| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 56.22 | 216.58 | 27.96 | 107.69 | 8.96 | 289.45 | 1.89 | 284.23 | 0.0822 | -496.9 | -338.5 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2014-09-23 05:00:34 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 | 2.30 | 0.00 | 1.15 | 6.04 | 294.66 | 7.10 | 262.39 | 0.1246 | 530.0 | 557.2 | |
| 0.00 | 1.51 | 0.00 | 0.75 | 10.74 | 292.29 | 4.73 | 308.74 | 0.1043 | -802.0 | -622.2 | |
| 0.00 | 1.33 | 0.00 | 0.66 | 10.53 | 292.19 | 4.63 | 307.67 | 0.1008 | -981.0 | -794.6 | |
| 18.68 | 27.89 | 9.29 | 13.86 | 5.14 | 291.91 | 4.35 | 246.65 | 0.0828 | -1232.0 | -715.8 | |
| 0.00 | 2.92 | 0.00 | 1.45 | 10.32 | 291.91 | 4.35 | 307.67 | 0.0948 | -955.0 | -818.5 | |
| 0.00 | 8.15 | 0.00 | 4.05 | 5.51 | 291.40 | 3.84 | 248.46 | 0.0721 | -762.0 | -836.1 | |
| 0.00 | 4.34 | 0.00 | 2.15 | 5.33 | 291.10 | 3.54 | 244.37 | 0.0685 | -1047.0 | -897.5 | |
| 0.00 | 1.33 | 0.00 | 0.66 | 5.54 | 291.07 | 3.51 | 247.05 | 0.0665 | -769.0 | -579.1 | |
| 0.00 | 1.15 | 0.00 | 0.57 | 5.00 | 290.55 | 2.99 | 235.87 | 0.0631 | -893.0 | -703.8 | |
| 0.00 | 1.06 | 0.00 | 0.53 | 5.43 | 290.49 | 2.93 | 241.31 | 0.0584 | -868.0 | -619.2 | |
| 0.35 | 5.05 | 0.18 | 2.50 | 5.21 | 290.43 | 2.87 | 237.69 | 0.0593 | -1079.2 | -782.1 | |
| 7.17 | 130.51 | 3.57 | 64.87 | 11.30 | 290.33 | 2.77 | 327.52 | 0.0887 | -1118.4 | -488.3 | |
| 0.00 | 1.68 | 0.00 | 0.83 | 5.34 | 290.07 | 2.51 | 235.96 | 0.0529 | -929.0 | -700.6 | |
| 0.00 | 1.42 | 0.00 | 0.70 | 3.89 | 289.97 | 2.41 | 217.54 | 0.0692 | 879.0 | 604.8 | |
| 22.49 | -12.00 | 11.18 | -12.00 | 11.03 | 289.77 | 2.22 | 331.46 | 0.0798 | -1328.6 | 999999 | |
| 0.00 | 1.15 | 0.00 | 0.57 | 5.64 | 289.61 | 2.06 | 235.90 | 0.0434 | 835.0 | 604.2 | |
| 1.24 | -12.00 | 0.62 | -12.00 | 11.15 | 289.44 | 1.88 | 335.88 | 0.0791 | -991.0 | 999999 | |
| 6.29 | -12.00 | 3.12 | -12.00 | 10.91 | 289.28 | 1.72 | 336.41 | 0.0742 | -1158.3 | 999999 | |
| 0.00 | 1.59 | 0.00 | 0.79 | 6.52 | 287.41 | -0.15 | 163.95 | 0.0093 | 823.0 | 672.1 | |
| 0.00 | 1.68 | 0.00 | 0.83 | 6.58 | 287.08 | -0.48 | 133.33 | 0.0115 | 869.0 | 793.7 | |
| 0.00 | 1.24 | 0.00 | 0.61 | 6.28 | 286.29 | -1.27 | 120.78 | 0.0257 | 894.0 | 686.6 | |
| 0.00 | 2.92 | 0.00 | 1.45 | 5.26 | 286.14 | -1.42 | 141.47 | 0.0397 | 980.0 | 781.7 | |
| 0.00 | 4.43 | 0.00 | 2.20 | 5.29 | 285.84 | -1.72 | 135.50 | 0.0428 | 660.0 | 682.2 | |
| 0.00 | 1.15 | 0.00 | 0.57 | 5.08 | 285.72 | -1.84 | 136.81 | 0.0470 | 938.0 | 808.1 | |
| 0.00 | 0.71 | 0.00 | 0.35 | 7.96 | 285.56 | -2.00 | 64.73 | 0.0384 | 808.0 | 551.0 | |
| 0.00 | 2.39 | 0.00 | 1.19 | 4.07 | 283.75 | -3.80 | 127.84 | 0.0841 | 840.0 | 775.7 | |
| 0.00 | 0.97 | 0.00 | 0.48 | 8.10 | 283.30 | -4.25 | 75.50 | 0.0762 | 1104.0 | 927.5 | |
| 0.00 | 0.80 | 0.00 | 0.40 | 7.95 | 283.00 | -4.56 | 78.25 | 0.0807 | 755.0 | 557.3 | |
| 0.00 | 1.95 | 0.00 | 0.98 | 11.62 | 278.10 | -9.46 | 63.13 | 0.1813 | 767.0 | 418.9 | |
| 0.00 | 0.97 | 0.00 | 0.49 | 7.51 | 274.83 | -12.72 | 87.04 | 0.2196 | 902.0 | 733.0 | |
| 0.00 | 0.89 | 0.00 | 0.45 | 1.24 | 274.93 | -12.62 | 114.14 | 0.2405 | 651.0 | 524.5 | |
| 0.00 | 1.42 | 0.00 | 0.73 | 0.23 | 273.33 | -14.23 | 115.01 | 0.2725 | 852.0 | 670.7 | |
| 0.00 | 0.62 | 0.00 | 0.32 | 2.12 | 272.95 | -14.61 | 107.94 | 0.2661 | 569.0 | 583.1 | |
| 0.00 | 1.06 | 0.00 | 0.55 | 8.80 | 269.77 | -17.78 | 83.09 | 0.3054 | 838.0 | 642.8 | |
| 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. | |