SDO HMI 2011-11-29 06:58:56 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 |
| 74.47 | 376.46 | 39.19 | 197.92 | 20.05 | 192.11 | 3.38 | 349.71 | 0.3355 | -4.1 | -209.1 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2011-11-29 06:58:56 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 |
| 20.52 | 224.06 | 10.73 | 117.31 | 18.92 | 194.70 | 5.96 | 342.16 | 0.3222 | -1570.6 | -483.0 | |
| 7.27 | -1.00 | 3.81 | -1.00 | 19.29 | 194.71 | 5.98 | 342.49 | 0.3281 | -1261.9 | 999999 | |
| 4.62 | -1.00 | 2.42 | -1.00 | 19.42 | 194.49 | 5.76 | 343.20 | 0.3290 | -1169.9 | 999999 | |
| 1.71 | -1.00 | 0.90 | -1.00 | 19.17 | 194.42 | 5.69 | 343.17 | 0.3248 | -1143.4 | 999999 | |
| 2.82 | 8.38 | 1.47 | 4.37 | 18.49 | 193.93 | 5.20 | 343.93 | 0.3116 | -1102.3 | -778.1 | |
| 0.00 | 1.37 | 0.00 | 0.73 | 22.53 | 193.97 | 5.24 | 346.98 | 0.3760 | -672.0 | -586.6 | |
| 0.00 | 1.28 | 0.00 | 0.68 | 22.60 | 193.30 | 4.57 | 348.64 | 0.3747 | -735.0 | -496.3 | |
| 0.68 | 3.85 | 0.35 | 1.99 | 17.56 | 192.91 | 4.17 | 346.21 | 0.2923 | -1204.9 | -929.1 | |
| 0.00 | 5.73 | 0.00 | 3.03 | 21.08 | 192.81 | 4.07 | 349.00 | 0.3489 | -727.0 | -685.2 | |
| 0.00 | 1.03 | 0.00 | 0.53 | 18.58 | 192.74 | 4.01 | 347.53 | 0.3083 | -937.0 | -654.6 | |
| 0.00 | 2.74 | 0.00 | 1.43 | 19.70 | 192.52 | 3.78 | 348.95 | 0.3257 | -773.0 | -740.6 | |
| 0.00 | 1.28 | 0.00 | 0.68 | 20.95 | 192.49 | 3.75 | 349.78 | 0.3459 | -892.0 | -699.3 | |
| 0.00 | 1.62 | 0.00 | 0.85 | 19.83 | 192.08 | 3.35 | 350.27 | 0.3264 | -830.0 | -613.7 | |
| 0.00 | 1.45 | 0.00 | 0.76 | 18.46 | 191.99 | 3.26 | 349.74 | 0.3038 | 957.0 | 595.9 | |
| 0.00 | 2.74 | 0.00 | 1.44 | 20.20 | 191.96 | 3.23 | 350.80 | 0.3322 | -1059.0 | -738.0 | |
| 4.96 | 9.06 | 2.60 | 4.76 | 20.17 | 191.55 | 2.82 | 351.94 | 0.3307 | -1043.6 | -634.2 | |
| 0.00 | 1.88 | 0.00 | 0.98 | 19.64 | 190.41 | 1.68 | 355.03 | 0.3198 | -987.0 | -815.6 | |
| 0.00 | 2.05 | 0.00 | 1.04 | 14.11 | 189.97 | 1.23 | 354.69 | 0.2263 | -603.0 | -511.6 | |
| 0.00 | 1.11 | 0.00 | 0.58 | 20.33 | 189.00 | 0.27 | 359.24 | 0.3301 | 752.0 | 662.3 | |
| 0.00 | 1.20 | 0.00 | 0.64 | 22.19 | 188.49 | -0.24 | 0.62 | 0.3606 | 867.0 | 726.1 | |
| 6.33 | 10.60 | 3.34 | 5.59 | 21.18 | 188.40 | -0.33 | 0.91 | 0.3441 | 1096.8 | 756.8 | |
| 0.00 | 1.88 | 0.00 | 0.99 | 20.86 | 187.83 | -0.90 | 2.50 | 0.3392 | 624.0 | 479.5 | |
| 0.00 | 1.37 | 0.00 | 0.73 | 23.24 | 187.82 | -0.92 | 2.24 | 0.3780 | 616.0 | 493.9 | |
| 0.00 | 0.94 | 0.00 | 0.50 | 22.98 | 187.79 | -0.95 | 2.35 | 0.3739 | 828.0 | 686.5 | |
| 0.00 | 1.28 | 0.00 | 0.67 | 20.52 | 187.71 | -1.03 | 2.90 | 0.3336 | -758.0 | -602.4 | |
