| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 11.05 | 40.58 | 5.81 | 21.39 | -15.54 | 244.74 | -11.35 | 146.23 | 0.3409 | -130.2 | -22.8 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2011-06-13 15:59:11 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 | 0.80 | -14.71 | 248.06 | -8.04 | 153.16 | 0.3008 | 903.0 | 685.3 | |
| 0.00 | 3.35 | 0.00 | 1.75 | -15.60 | 247.48 | -8.61 | 152.92 | 0.3183 | 823.0 | 711.4 | |
| 5.89 | 8.06 | 3.07 | 4.21 | -14.68 | 246.27 | -9.82 | 148.27 | 0.3150 | 1047.2 | 770.1 | |
| 0.00 | 5.80 | 0.00 | 3.03 | -14.68 | 245.89 | -10.20 | 147.29 | 0.3184 | 883.0 | 692.4 | |
| 0.00 | 0.72 | 0.00 | 0.38 | -14.65 | 245.67 | -10.42 | 146.67 | 0.3200 | 661.0 | 517.9 | |
| 0.00 | 1.00 | 0.00 | 0.52 | -15.22 | 244.64 | -11.45 | 145.22 | 0.3372 | -833.0 | -612.3 | |
| 0.00 | 1.18 | 0.00 | 0.64 | -19.20 | 243.73 | -12.36 | 149.39 | 0.3987 | 732.0 | 631.8 | |
| 0.00 | 1.81 | 0.00 | 0.96 | -15.99 | 243.89 | -12.20 | 144.84 | 0.3544 | -905.0 | -779.1 | |
| 0.00 | 1.00 | 0.00 | 0.53 | -16.18 | 243.62 | -12.48 | 144.58 | 0.3595 | -787.0 | -702.1 | |
| 5.16 | 8.33 | 2.74 | 4.41 | -15.70 | 243.42 | -12.67 | 143.34 | 0.3552 | -1097.2 | -868.3 | |
| 0.00 | 1.45 | 0.00 | 0.77 | -16.63 | 243.10 | -12.99 | 144.24 | 0.3702 | -743.0 | -551.2 | |
| 0.00 | 2.08 | 0.00 | 1.11 | -15.90 | 242.95 | -13.14 | 142.70 | 0.3623 | -894.0 | -720.5 | |
| 0.00 | 1.63 | 0.00 | 0.87 | -15.83 | 242.60 | -13.49 | 141.86 | 0.3650 | -990.0 | -850.2 | |
| 0.00 | 1.45 | 0.00 | 0.77 | -15.80 | 242.44 | -13.65 | 141.48 | 0.3663 | -803.0 | -707.4 | |
| 0.00 | 1.18 | 0.00 | 0.64 | -18.31 | 240.33 | -15.77 | 141.72 | 0.4181 | -704.0 | -490.8 | |
| 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. | |