| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 17.50 | 50.90 | 10.37 | 30.02 | -8.41 | 9.12 | -33.04 | 95.67 | 0.5439 | 569.1 | 479.6 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2014-04-04 04:00:32 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 | 1.14 | 0.00 | 0.65 | -8.85 | 12.98 | -29.17 | 96.75 | 0.4870 | 669.0 | 473.8 | |
| 0.00 | 1.67 | 0.00 | 0.95 | -8.74 | 12.54 | -29.62 | 96.47 | 0.4936 | 785.0 | 667.6 | |
| 0.00 | 1.58 | 0.00 | 0.91 | -5.87 | 11.74 | -30.42 | 90.71 | 0.5057 | 743.0 | 614.4 | |
| 6.77 | 8.97 | 3.93 | 5.21 | -8.35 | 10.49 | -31.67 | 95.57 | 0.5239 | 955.4 | 579.7 | |
| 0.00 | 1.05 | 0.00 | 0.61 | -8.69 | 10.17 | -31.98 | 96.21 | 0.5288 | 599.0 | 450.6 | |
| 3.34 | 23.39 | 1.96 | 13.72 | -8.54 | 9.76 | -32.40 | 95.91 | 0.5348 | 985.3 | 612.5 | |
| 0.62 | -6.00 | 0.36 | -6.00 | -8.80 | 9.52 | -32.64 | 96.38 | 0.5385 | 926.4 | 999999 | |
| 3.25 | -6.00 | 1.91 | -6.00 | -8.94 | 9.29 | -32.87 | 96.62 | 0.5419 | 797.6 | 999999 | |
| 0.00 | 0.97 | 0.00 | 0.57 | -7.16 | 9.27 | -32.89 | 93.33 | 0.5418 | 715.0 | 637.0 | |
| 0.00 | 1.49 | 0.00 | 0.88 | -10.81 | 8.85 | -33.31 | 100.01 | 0.5499 | 651.0 | 527.2 | |
| 0.00 | 0.97 | 0.00 | 0.57 | -8.64 | 8.88 | -33.28 | 96.05 | 0.5477 | 789.0 | 585.3 | |
| 0.00 | 2.46 | 0.00 | 1.46 | -8.04 | 8.83 | -33.33 | 94.94 | 0.5482 | 671.0 | 488.1 | |
| 0.00 | 0.88 | 0.00 | 0.52 | -9.00 | 8.37 | -33.79 | 96.67 | 0.5552 | 467.0 | 414.7 | |
| 3.52 | 5.45 | 2.21 | 3.42 | -7.57 | 3.94 | -38.22 | 94.13 | 0.6171 | -822.5 | -604.1 | |
| 0.00 | 0.88 | 0.00 | 0.55 | -6.34 | 4.02 | -38.14 | 92.13 | 0.6165 | -578.0 | -467.4 | |
| 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. | |