| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 21.70 | 56.00 | 11.25 | 29.20 | -4.33 | 31.10 | -14.12 | 128.03 | 0.3100 | 507.0 | 372.8 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2014-08-18 01:00:38 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 |
| 19.00 | 40.07 | 9.85 | 20.80 | -4.17 | 31.97 | -13.25 | 129.27 | 0.2966 | 1122.2 | 683.1 | |
| 2.70 | -1.00 | 1.40 | -1.00 | -4.58 | 31.90 | -13.32 | 130.15 | 0.3018 | 869.2 | 999999 | |
| 0.00 | 0.27 | 0.00 | 0.14 | -5.64 | 31.53 | -13.69 | 131.96 | 0.3181 | 665.0 | 610.7 | |
| 0.00 | 0.27 | 0.00 | 0.14 | -7.23 | 30.35 | -14.87 | 133.10 | 0.3502 | 8.0 | 7.0 | |
| 0.00 | 2.07 | 0.00 | 1.08 | -3.85 | 30.29 | -14.94 | 125.06 | 0.3156 | 853.0 | 773.7 | |
| 0.00 | 1.08 | 0.00 | 0.57 | -5.90 | 30.05 | -15.18 | 129.60 | 0.3394 | -837.0 | -587.2 | |
| 0.00 | 3.15 | 0.00 | 1.65 | -4.04 | 30.06 | -15.16 | 125.15 | 0.3204 | 910.0 | 788.9 | |
| 0.00 | 0.81 | 0.00 | 0.42 | -3.96 | 29.81 | -15.41 | 124.48 | 0.3230 | 643.0 | 558.4 | |
| 0.00 | 1.98 | 0.00 | 1.05 | -5.58 | 29.33 | -15.90 | 127.56 | 0.3453 | -887.0 | -799.3 | |
| 0.00 | 0.99 | 0.00 | 0.52 | -5.49 | 29.24 | -15.99 | 127.19 | 0.3456 | -762.0 | -741.5 | |
| 0.00 | 2.16 | 0.00 | 1.14 | -5.34 | 28.99 | -16.24 | 126.41 | 0.3474 | -906.0 | -653.9 | |
| 0.00 | 1.17 | 0.00 | 0.62 | -6.41 | 27.71 | -17.52 | 126.69 | 0.3746 | 574.0 | 407.8 | |
| 0.00 | 1.26 | 0.00 | 0.67 | 0.05 | 25.91 | -19.31 | 108.48 | 0.3502 | 5.0 | 2.1 | |
| 0.00 | 0.72 | 0.00 | 0.40 | -5.40 | 22.84 | -22.38 | 118.06 | 0.4314 | -750.0 | -613.6 | |
| 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. | |