| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 179.69 | 963.50 | 125.26 | 670.96 | 15.08 | 86.71 | -44.94 | 75.83 | 0.7057 | 239.8 | -73.9 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2014-09-07 18:00:36 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 | 1.43 | 0.00 | 0.93 | 15.12 | 90.72 | -40.93 | 75.23 | 0.6563 | -739.0 | -711.1 | |
| 0.00 | 0.54 | 0.00 | 0.35 | 17.23 | 90.19 | -41.46 | 72.15 | 0.6667 | -644.0 | -546.0 | |
| 0.00 | 0.45 | 0.00 | 0.30 | 17.38 | 90.11 | -41.55 | 71.95 | 0.6680 | -524.0 | -488.8 | |
| 0.00 | 1.34 | 0.00 | 0.88 | 15.19 | 90.54 | -41.11 | 75.15 | 0.6588 | -509.0 | -502.7 | |
| 0.00 | 1.16 | 0.00 | 0.76 | 14.71 | 90.32 | -41.33 | 75.91 | 0.6609 | -645.0 | -536.0 | |
| 0.00 | 2.23 | 0.00 | 1.50 | 16.07 | 89.18 | -42.47 | 74.07 | 0.6770 | 550.0 | 531.2 | |
| 0.00 | 1.69 | 0.00 | 1.15 | 17.57 | 88.63 | -43.02 | 71.98 | 0.6863 | 785.0 | 667.4 | |
| 0.00 | 0.71 | 0.00 | 0.49 | 18.98 | 87.93 | -43.72 | 70.12 | 0.6973 | 604.0 | 527.1 | |
| 0.54 | 904.19 | 0.36 | 629.49 | 15.17 | 88.77 | -42.88 | 75.45 | 0.6808 | 777.7 | -78.4 | |
| 0.00 | 1.16 | 0.00 | 0.80 | 18.96 | 87.67 | -43.98 | 70.20 | 0.7003 | 685.0 | 489.2 | |
| 0.00 | 1.16 | 0.00 | 0.78 | 14.57 | 88.92 | -42.73 | 76.32 | 0.6783 | 586.0 | 443.2 | |
| 0.00 | 0.98 | 0.00 | 0.66 | 14.17 | 88.97 | -42.68 | 76.89 | 0.6772 | 715.0 | 596.3 | |
| 0.00 | 1.25 | 0.00 | 0.87 | 18.96 | 87.40 | -44.25 | 70.25 | 0.7035 | 817.0 | 709.1 | |
| 1.52 | -9.00 | 1.03 | -9.00 | 16.05 | 88.20 | -43.46 | 74.26 | 0.6890 | 1133.1 | 999999 | |
| 0.00 | 0.89 | 0.00 | 0.62 | 18.99 | 87.03 | -44.62 | 70.29 | 0.7078 | 567.0 | 514.2 | |
| 0.00 | 1.07 | 0.00 | 0.75 | 18.82 | 86.82 | -44.83 | 70.57 | 0.7099 | 615.0 | 438.4 | |
| 0.00 | 0.98 | 0.00 | 0.69 | 19.43 | 86.61 | -45.04 | 69.77 | 0.7135 | 512.0 | 428.5 | |
| 0.98 | 9.90 | 0.66 | 6.72 | 13.35 | 88.30 | -43.35 | 78.17 | 0.6847 | 622.5 | 110.7 | |
| 0.00 | 1.78 | 0.00 | 1.25 | 18.70 | 86.82 | -44.83 | 70.75 | 0.7097 | 687.0 | 480.4 | |
| 35.67 | -9.00 | 24.62 | -9.00 | 16.39 | 87.45 | -44.21 | 73.89 | 0.6986 | 997.2 | 999999 | |
| 73.12 | -9.00 | 50.33 | -9.00 | 15.50 | 87.52 | -44.14 | 75.16 | 0.6965 | 1076.4 | 999999 | |
| 0.00 | 0.71 | 0.00 | 0.48 | 11.67 | 88.31 | -43.34 | 80.64 | 0.6835 | -727.0 | -630.9 | |
| 2.05 | -9.00 | 1.42 | -9.00 | 14.94 | 87.14 | -44.52 | 76.00 | 0.7004 | 221.4 | 999999 | |
| 0.00 | 1.07 | 0.00 | 0.76 | 18.32 | 86.13 | -45.53 | 71.40 | 0.7170 | 511.0 | 460.2 | |
| 0.27 | -9.00 | 0.19 | -9.00 | 15.99 | 86.81 | -44.85 | 74.55 | 0.7056 | 384.3 | 999999 | |
| 0.62 | -9.00 | 0.43 | -9.00 | 12.96 | 87.31 | -44.34 | 78.82 | 0.6966 | -916.1 | 999999 | |
| 0.00 | 0.98 | 0.00 | 0.70 | 17.99 | 85.87 | -45.78 | 71.90 | 0.7194 | 489.0 | 407.8 | |
