| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 63.12 | 275.97 | 31.37 | 137.19 | 5.96 | 204.13 | 3.62 | 289.57 | 0.0789 | -295.1 | -217.9 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2014-07-10 02:00:40 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 | 0.73 | 0.00 | 0.36 | 6.38 | 208.17 | 7.67 | 288.81 | 0.1407 | -765.0 | -574.1 | |
| 0.00 | 1.63 | 0.00 | 0.81 | 3.86 | 206.48 | 5.97 | 270.60 | 0.1043 | -997.0 | -771.0 | |
| 23.88 | 148.75 | 11.89 | 74.04 | 6.01 | 205.49 | 4.98 | 293.94 | 0.0949 | -1399.4 | -457.5 | |
| 0.73 | 3.09 | 0.36 | 1.53 | 4.46 | 204.49 | 3.98 | 279.20 | 0.0705 | -1081.5 | -834.0 | |
| 5.54 | 11.62 | 2.75 | 5.77 | 4.95 | 204.16 | 3.65 | 287.28 | 0.0667 | -1189.0 | -864.2 | |
| 0.00 | 1.27 | 0.00 | 0.63 | 6.04 | 204.07 | 3.57 | 302.15 | 0.0734 | -952.0 | -727.1 | |
| 9.17 | 22.43 | 4.55 | 11.14 | 5.50 | 204.04 | 3.53 | 295.55 | 0.0683 | -1155.3 | -746.7 | |
| 6.45 | -7.00 | 3.20 | -7.00 | 5.41 | 203.79 | 3.29 | 295.91 | 0.0637 | -1221.6 | 999999 | |
| 0.00 | 1.00 | 0.00 | 0.50 | 8.06 | 203.57 | 3.06 | 324.45 | 0.0914 | -803.0 | -573.1 | |
| 0.00 | 0.91 | 0.00 | 0.45 | 4.40 | 203.30 | 2.79 | 281.85 | 0.0498 | 764.0 | 577.6 | |
| 1.00 | 13.17 | 0.50 | 6.54 | 7.15 | 203.13 | 2.62 | 321.96 | 0.0740 | -1029.5 | -846.6 | |
| 0.82 | -11.00 | 0.41 | -11.00 | 6.87 | 203.07 | 2.56 | 320.22 | 0.0696 | -1150.9 | 999999 | |
| 0.00 | 0.91 | 0.00 | 0.45 | 6.29 | 202.94 | 2.43 | 315.64 | 0.0606 | -791.0 | -544.6 | |
| 0.00 | 1.18 | 0.00 | 0.59 | 7.64 | 202.55 | 2.04 | 332.05 | 0.0757 | 496.0 | 352.2 | |
| 4.45 | 35.24 | 2.21 | 17.47 | 5.35 | 202.41 | 1.91 | 308.84 | 0.0428 | 1063.3 | 564.4 | |
| 5.18 | -15.00 | 2.57 | -15.00 | 5.69 | 202.23 | 1.73 | 317.36 | 0.0444 | 1191.7 | 999999 | |
| 0.00 | 7.17 | 0.00 | 3.56 | 7.70 | 202.24 | 1.74 | 336.07 | 0.0743 | 1133.0 | 774.1 | |
| 2.36 | -15.00 | 1.17 | -15.00 | 5.47 | 202.20 | 1.69 | 314.40 | 0.0414 | 1174.0 | 999999 | |
| 0.00 | 1.91 | 0.00 | 0.95 | 6.30 | 202.14 | 1.64 | 326.68 | 0.0519 | 1012.0 | 791.8 | |
| 0.00 | 1.09 | 0.00 | 0.54 | 7.30 | 202.06 | 1.55 | 336.18 | 0.0667 | -696.0 | -466.2 | |
| 0.00 | 1.09 | 0.00 | 0.54 | 5.57 | 201.96 | 1.45 | 320.39 | 0.0397 | 928.0 | 706.5 | |
| 1.00 | 4.27 | 0.50 | 2.12 | 7.64 | 201.90 | 1.40 | 340.06 | 0.0711 | 1101.1 | 823.5 | |
| 2.54 | 4.99 | 1.26 | 2.48 | 5.35 | 201.74 | 1.23 | 321.23 | 0.0344 | 1111.0 | 870.0 | |
| 0.00 | 1.18 | 0.00 | 0.59 | 6.02 | 201.31 | 0.81 | 339.95 | 0.0411 | 941.0 | 759.0 | |
| 0.00 | 1.45 | 0.00 | 0.72 | 5.87 | 199.17 | -1.34 | 32.95 | 0.0429 | 993.0 | 796.1 | |
| 0.00 | 1.09 | 0.00 | 0.54 | 5.93 | 198.99 | -1.52 | 35.60 | 0.0455 | 891.0 | 714.1 | |
| 0.00 | 1.09 | 0.00 | 0.54 | 5.51 | 198.59 | -1.92 | 48.54 | 0.0447 | 953.0 | 809.1 | |
| 0.00 | 2.45 | 0.00 | 1.22 | 5.42 | 198.41 | -2.10 | 52.67 | 0.0461 | 896.0 | 796.6 | |
| 0.00 | 1.54 | 0.00 | 0.77 | 7.34 | 197.54 | -2.97 | 39.93 | 0.0804 | 910.0 | 770.2 | |
| 0.00 | 2.00 | 0.00 | 0.99 | 6.60 | 197.05 | -3.46 | 50.93 | 0.0775 | 953.0 | 802.4 | |
| 0.00 | 1.63 | 0.00 | 0.81 | 6.82 | 196.80 | -3.70 | 50.78 | 0.0831 | 868.0 | 682.8 | |
| 0.00 | 1.09 | 0.00 | 0.54 | 6.81 | 196.40 | -4.10 | 53.62 | 0.0886 | 798.0 | 605.7 | |
| 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. | |