| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 28.89 | 109.92 | 39.84 | 152.11 | 8.59 | 102.65 | 67.90 | 280.99 | 0.9323 | 287.9 | 116.6 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2014-01-12 18:00:24 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 | 0.76 | 0.00 | 1.63 | 6.13 | 110.70 | 75.95 | 277.36 | 0.9736 | -162.0 | -119.4 | |
| 1.02 | 13.17 | 2.15 | 28.17 | 6.42 | 110.58 | 75.83 | 277.67 | 0.9733 | -350.9 | 40.8 | |
| 3.48 | -2.00 | 7.39 | -2.00 | 6.87 | 110.55 | 75.80 | 278.13 | 0.9733 | 168.5 | 999999 | |
| 0.00 | 6.12 | 0.00 | 9.74 | 7.00 | 105.83 | 71.08 | 278.82 | 0.9515 | -495.0 | -274.4 | |
| 0.00 | 1.36 | 0.00 | 2.37 | 10.35 | 107.13 | 72.38 | 282.12 | 0.9602 | 88.0 | 65.6 | |
| 0.00 | 1.78 | 0.00 | 2.60 | 6.65 | 104.19 | 69.44 | 278.65 | 0.9422 | -492.0 | -300.4 | |
| 1.87 | 3.14 | 2.67 | 4.49 | 8.46 | 103.49 | 68.73 | 280.66 | 0.9395 | 75.5 | -4.1 | |
| 0.00 | 1.95 | 0.00 | 2.54 | 9.26 | 101.18 | 66.43 | 281.86 | 0.9260 | 113.0 | -14.6 | |
| 4.59 | 63.97 | 5.81 | 79.44 | 9.42 | 100.50 | 65.75 | 282.15 | 0.9217 | 135.3 | 172.2 | |
| 0.51 | 1.19 | 0.63 | 1.47 | 8.25 | 100.09 | 65.34 | 280.95 | 0.9178 | 530.0 | 464.8 | |
| 1.53 | 5.61 | 1.87 | 6.89 | 7.94 | 99.92 | 65.17 | 280.64 | 0.9163 | 139.6 | 295.2 | |
| 4.42 | -9.00 | 5.49 | -9.00 | 9.31 | 100.09 | 65.34 | 282.09 | 0.9189 | 482.6 | 999999 | |
| 6.88 | -9.00 | 8.42 | -9.00 | 9.49 | 99.65 | 64.90 | 282.36 | 0.9161 | 695.3 | 999999 | |
| 4.59 | 10.87 | 5.41 | 12.77 | 9.30 | 98.68 | 63.92 | 282.32 | 0.9091 | 606.6 | 504.3 | |
| 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. | |