| 0.98 | -9.00 | 0.69 | -9.00 | 16.58 | 86.09 | -45.56 | 73.83 | 0.7148 | 347.7 | 999999 | |
| 0.00 | 2.14 | 0.00 | 1.53 | 17.59 | 85.59 | -46.06 | 72.50 | 0.7220 | 647.0 | 461.0 | |
| 0.00 | 3.21 | 0.00 | 2.29 | 16.87 | 85.46 | -46.19 | 73.52 | 0.7225 | 536.0 | 442.6 | |
| 1.34 | -9.00 | 0.93 | -9.00 | 12.77 | 86.48 | -45.17 | 79.15 | 0.7066 | -845.8 | 999999 | |
| 0.00 | 4.10 | 0.00 | 2.86 | 12.43 | 86.51 | -45.14 | 79.63 | 0.7061 | -472.0 | -517.3 | |
| 12.57 | -9.00 | 8.80 | -9.00 | 13.12 | 86.31 | -45.34 | 78.67 | 0.7088 | -1003.5 | 999999 | |
| 0.00 | 0.89 | 0.00 | 0.62 | 12.22 | 86.51 | -45.14 | 79.93 | 0.7059 | -648.0 | -576.7 | |
| 2.68 | -9.00 | 1.88 | -9.00 | 13.62 | 86.06 | -45.60 | 77.98 | 0.7122 | -856.2 | 999999 | |
| 2.41 | -9.00 | 1.69 | -9.00 | 13.38 | 86.07 | -45.58 | 78.32 | 0.7119 | -869.2 | 999999 | |
| 2.23 | -9.00 | 1.59 | -9.00 | 15.41 | 85.44 | -46.21 | 75.54 | 0.7210 | 117.0 | 999999 | |
| 0.00 | 1.43 | 0.00 | 1.01 | 12.74 | 85.86 | -45.79 | 79.22 | 0.7140 | -478.0 | -427.6 | |
| 12.66 | -9.00 | 9.07 | -9.00 | 14.45 | 85.03 | -46.62 | 76.91 | 0.7249 | -1145.8 | 999999 | |
| 10.43 | -9.00 | 7.44 | -9.00 | 13.58 | 85.26 | -46.39 | 78.10 | 0.7216 | -921.6 | 999999 | |
| 2.32 | -9.00 | 1.67 | -9.00 | 14.80 | 84.80 | -46.86 | 76.45 | 0.7280 | -706.1 | 999999 | |
| 0.00 | 2.05 | 0.00 | 1.46 | 12.33 | 85.38 | -46.28 | 79.82 | 0.7196 | -577.0 | -452.7 | |
| 0.89 | -9.00 | 0.64 | -9.00 | 13.83 | 84.92 | -46.73 | 77.78 | 0.7257 | -803.2 | 999999 | |
| 14.00 | -9.00 | 10.08 | -9.00 | 14.21 | 84.77 | -46.88 | 77.26 | 0.7277 | -818.6 | 999999 | |
| 2.41 | -9.00 | 1.74 | -9.00 | 14.53 | 84.50 | -47.15 | 76.85 | 0.7311 | -479.3 | 999999 | |
| 0.00 | 1.34 | 0.00 | 0.96 | 12.18 | 85.05 | -46.60 | 80.05 | 0.7234 | -279.0 | -329.4 | |
| 0.00 | 0.98 | 0.00 | 0.71 | 12.39 | 84.59 | -47.06 | 79.78 | 0.7288 | -465.0 | -333.5 | |
| 0.00 | 0.98 | 0.00 | 0.70 | 11.15 | 84.78 | -46.87 | 81.48 | 0.7264 | -366.0 | -308.9 | |
| 0.00 | 1.61 | 0.00 | 1.18 | 14.87 | 83.57 | -48.09 | 76.46 | 0.7421 | -579.0 | -420.9 | |
| 0.00 | 0.54 | 0.00 | 0.39 | 13.51 | 83.81 | -47.84 | 78.29 | 0.7384 | -632.0 | -560.7 | |
| 0.00 | 2.05 | 0.00 | 1.52 | 14.29 | 83.27 | -48.39 | 77.27 | 0.7451 | -531.0 | -432.9 | |
| 0.00 | 1.43 | 0.00 | 1.05 | 12.66 | 83.61 | -48.05 | 79.44 | 0.7404 | -605.0 | -466.7 | |
| 0.00 | 1.69 | 0.00 | 1.25 | 13.88 | 83.19 | -48.46 | 77.82 | 0.7457 | -386.0 | -294.4 | |
| 0.00 | 1.78 | 0.00 | 1.32 | 14.12 | 83.08 | -48.57 | 77.51 | 0.7471 | -325.0 | -216.4 | |
| 0.00 | 1.61 | 0.00 | 1.18 | 12.83 | 83.42 | -48.23 | 79.23 | 0.7425 | -546.0 | -435.3 | |
| 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. | |