -17.36 | 342.02 | 22.57 | 227.60 | 0.4981 | 845.9 | 687.6 | |
| 0.00 | 0.94 | 0.00 | 0.54 | -16.98 | 341.80 | 22.35 | 227.93 | 0.4920 | -342.0 | -177.1 | |
| 0.00 | 2.49 | 0.00 | 1.41 | -16.66 | 341.73 | 22.28 | 228.34 | 0.4882 | 964.0 | 741.4 | |
| 0.00 | 1.46 | 0.00 | 0.83 | -17.48 | 341.80 | 22.35 | 227.14 | 0.4969 | 738.0 | 658.8 | |
| 0.00 | 6.61 | 0.00 | 3.89 | -21.32 | 342.33 | 22.88 | 222.25 | 0.5408 | 945.0 | 716.4 | |
| 0.00 | 1.03 | 0.00 | 0.59 | -17.29 | 341.74 | 22.29 | 227.36 | 0.4944 | 928.0 | 802.4 | |
| 0.00 | 0.77 | 0.00 | 0.45 | -21.25 | 342.07 | 22.63 | 222.04 | 0.5376 | 782.0 | 642.4 | |
| 0.00 | 2.23 | 0.00 | 1.29 | -19.70 | 341.80 | 22.35 | 223.84 | 0.5190 | 728.0 | 638.1 | |
| 0.00 | 1.72 | 0.00 | 0.97 | -16.62 | 341.22 | 21.77 | 227.77 | 0.4820 | 752.0 | 606.9 | |
| 0.00 | 1.80 | 0.00 | 1.02 | -17.56 | 340.83 | 21.39 | 225.80 | 0.4870 | 757.0 | 528.7 | |
| 0.00 | 2.49 | 0.00 | 1.42 | -18.76 | 340.79 | 21.34 | 223.92 | 0.4988 | -536.0 | -350.8 | |
| 2.75 | 110.56 | 1.55 | 62.11 | -17.36 | 340.34 | 20.90 | 225.46 | 0.4796 | 918.4 | 488.5 | |
| 0.00 | 1.37 | 0.00 | 0.77 | -16.04 | 340.19 | 20.75 | 227.37 | 0.4646 | 878.0 | 731.2 | |
| 0.00 | 0.60 | 0.00 | 0.34 | -18.94 | 340.27 | 20.83 | 222.98 | 0.4953 | -662.0 | -507.0 | |
| 20.09 | -22.00 | 11.28 | -22.00 | -17.35 | 339.78 | 20.33 | 224.71 | 0.4734 | 1202.8 | 999999 | |
| 0.00 | 1.20 | 0.00 | 0.67 | -15.78 | 339.21 | 19.76 | 226.47 | 0.4508 | 677.0 | 473.1 | |
| 0.00 | 0.94 | 0.00 | 0.52 | -15.62 | 338.93 | 19.49 | 226.34 | 0.4460 | -759.0 | -556.1 | |
| 0.00 | 1.46 | 0.00 | 0.80 | -14.43 | 338.17 | 18.73 | 227.30 | 0.4249 | 322.0 | 413.9 | |
| 1.46 | 8.33 | 0.80 | 4.58 | -16.75 | 337.09 | 17.64 | 221.71 | 0.4381 | -855.7 | -629.9 | |
| 0.00 | 1.03 | 0.00 | 0.55 | -12.80 | 336.35 | 16.90 | 227.47 | 0.3863 | 829.0 | 583.2 | |
| 0.00 | 1.72 | 0.00 | 0.95 | -19.67 | 335.23 | 15.78 | 214.42 | 0.4550 | 943.0 | 723.7 | |
| 0.00 | 1.46 | 0.00 | 0.81 | -20.04 | 333.76 | 14.32 | 211.44 | 0.4473 | 891.0 | 649.2 | |
| 0.00 | 0.86 | 0.00 | 0.47 | -20.72 | 331.19 | 11.75 | 205.95 | 0.4371 | -790.0 | -684.2 | |
| 0.00 | 4.03 | 0.00 | 2.21 | -21.28 | 328.72 | 9.27 | 200.54 | 0.4297 | -864.0 | -662.5 | |
| 0.00 | 2.23 | 0.00 | 1.24 | -23.30 | 328.00 | 8.56 | 197.53 | 0.4557 | -879.0 | -654.3 | |
| 0.00 | 4.12 | 0.00 | 2.30 | -23.83 | 328.01 | 8.56 | 197.16 | 0.4635 | -597.0 | -654.9 | |
| 0.00 | 0.69 | 0.00 | 0.38 | -23.46 | 327.79 | 8.34 | 196.99 | 0.4571 | -872.0 | -779.1 | |
| 0.00 | 6.87 | 0.00 | 3.84 | -24.06 | 327.76 | 8.31 | 196.54 | 0.4658 | -612.0 | -651.7 | |
| 0.00 | 1.29 | 0.00 | 0.72 | -23.59 | 327.47 | 8.02 | 196.30 | 0.4576 | -1021.0 | -857.9 | |
| 0.00 | 1.29 | 0.00 | 0.72 | -24.45 | 327.39 | 7.94 | 195.59 | 0.4701 | -705.0 | -582.9 | |
| 0.00 | 0.43 | 0.00 | 0.25 | -26.77 | 327.31 | 7.87 | 194.10 | 0.5038 | -770.0 | -661.4 | |
| 2.58 | 6.18 | 1.43 | 3.44 | -23.75 | 326.99 | 7.54 | 195.27 | 0.4580 | -1024.2 | -751.5 | |
| 0.00 | 1.46 | 0.00 | 0.83 | -26.53 | 327.16 | 7.72 | 193.97 | 0.4997 | -719.0 | -559.5 | |
| 0.00 | 1.03 | 0.00 | 0.58 | -24.45 | 326.90 | 7.45 | 194.67 | 0.4680 | -518.0 | -434.2 | |
| 0.00 | 2.75 | 0.00 | 1.53 | -23.85 | 326.73 | 7.29 | 194.72 | 0.4585 | -954.0 | -841.8 | |
| 0.00 | 0.94 | 0.00 | 0.53 | -24.65 | 326.38 | 6.94 | 193.59 | 0.4690 | -759.0 | -567.4 | |
| 0.00 | 1.12 | 0.00 | 0.62 | -24.54 | 326.02 | 6.57 | 192.96 | 0.4662 | -460.0 | -453.8 | |
| 0.00 | 1.55 | 0.00 | 0.86 | -23.85 | 325.75 | 6.31 | 192.82 | 0.4547 | -898.0 | -795.1 | |
| 0.00 | 1.20 | 0.00 | 0.67 | -24.51 | 325.56 | 6.11 | 192.10 | 0.4641 | -840.0 | -606.4 | |
| 0.00 | 1.20 | 0.00 | 0.67 | -24.37 | 325.29 | 5.84 | 191.65 | 0.4612 | -701.0 | -548.9 | |
| 0.00 | 1.37 | 0.00 | 0.74 | -20.84 | 324.57 | 5.12 | 191.95 | 0.4044 | -531.0 | -503.2 | |
| 0.00 | 1.37 | 0.00 | 0.78 | -26.55 | 323.60 | 4.15 | 187.63 | 0.4898 | -782.0 | -507.4 | |
| 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. | |