SDO HMI 2011-06-04 12:59:10 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!)
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 62.56 | 431.16 | 35.24 | 242.61 | -22.18 | 35.32 | 18.45 | 218.14 | 0.4778 | 134.8 | 17.2 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2011-06-04 12:59:10 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 | 0.63 | 0.00 | 0.37 | -21.40 | 41.49 | 24.62 | 227.08 | 0.5317 | 734.0 | 508.6 | |
| 0.00 | 1.45 | 0.00 | 0.83 | -21.86 | 39.39 | 22.52 | 224.00 | 0.5138 | 629.0 | 468.2 | |
| 20.16 | 69.08 | 11.40 | 39.03 | -19.37 | 38.79 | 21.93 | 227.12 | 0.4827 | 1135.2 | 440.0 | |
| 0.00 | 1.09 | 0.00 | 0.63 | -23.98 | 39.26 | 22.39 | 220.88 | 0.5339 | 636.0 | 563.7 | |
| 0.00 | 1.99 | 0.00 | 1.17 | -24.21 | 39.20 | 22.33 | 220.49 | 0.5357 | 758.0 | 645.4 | |
| 0.00 | 2.26 | 0.00 | 1.32 | -23.64 | 38.91 | 22.05 | 220.91 | 0.5271 | 786.0 | 703.8 | |
| 0.00 | 10.58 | 0.00 | 6.14 | -23.68 | 38.38 | 21.51 | 220.21 | 0.5223 | 867.0 | 754.8 | |
| 0.00 | 3.71 | 0.00 | 2.14 | -23.58 | 37.83 | 20.96 | 219.65 | 0.5159 | 641.0 | 694.4 | |
| 0.00 | 0.99 | 0.00 | 0.56 | -20.11 | 37.30 | 20.43 | 224.01 | 0.4738 | 812.0 | 665.2 | |
| 0.00 | 0.99 | 0.00 | 0.56 | -20.27 | 37.12 | 20.25 | 223.51 | 0.4735 | 573.0 | 521.5 | |
| 0.00 | 0.99 | 0.00 | 0.56 | -19.75 | 37.01 | 20.15 | 224.18 | 0.4670 | 675.0 | 556.5 | |
| 0.00 | 3.16 | 0.00 | 1.77 | -19.53 | 36.92 | 20.05 | 224.41 | 0.4636 | 949.0 | 856.6 | |
| 0.00 | 0.99 | 0.00 | 0.57 | -23.15 | 37.44 | 20.57 | 219.73 | 0.5075 | 804.0 | 681.1 | |
| 0.00 | 6.42 | 0.00 | 3.59 | -19.95 | 36.80 | 19.93 | 223.58 | 0.4667 | 919.0 | 765.7 | |
| 0.00 | 4.88 | 0.00 | 2.73 | -20.11 | 36.44 | 19.57 | 222.83 | 0.4646 | 888.0 | 651.4 | |
| 0.00 | 0.81 | 0.00 | 0.45 | -20.18 | 36.21 | 19.34 | 222.40 | 0.4629 | 463.0 | 460.2 | |
| 4.61 | 14.92 | 2.57 | 8.34 | -20.69 | 35.59 | 18.72 | 220.71 | 0.4622 | 936.5 | 535.5 | |
| 2.08 | -17.00 | 1.16 | -17.00 | -21.22 | 35.38 | 18.51 | 219.63 | 0.4660 | 768.3 | 999999 | |
| 3.80 | 127.77 | 2.16 | 72.21 | -23.78 | 35.50 | 18.63 | 216.24 | 0.4965 | 763.1 | -270.8 | |
| 0.00 | 1.09 | 0.00 | 0.62 | -24.45 | 35.60 | 18.73 | 215.52 | 0.5051 | -623.0 | -509.4 | |
| 0.00 | 0.99 | 0.00 | 0.57 | -25.05 | 35.62 | 18.75 | 214.80 | 0.5124 | -631.0 | -544.5 | |
| 0.00 | 1.45 | 0.00 | 0.82 | -24.01 | 35.01 | 18.14 | 215.23 | 0.4948 | -576.0 | -397.5 | |
| 0.00 | 3.16 | 0.00 | 1.77 | -21.67 | 34.62 | 17.75 | 217.82 | 0.4638 | 781.0 | 657.7 | |
| 0.36 | 133.01 | 0.20 | 74.38 | -22.03 | 34.63 | 17.76 | 217.33 | 0.4681 | 893.5 | -74.3 | |
| 0.81 | -24.00 | 0.46 | -24.00 | -22.33 | 34.67 | 17.80 | 216.98 | 0.4719 | 738.8 | 999999 | |