| 0.00 | 1.80 | 0.00 | 0.96 | 22.76 | 187.40 | -1.33 | 3.33 | 0.3706 | 835.0 | 662.7 | |
| 3.59 | 35.75 | 1.90 | 18.94 | 21.68 | 187.38 | -1.35 | 3.58 | 0.3530 | 1160.7 | 729.9 | |
| 3.16 | -27.00 | 1.68 | -27.00 | 22.25 | 187.28 | -1.46 | 3.74 | 0.3624 | 920.7 | 999999 | |
| 2.22 | -27.00 | 1.18 | -27.00 | 21.93 | 187.15 | -1.58 | 4.12 | 0.3574 | 1077.6 | 999999 | |
| 2.48 | -27.00 | 1.31 | -27.00 | 21.62 | 187.13 | -1.61 | 4.27 | 0.3523 | 983.8 | 999999 | |
| 0.00 | 1.03 | 0.00 | 0.54 | 21.05 | 186.88 | -1.86 | 5.07 | 0.3433 | 879.0 | 790.2 | |
| 14.11 | 18.81 | 7.50 | 9.99 | 22.25 | 186.83 | -1.90 | 4.88 | 0.3630 | 989.3 | 676.6 | |
| 0.00 | 2.39 | 0.00 | 1.26 | 21.27 | 186.50 | -2.24 | 6.04 | 0.3475 | 940.0 | 871.0 | |
| 0.00 | 1.62 | 0.00 | 0.88 | 24.81 | 186.44 | -2.30 | 5.18 | 0.4048 | 979.0 | 787.8 | |
| 0.00 | 2.82 | 0.00 | 1.49 | 21.59 | 186.46 | -2.28 | 6.04 | 0.3527 | 907.0 | 708.6 | |
| 0.00 | 1.20 | 0.00 | 0.63 | 21.87 | 186.45 | -2.28 | 5.96 | 0.3574 | 780.0 | 627.5 | |
| 0.00 | 2.48 | 0.00 | 1.31 | 21.33 | 186.27 | -2.46 | 6.62 | 0.3490 | 778.0 | 697.7 | |
| 0.00 | 1.97 | 0.00 | 1.05 | 22.38 | 186.19 | -2.54 | 6.47 | 0.3661 | 677.0 | 641.8 | |
| 0.00 | 1.97 | 0.00 | 1.05 | 22.57 | 186.06 | -2.68 | 6.73 | 0.3694 | 1043.0 | 858.4 | |
| 0.00 | 1.03 | 0.00 | 0.54 | 22.09 | 185.88 | -2.86 | 7.37 | 0.3621 | 708.0 | 545.8 | |
| 0.00 | 1.03 | 0.00 | 0.54 | 20.73 | 185.87 | -2.86 | 7.93 | 0.3400 | 888.0 | 686.4 | |
| 0.00 | 0.60 | 0.00 | 0.32 | 22.60 | 185.67 | -3.06 | 7.68 | 0.3707 | 829.0 | 705.9 | |
| 0.00 | 1.71 | 0.00 | 0.90 | 20.67 | 185.68 | -3.05 | 8.48 | 0.3395 | 701.0 | 667.8 | |
| 0.00 | 0.94 | 0.00 | 0.50 | 23.08 | 185.50 | -3.23 | 7.91 | 0.3787 | 772.0 | 718.5 | |
| 0.00 | 1.97 | 0.00 | 1.07 | 25.78 | 185.40 | -3.34 | 7.17 | 0.4220 | 640.0 | 544.7 | |
| 0.00 | 2.39 | 0.00 | 1.30 | 25.23 | 184.82 | -3.91 | 8.60 | 0.4145 | 1021.0 | 806.0 | |
| 0.00 | 0.86 | 0.00 | 0.46 | 24.32 | 184.79 | -3.95 | 9.06 | 0.4003 | 768.0 | 673.1 | |
| 0.00 | 0.77 | 0.00 | 0.42 | 25.10 | 184.60 | -4.14 | 9.14 | 0.4130 | 717.0 | 566.6 | |
| 0.00 | 0.60 | 0.00 | 0.33 | 25.42 | 184.29 | -4.44 | 9.66 | 0.4189 | 572.0 | 407.6 | |
| 0.00 | 0.94 | 0.00 | 0.51 | 25.55 | 184.19 | -4.55 | 9.82 | 0.4212 | 677.0 | 558.6 | |
| 0.00 | 1.97 | 0.00 | 1.05 | 22.44 | 184.07 | -4.66 | 11.69 | 0.3725 | 823.0 | 682.8 | |
| 0.00 | 1.11 | 0.00 | 0.59 | 22.34 | 183.27 | -5.46 | 13.68 | 0.3738 | 717.0 | 522.3 | |
| 0.00 | 1.80 | 0.00 | 1.01 | 27.88 | 180.66 | -8.08 | 15.43 | 0.4687 | 436.0 | 486.4 | |
| 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. | |