| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 46.45 | 128.69 | 35.07 | 97.71 | 7.00 | 210.18 | 49.64 | 273.52 | 0.7595 | 23.6 | -11.9 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2014-10-02 20:00:32 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 |
| 5.37 | 34.57 | 4.28 | 27.61 | 7.49 | 212.62 | 52.08 | 274.31 | 0.7866 | -790.1 | -305.8 | |
| 14.43 | 24.89 | 11.33 | 19.52 | 7.20 | 211.84 | 51.30 | 273.89 | 0.7783 | -822.5 | -503.3 | |
| 0.00 | 1.32 | 0.00 | 1.02 | 6.83 | 210.96 | 50.42 | 273.35 | 0.7689 | -260.0 | -394.6 | |
| 0.79 | 2.55 | 0.60 | 1.94 | 6.14 | 210.21 | 49.66 | 272.40 | 0.7609 | -513.8 | -475.0 | |
| 0.00 | 0.88 | 0.00 | 0.65 | 7.29 | 209.20 | 48.66 | 273.85 | 0.7488 | 263.0 | 293.7 | |
| 1.23 | 31.76 | 0.91 | 23.33 | 6.72 | 208.80 | 48.26 | 273.06 | 0.7444 | 321.9 | 296.7 | |
| 2.29 | -6.00 | 1.68 | -6.00 | 6.83 | 208.59 | 48.05 | 273.19 | 0.7419 | -214.3 | 999999 | |
| 8.36 | -6.00 | 6.14 | -6.00 | 6.47 | 208.50 | 47.96 | 272.71 | 0.7410 | 670.7 | 999999 | |
| 2.90 | 25.07 | 2.11 | 18.16 | 6.77 | 207.82 | 47.27 | 273.07 | 0.7329 | 816.7 | 587.7 | |
| 0.00 | 1.23 | 0.00 | 0.89 | 7.26 | 207.79 | 47.25 | 273.73 | 0.7323 | 333.0 | 359.9 | |
| 7.65 | -9.00 | 5.54 | -9.00 | 6.81 | 207.69 | 47.15 | 273.12 | 0.7313 | 799.9 | 999999 | |
| 0.00 | 2.55 | 0.00 | 1.84 | 6.10 | 207.60 | 47.06 | 272.13 | 0.7307 | 361.0 | 377.2 | |
| 3.43 | -9.00 | 2.48 | -9.00 | 6.59 | 207.53 | 46.98 | 272.80 | 0.7295 | 791.1 | 999999 | |
| 0.00 | 2.81 | 0.00 | 2.01 | 7.19 | 206.85 | 46.31 | 273.58 | 0.7211 | 586.0 | 481.0 | |
| 0.00 | 1.06 | 0.00 | 0.74 | 7.35 | 206.31 | 45.76 | 273.78 | 0.7144 | 526.0 | 430.7 | |
| 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. | |