| 2.44 | -24.00 | 1.37 | -24.00 | -22.16 | 34.51 | 17.64 | 216.97 | 0.4685 | 1064.3 | 999999 | |
| 0.00 | 2.62 | 0.00 | 1.45 | -19.98 | 34.21 | 17.34 | 219.71 | 0.4402 | -960.0 | -720.2 | |
| 0.00 | 3.26 | 0.00 | 1.81 | -21.58 | 34.40 | 17.53 | 217.63 | 0.4606 | 857.0 | 763.3 | |
| 4.07 | -24.00 | 2.28 | -24.00 | -22.39 | 34.43 | 17.56 | 216.54 | 0.4706 | 918.2 | 999999 | |
| 2.71 | 6.96 | 1.51 | 3.89 | -21.87 | 34.30 | 17.43 | 217.06 | 0.4631 | 922.3 | 706.3 | |
| 1.54 | -19.00 | 0.87 | -19.00 | -23.52 | 34.48 | 17.61 | 215.11 | 0.4843 | -788.8 | 999999 | |
| 14.29 | -19.00 | 8.11 | -19.00 | -24.08 | 34.35 | 17.48 | 214.19 | 0.4900 | -968.1 | 999999 | |
| 0.00 | 1.18 | 0.00 | 0.65 | -20.18 | 33.69 | 16.82 | 218.58 | 0.4373 | -926.0 | -821.7 | |
| 0.45 | -19.00 | 0.25 | -19.00 | -23.55 | 33.89 | 17.03 | 214.19 | 0.4796 | 461.4 | 999999 | |
| 0.00 | 1.27 | 0.00 | 0.70 | -20.99 | 33.54 | 16.67 | 217.14 | 0.4455 | -1007.0 | -769.0 | |
| 2.89 | 3.35 | 1.60 | 1.85 | -21.15 | 33.19 | 16.32 | 216.33 | 0.4441 | -965.4 | -773.6 | |
| 0.00 | 1.54 | 0.00 | 0.85 | -20.66 | 33.13 | 16.26 | 216.95 | 0.4377 | -909.0 | -563.5 | |
| 0.00 | 1.45 | 0.00 | 0.80 | -21.45 | 33.12 | 16.25 | 215.80 | 0.4471 | -887.0 | -735.8 | |
| 0.00 | 2.08 | 0.00 | 1.18 | -24.25 | 33.36 | 16.49 | 212.50 | 0.4837 | -791.0 | -568.9 | |
| 1.54 | -24.00 | 0.85 | -24.00 | -21.77 | 33.02 | 16.15 | 215.18 | 0.4502 | -934.4 | 999999 | |
| 0.00 | 2.98 | 0.00 | 1.67 | -22.86 | 33.11 | 16.25 | 213.88 | 0.4644 | -252.0 | -341.9 | |
| 0.00 | 1.09 | 0.00 | 0.58 | -16.85 | 32.36 | 15.49 | 221.87 | 0.3846 | -800.0 | -568.1 | |
| 0.81 | -24.00 | 0.45 | -24.00 | -22.53 | 32.80 | 15.93 | 213.80 | 0.4576 | -1024.0 | 999999 | |
| 0.00 | 1.27 | 0.00 | 0.70 | -22.13 | 32.51 | 15.65 | 213.86 | 0.4502 | -882.0 | -733.2 | |
| 0.00 | 1.09 | 0.00 | 0.61 | -23.68 | 32.53 | 15.66 | 211.89 | 0.4698 | -599.0 | -491.1 | |
| 0.00 | 1.36 | 0.00 | 0.75 | -21.90 | 32.15 | 15.28 | 213.56 | 0.4441 | -916.0 | -760.7 | |
| 0.00 | 1.09 | 0.00 | 0.60 | -22.63 | 32.23 | 15.36 | 212.74 | 0.4539 | -664.0 | -555.8 | |
| 0.00 | 1.54 | 0.00 | 0.85 | -22.00 | 31.95 | 15.09 | 213.10 | 0.4437 | -863.0 | -734.2 | |
| 0.00 | 0.72 | 0.00 | 0.40 | -22.50 | 31.63 | 14.77 | 211.91 | 0.4473 | -734.0 | -597.0 | |
| 0.00 | 1.18 | 0.00 | 0.64 | -21.25 | 31.33 | 14.47 | 213.04 | 0.4288 | -909.0 | -708.2 | |
| 0.00 | 1.63 | 0.00 | 0.89 | -21.87 | 31.09 | 14.22 | 211.78 | 0.4347 | -959.0 | -842.3 | |
| 0.00 | 1.09 | 0.00 | 0.61 | -24.82 | 29.66 | 12.79 | 205.83 | 0.4632 | -808.0 | -602.0 | |
| 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. | |