| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 22.02 | 109.39 | 31.15 | 156.58 | -16.49 | 64.31 | -66.24 | 110.65 | 0.9385 | 167.4 | 43.9 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2014-09-07 20:00:36 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 |
| 16.67 | 76.50 | 22.09 | 101.54 | -16.58 | 66.05 | -64.50 | 111.18 | 0.9293 | 538.8 | 122.5 | |
| 0.00 | 2.67 | 0.00 | 3.86 | -17.02 | 64.22 | -66.33 | 111.16 | 0.9405 | 129.0 | 25.3 | |
| 0.00 | 1.52 | 0.00 | 2.17 | -16.14 | 64.04 | -66.51 | 110.20 | 0.9402 | 226.0 | 117.6 | |
| 0.00 | 0.98 | 0.00 | 1.48 | -16.86 | 63.12 | -67.43 | 110.71 | 0.9462 | -151.0 | -85.3 | |
| 0.00 | 0.71 | 0.00 | 1.07 | -16.59 | 63.23 | -67.31 | 110.46 | 0.9452 | -12.0 | 28.9 | |
| 0.00 | 0.71 | 0.00 | 1.20 | -16.43 | 60.83 | -69.72 | 109.72 | 0.9571 | -519.0 | -483.0 | |
| 0.00 | 1.96 | 0.00 | 3.41 | -16.68 | 60.34 | -70.21 | 109.87 | 0.9596 | -282.0 | -166.7 | |
| 0.00 | 0.80 | 0.00 | 1.47 | -17.59 | 59.53 | -71.02 | 110.61 | 0.9642 | -183.0 | -188.8 | |
| 4.64 | 23.54 | 7.81 | 40.38 | -16.12 | 60.71 | -69.84 | 109.38 | 0.9573 | -617.2 | -97.3 | |
| 0.71 | -9.00 | 1.25 | -9.00 | -16.45 | 60.16 | -70.39 | 109.59 | 0.9602 | 76.2 | 999999 | |
| 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. | |