| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 24.00 | 141.89 | 32.46 | 193.78 | -13.55 | 230.52 | -68.78 | 103.24 | 0.9278 | 383.4 | 142.7 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2014-05-09 05:00:37 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 | 1.70 | 0.00 | 1.73 | -12.73 | 238.55 | -60.75 | 102.73 | 0.8745 | 124.0 | 195.8 | |
| 0.00 | 1.43 | 0.00 | 1.42 | -10.23 | 239.08 | -60.22 | 99.89 | 0.8690 | 554.0 | 488.9 | |
| 0.00 | 0.81 | 0.00 | 0.83 | -10.14 | 237.97 | -61.34 | 99.74 | 0.8784 | 267.0 | 245.4 | |
| 15.05 | 98.98 | 17.08 | 113.04 | -11.68 | 235.06 | -64.24 | 101.38 | 0.9015 | 803.4 | 268.4 | |
| 1.97 | -4.00 | 2.29 | -4.00 | -11.47 | 234.43 | -64.88 | 101.11 | 0.9060 | 331.7 | 999999 | |
| 1.16 | -4.00 | 1.35 | -4.00 | -11.22 | 234.46 | -64.84 | 100.84 | 0.9058 | 328.1 | 999999 | |
| 0.00 | 1.43 | 0.00 | 1.74 | -11.31 | 233.14 | -66.16 | 100.90 | 0.9151 | -84.0 | -99.4 | |
| 0.00 | 0.90 | 0.00 | 1.07 | -7.71 | 233.68 | -65.63 | 96.96 | 0.9111 | 124.0 | 130.6 | |
| 0.00 | 0.27 | 0.00 | 0.45 | -14.28 | 226.12 | -73.18 | 103.92 | 0.9570 | 174.0 | 201.7 | |
| 0.00 | 0.27 | 0.00 | 0.49 | -15.67 | 224.69 | -74.62 | 105.35 | 0.9639 | -120.0 | -109.3 | |
| 5.28 | 30.45 | 10.76 | 62.62 | -17.06 | 222.95 | -76.36 | 106.76 | 0.9713 | 138.4 | -12.3 | |
| 0.00 | 2.87 | 0.00 | 5.30 | -15.48 | 224.53 | -74.78 | 105.15 | 0.9646 | -280.0 | -196.8 | |
| 0.54 | 2.24 | 0.98 | 4.09 | -15.08 | 224.69 | -74.61 | 104.73 | 0.9638 | -322.2 | -324.3 | |
| 0.00 | 0.27 | 0.00 | 0.45 | -11.09 | 226.25 | -73.05 | 100.58 | 0.9563 | -251.0 | -266.3 | |
| 0.00 | 0.27 | 0.00 | 0.55 | -14.04 | 222.95 | -76.35 | 103.65 | 0.9712 | -329.0 | -357.0 | |
| 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. | |