| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 60.91 | 174.86 | 40.38 | 115.13 | -19.20 | 107.45 | 36.77 | 239.13 | 0.6603 | 8.9 | -76.4 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2014-12-03 06:00:25 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 | 1.54 | 0.00 | 1.08 | -20.00 | 111.82 | 41.14 | 240.52 | 0.7126 | 591.0 | 456.3 | |
| 10.51 | 21.87 | 7.28 | 15.11 | -19.67 | 110.89 | 40.21 | 240.47 | 0.7010 | 721.7 | 540.3 | |
| 1.03 | -2.00 | 0.70 | -2.00 | -19.42 | 110.53 | 39.85 | 240.62 | 0.6958 | 743.1 | 999999 | |
| 0.00 | 1.45 | 0.00 | 0.99 | -19.23 | 110.31 | 39.63 | 240.76 | 0.6925 | 409.0 | 411.1 | |
| 0.00 | 1.79 | 0.00 | 1.23 | -19.51 | 110.27 | 39.59 | 240.36 | 0.6935 | 710.0 | 631.9 | |
| 0.00 | 2.05 | 0.00 | 1.42 | -20.21 | 110.48 | 39.80 | 239.55 | 0.6991 | 629.0 | 614.2 | |
| 10.17 | 15.38 | 6.92 | 10.47 | -19.13 | 110.00 | 39.32 | 240.73 | 0.6886 | 842.6 | 611.0 | |
| 0.00 | 4.27 | 0.00 | 2.89 | -19.09 | 109.50 | 38.82 | 240.51 | 0.6829 | 704.0 | 566.0 | |
| 0.00 | 1.20 | 0.00 | 0.81 | -19.35 | 109.57 | 38.89 | 240.21 | 0.6850 | 214.0 | 188.1 | |
| 1.45 | 22.89 | 0.97 | 15.21 | -18.75 | 109.09 | 38.40 | 240.76 | 0.6765 | 753.3 | 276.1 | |
| 1.20 | -10.00 | 0.80 | -10.00 | -18.62 | 108.53 | 37.85 | 240.63 | 0.6696 | -457.9 | 999999 | |
| 1.79 | -10.00 | 1.19 | -10.00 | -18.36 | 108.39 | 37.71 | 240.90 | 0.6667 | 629.6 | 999999 | |
| 1.37 | -10.00 | 0.90 | -10.00 | -18.24 | 108.20 | 37.52 | 240.97 | 0.6639 | 808.7 | 999999 | |
| 3.33 | -10.00 | 2.20 | -10.00 | -18.46 | 108.18 | 37.50 | 240.65 | 0.6647 | -338.2 | 999999 | |
| 2.99 | 5.47 | 1.95 | 3.57 | -17.33 | 107.70 | 37.02 | 241.97 | 0.6535 | 756.9 | 562.0 | |
| 5.89 | 15.12 | 3.84 | 9.86 | -19.07 | 106.85 | 36.17 | 239.01 | 0.6529 | -686.4 | -434.0 | |
| 0.00 | 1.28 | 0.00 | 0.83 | -18.82 | 106.63 | 35.95 | 239.23 | 0.6490 | -685.0 | -570.4 | |
| 2.56 | -16.00 | 1.67 | -16.00 | -19.32 | 106.72 | 36.04 | 238.59 | 0.6528 | -730.7 | 999999 | |
| 1.45 | -16.00 | 0.95 | -16.00 | -19.48 | 106.64 | 35.96 | 238.32 | 0.6529 | -735.5 | 999999 | |
| 2.22 | 7.09 | 1.44 | 4.59 | -19.26 | 106.35 | 35.67 | 238.45 | 0.6483 | -809.2 | -712.6 | |
| 0.60 | 5.47 | 0.39 | 3.54 | -19.38 | 106.15 | 35.47 | 238.15 | 0.6468 | -935.1 | -679.9 | |
| 0.00 | 1.45 | 0.00 | 0.94 | -18.91 | 105.96 | 35.28 | 238.69 | 0.6418 | -847.0 | -696.3 | |
| 0.51 | -21.00 | 0.33 | -21.00 | -19.60 | 106.05 | 35.37 | 237.78 | 0.6469 | -671.2 | 999999 | |
| 0.00 | 0.51 | 0.00 | 0.33 | -19.60 | 105.70 | 35.02 | 237.56 | 0.6430 | -573.0 | -494.2 | |
| 0.43 | 2.99 | 0.27 | 1.91 | -18.68 | 105.41 | 34.73 | 238.65 | 0.6342 | -734.8 | -604.5 | |
| 0.00 | 1.54 | 0.00 | 0.98 | -18.31 | 105.32 | 34.64 | 239.14 | 0.6310 | -811.0 | -726.1 | |
| 0.94 | 49.46 | 0.60 | 31.74 | -19.53 | 105.34 | 34.66 | 237.41 | 0.6385 | -867.5 | -414.1 | |
| 3.16 | 4.87 | 2.01 | 3.09 | -18.40 | 105.00 | 34.32 | 238.80 | 0.6278 | 771.6 | 533.6 | |
| 6.41 | -27.00 | 4.11 | -27.00 | -19.72 | 105.28 | 34.59 | 237.10 | 0.6389 | -918.5 | 999999 | |
| 0.68 | 4.61 | 0.44 | 2.94 | -18.96 | 105.05 | 34.37 | 238.03 | 0.6318 | -521.2 | -143.4 | |
| 2.22 | -27.00 | 1.42 | -27.00 | -19.50 | 105.03 | 34.35 | 237.25 | 0.6347 | -1063.3 | 999999 | |
| 0.00 | 2.56 | 0.00 | 1.60 | -18.98 | 103.48 | 32.80 | 236.91 | 0.6137 | -175.0 | -301.5 | |
| 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. | |