| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 26.14 | 107.37 | 18.52 | 76.45 | -4.75 | 84.12 | -45.12 | 100.89 | 0.7212 | 335.0 | 278.3 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2014-11-01 12:00:28 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 |
| 0.00 | 0.95 | 0.00 | 0.65 | -4.58 | 86.82 | -42.42 | 101.38 | 0.6882 | 579.0 | 444.3 | |
| 0.00 | 1.04 | 0.00 | 0.72 | -6.39 | 86.25 | -42.99 | 103.76 | 0.7000 | -621.0 | -493.1 | |
| 0.00 | 1.04 | 0.00 | 0.72 | -5.40 | 86.02 | -43.22 | 102.31 | 0.7002 | -521.0 | -533.0 | |
| 0.00 | 1.30 | 0.00 | 0.91 | -6.15 | 85.61 | -43.62 | 103.23 | 0.7070 | -668.0 | -551.5 | |
| 0.00 | 1.21 | 0.00 | 0.85 | -5.92 | 85.39 | -43.85 | 102.84 | 0.7091 | -502.0 | -335.2 | |
| 0.00 | 0.87 | 0.00 | 0.61 | -4.66 | 85.17 | -44.07 | 101.04 | 0.7086 | 574.0 | 508.2 | |
| 0.00 | 0.95 | 0.00 | 0.67 | -6.10 | 84.83 | -44.41 | 102.93 | 0.7163 | 287.0 | 241.6 | |
| 4.41 | 18.87 | 3.12 | 13.30 | -5.62 | 84.79 | -44.45 | 102.26 | 0.7155 | 534.1 | -35.9 | |
| 8.57 | 66.31 | 6.05 | 46.90 | -4.30 | 84.57 | -44.67 | 100.39 | 0.7151 | 991.8 | 546.0 | |
| 2.94 | -9.00 | 2.08 | -9.00 | -4.73 | 84.54 | -44.70 | 100.96 | 0.7164 | 683.0 | 999999 | |
| 4.33 | -9.00 | 3.07 | -9.00 | -4.14 | 84.33 | -44.91 | 100.10 | 0.7176 | 753.1 | 999999 | |
| 0.00 | 1.04 | 0.00 | 0.74 | -5.11 | 84.21 | -45.03 | 101.39 | 0.7212 | 537.0 | 358.8 | |
| 0.00 | 1.04 | 0.00 | 0.74 | -5.57 | 83.95 | -45.29 | 101.96 | 0.7254 | 408.0 | 312.1 | |
| 0.95 | -9.00 | 0.68 | -9.00 | -4.21 | 84.03 | -45.21 | 100.13 | 0.7213 | 440.6 | 999999 | |
| 0.35 | 3.64 | 0.25 | 2.61 | -4.91 | 83.93 | -45.31 | 101.05 | 0.7241 | 478.8 | 368.9 | |
| 4.59 | -9.00 | 3.27 | -9.00 | -3.83 | 83.97 | -45.27 | 99.58 | 0.7212 | 669.4 | 999999 | |
| 0.00 | 2.34 | 0.00 | 1.68 | -4.05 | 83.66 | -45.58 | 99.82 | 0.7254 | 367.0 | 283.1 | |
| 0.00 | 0.61 | 0.00 | 0.45 | -4.81 | 81.89 | -47.34 | 100.42 | 0.7475 | -571.0 | -457.7 | |
| 0.00 | 1.13 | 0.00 | 0.84 | -5.31 | 81.58 | -47.66 | 101.00 | 0.7521 | 536.0 | 353.5 | |
| 0.00 | 1.82 | 0.00 | 1.46 | -6.45 | 78.49 | -50.75 | 101.72 | 0.7881 | -625.0 | -553.7 | |
| 0.00 | 0.35 | 0.00 | 0.28 | -6.64 | 78.42 | -50.82 | 101.94 | 0.7893 | -422.0 | -490.5 | |
| 0.00 | 1.13 | 0.00 | 0.90 | -6.28 | 78.37 | -50.87 | 101.48 | 0.7890 | -644.0 | -492.5 | |
| 0.00 | 0.95 | 0.00 | 0.76 | -6.16 | 78.34 | -50.90 | 101.32 | 0.7891 | -533.0 | -510.3 | |
| 0.00 | 0.78 | 0.00 | 0.66 | -8.90 | 76.65 | -52.59 | 104.28 | 0.8119 | -432.0 | -373.4 | |
| 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. | |