| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 11.25 | 39.89 | 5.96 | 21.38 | -16.84 | 98.86 | -6.74 | 163.34 | 0.3818 | -11.7 | -73.4 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2014-11-03 07:00:28 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 |
| 8.48 | 13.24 | 4.49 | 7.00 | -16.32 | 103.68 | -1.92 | 174.74 | 0.3528 | 1043.7 | 757.4 | |
| 0.00 | 0.87 | 0.00 | 0.46 | -16.13 | 101.63 | -3.97 | 169.15 | 0.3545 | 829.0 | 601.3 | |
| 2.77 | 8.57 | 1.47 | 4.56 | -16.74 | 100.25 | -5.35 | 165.94 | 0.3691 | 1142.8 | 830.1 | |
| 0.00 | 1.12 | 0.00 | 0.60 | -16.18 | 98.40 | -7.20 | 160.87 | 0.3690 | -699.0 | -534.1 | |
| 0.00 | 0.95 | 0.00 | 0.51 | -17.48 | 96.04 | -9.56 | 156.71 | 0.4022 | -747.0 | -613.1 | |
| 0.00 | 4.15 | 0.00 | 2.24 | -16.75 | 95.77 | -9.83 | 155.32 | 0.3933 | -760.0 | -750.1 | |
| 0.00 | 2.16 | 0.00 | 1.18 | -17.47 | 94.39 | -11.20 | 153.22 | 0.4132 | -728.0 | -635.0 | |
| 0.00 | 1.30 | 0.00 | 0.71 | -18.12 | 94.13 | -11.47 | 153.42 | 0.4241 | -800.0 | -618.1 | |
| 0.00 | 0.69 | 0.00 | 0.38 | -18.06 | 93.72 | -11.88 | 152.54 | 0.4263 | -825.0 | -729.9 | |
| 0.00 | 3.72 | 0.00 | 2.04 | -18.00 | 93.40 | -12.20 | 151.85 | 0.4278 | -605.0 | -545.2 | |
| 0.00 | 0.87 | 0.00 | 0.47 | -17.13 | 93.46 | -12.14 | 150.94 | 0.4154 | -675.0 | -598.1 | |
| 0.00 | 1.04 | 0.00 | 0.55 | -13.47 | 93.49 | -12.10 | 145.91 | 0.3654 | -783.0 | -594.9 | |
| 0.00 | 1.21 | 0.00 | 0.68 | -19.72 | 90.90 | -14.70 | 149.31 | 0.4700 | -771.0 | -563.6 | |
| 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. | |