| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 4.59 | 28.27 | 3.40 | 21.04 | 6.97 | 206.54 | -48.58 | 86.85 | 0.7475 | 55.3 | 211.2 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2014-09-25 16:00:33 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 | 2.03 | 0.00 | 1.44 | 7.15 | 209.21 | -45.92 | 86.78 | 0.7162 | -722.0 | -585.6 | |
| 0.00 | 0.97 | 0.00 | 0.69 | 6.85 | 209.25 | -45.88 | 87.20 | 0.7159 | -636.0 | -554.8 | |
| 0.62 | 1.86 | 0.44 | 1.32 | 6.39 | 209.13 | -46.00 | 87.84 | 0.7177 | -589.9 | -535.5 | |
| 0.00 | 0.88 | 0.00 | 0.63 | 6.53 | 209.02 | -46.10 | 87.63 | 0.7189 | -545.0 | -440.7 | |
| 0.88 | 2.03 | 0.63 | 1.45 | 6.03 | 208.86 | -46.27 | 88.31 | 0.7212 | -540.5 | -409.6 | |
| 0.00 | 1.15 | 0.00 | 0.83 | 7.09 | 208.16 | -46.97 | 86.79 | 0.7289 | -638.0 | -523.1 | |
| 0.00 | 1.06 | 0.00 | 0.80 | 6.54 | 206.00 | -49.13 | 87.38 | 0.7543 | 539.0 | 489.9 | |
| 1.68 | 12.54 | 1.26 | 9.48 | 6.80 | 205.92 | -49.21 | 87.02 | 0.7551 | 762.3 | 613.7 | |
| 1.41 | -8.00 | 1.07 | -8.00 | 7.04 | 205.51 | -49.61 | 86.68 | 0.7595 | 719.9 | 999999 | |
| 0.00 | 1.86 | 0.00 | 1.41 | 6.90 | 205.30 | -49.83 | 86.85 | 0.7621 | 329.0 | 292.9 | |
| 0.00 | 1.06 | 0.00 | 0.81 | 7.24 | 205.06 | -50.07 | 86.38 | 0.7645 | 488.0 | 398.9 | |
| 0.00 | 1.24 | 0.00 | 0.95 | 8.57 | 204.69 | -50.43 | 84.62 | 0.7679 | 579.0 | 520.4 | |
| 0.00 | 0.62 | 0.00 | 0.48 | 8.70 | 204.52 | -50.60 | 84.44 | 0.7697 | 369.0 | 303.4 | |
| 0.00 | 0.97 | 0.00 | 0.75 | 7.76 | 204.45 | -50.68 | 85.67 | 0.7710 | 493.0 | 407.8 | |
| 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. | |