| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 24.74 | 100.56 | 16.67 | 68.36 | -4.73 | 84.17 | -42.32 | 101.62 | 0.6870 | 328.3 | 261.1 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2014-11-01 17:00:28 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 | 0.61 | 0.00 | 0.39 | -4.47 | 86.95 | -39.54 | 102.08 | 0.6513 | 696.0 | 578.9 | |
| 0.43 | 1.47 | 0.29 | 0.97 | -6.03 | 86.48 | -40.01 | 104.24 | 0.6620 | 660.4 | 614.6 | |
| 0.00 | 1.12 | 0.00 | 0.74 | -5.32 | 86.15 | -40.34 | 103.08 | 0.6640 | -595.0 | -469.8 | |
| 0.00 | 1.47 | 0.00 | 0.98 | -6.54 | 85.80 | -40.69 | 104.75 | 0.6721 | -415.0 | -498.6 | |
| 0.00 | 1.21 | 0.00 | 0.81 | -6.01 | 85.54 | -40.95 | 103.89 | 0.6738 | -722.0 | -589.8 | |
| 0.00 | 1.21 | 0.00 | 0.80 | -4.35 | 85.63 | -40.86 | 101.49 | 0.6680 | 589.0 | 353.0 | |
| 0.00 | 1.56 | 0.00 | 1.04 | -5.78 | 85.40 | -41.09 | 103.50 | 0.6749 | -658.0 | -535.5 | |
| 0.00 | 1.12 | 0.00 | 0.75 | -5.60 | 85.29 | -41.20 | 103.22 | 0.6757 | -426.0 | -443.0 | |
| 0.00 | 2.08 | 0.00 | 1.39 | -5.27 | 85.28 | -41.21 | 102.73 | 0.6749 | -688.0 | -668.9 | |
| 4.41 | 7.96 | 2.97 | 5.37 | -5.68 | 84.93 | -41.56 | 103.21 | 0.6805 | 687.1 | 448.5 | |
| 0.00 | 1.04 | 0.00 | 0.70 | -5.30 | 84.76 | -41.73 | 102.61 | 0.6815 | 658.0 | 598.5 | |
| 16.52 | 56.58 | 11.13 | 38.11 | -4.22 | 84.68 | -41.81 | 101.02 | 0.6797 | 1032.2 | 510.9 | |
| 2.34 | -12.00 | 1.58 | -12.00 | -4.73 | 84.60 | -41.88 | 101.75 | 0.6819 | 703.5 | 999999 | |
| 0.00 | 2.08 | 0.00 | 1.41 | -5.01 | 84.46 | -42.03 | 102.10 | 0.6844 | 633.0 | 456.0 | |
| 1.04 | -12.00 | 0.70 | -12.00 | -3.91 | 84.14 | -42.35 | 100.44 | 0.6858 | 725.7 | 999999 | |
| 0.00 | 1.30 | 0.00 | 0.88 | -3.46 | 84.17 | -42.32 | 99.79 | 0.6844 | 632.0 | 516.3 | |
| 0.00 | 1.21 | 0.00 | 0.83 | -5.52 | 84.01 | -42.48 | 102.69 | 0.6913 | 364.0 | 268.4 | |
| 0.00 | 1.99 | 0.00 | 1.36 | -4.91 | 83.98 | -42.51 | 101.82 | 0.6901 | 625.0 | 530.4 | |
| 0.00 | 3.81 | 0.00 | 2.59 | -3.71 | 83.99 | -42.50 | 100.10 | 0.6872 | 736.0 | 576.8 | |
| 0.00 | 1.30 | 0.00 | 0.89 | -5.16 | 83.84 | -42.65 | 102.14 | 0.6925 | 514.0 | 329.5 | |
| 0.00 | 0.26 | 0.00 | 0.18 | -4.65 | 83.31 | -43.18 | 101.26 | 0.6978 | 446.0 | 422.3 | |
| 0.00 | 1.30 | 0.00 | 0.90 | -4.50 | 83.24 | -43.25 | 101.03 | 0.6983 | 477.0 | 383.5 | |
| 0.00 | 0.95 | 0.00 | 0.67 | -4.60 | 81.86 | -44.63 | 100.80 | 0.7153 | -589.0 | -511.1 | |
| 0.00 | 0.61 | 0.00 | 0.43 | -5.15 | 81.68 | -44.81 | 101.52 | 0.7186 | -695.0 | -546.0 | |
| 0.00 | 1.12 | 0.00 | 0.80 | -5.34 | 81.54 | -44.95 | 101.73 | 0.7208 | 91.0 | 59.7 | |
| 0.00 | 1.04 | 0.00 | 0.75 | -4.06 | 80.15 | -46.34 | 99.65 | 0.7343 | 520.0 | 363.9 | |
| 0.00 | 1.04 | 0.00 | 0.77 | -5.94 | 79.45 | -47.04 | 101.98 | 0.7465 | -692.0 | -496.1 | |
| 0.00 | 0.61 | 0.00 | 0.45 | -6.17 | 79.06 | -47.43 | 102.18 | 0.7513 | -644.0 | -567.0 | |
| 0.00 | 2.60 | 0.00 | 1.96 | -6.50 | 78.62 | -47.87 | 102.49 | 0.7570 | -715.0 | -555.9 | |
| 0.00 | 0.52 | 0.00 | 0.39 | -6.72 | 78.55 | -47.94 | 102.75 | 0.7583 | -515.0 | -394.8 | |
| 0.00 | 0.87 | 0.00 | 0.65 | -6.23 | 78.57 | -47.92 | 102.13 | 0.7570 | -476.0 | -484.8 | |
| 0.00 | 0.52 | 0.00 | 0.40 | -7.78 | 77.99 | -48.50 | 103.97 | 0.7670 | -489.0 | -489.5 | |
| 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. | |