| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 59.58 | 225.33 | 48.63 | 186.99 | -12.05 | 164.57 | 50.21 | 249.68 | 0.8027 | 138.1 | 108.6 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2014-10-06 08:00:32 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 |
| 0.97 | 145.78 | 0.84 | 125.68 | -12.29 | 166.66 | 52.30 | 250.18 | 0.8239 | -44.7 | 174.3 | |
| 2.37 | -1.00 | 2.05 | -1.00 | -11.96 | 166.47 | 52.11 | 250.50 | 0.8212 | 529.2 | 999999 | |
| 10.98 | -1.00 | 9.47 | -1.00 | -12.20 | 166.33 | 51.97 | 250.18 | 0.8206 | 791.7 | 999999 | |
| 6.33 | -1.00 | 5.41 | -1.00 | -11.83 | 166.08 | 51.72 | 250.52 | 0.8172 | 886.7 | 999999 | |
| 10.46 | -1.00 | 8.99 | -1.00 | -12.52 | 166.13 | 51.76 | 249.72 | 0.8196 | 919.9 | 999999 | |
| 1.58 | 3.25 | 1.32 | 2.72 | -11.75 | 165.18 | 50.81 | 250.30 | 0.8083 | 651.1 | 490.3 | |
| 0.00 | 1.85 | 0.00 | 1.53 | -11.40 | 164.80 | 50.44 | 250.57 | 0.8035 | 597.0 | 520.2 | |
| 0.00 | 2.64 | 0.00 | 2.19 | -12.22 | 164.81 | 50.45 | 249.61 | 0.8062 | 627.0 | 454.4 | |
| 0.00 | 0.53 | 0.00 | 0.43 | -11.33 | 164.35 | 49.99 | 250.50 | 0.7989 | 619.0 | 564.2 | |
| 0.00 | 0.26 | 0.00 | 0.22 | -12.80 | 164.63 | 50.27 | 248.85 | 0.8063 | 193.0 | 269.0 | |
| 0.00 | 1.05 | 0.00 | 0.87 | -11.74 | 164.35 | 49.99 | 250.01 | 0.8002 | 398.0 | 444.8 | |
| 0.00 | 0.97 | 0.00 | 0.79 | -11.51 | 163.96 | 49.60 | 250.13 | 0.7957 | 649.0 | 588.9 | |
| 0.00 | 0.97 | 0.00 | 0.78 | -11.19 | 163.79 | 49.43 | 250.47 | 0.7929 | 682.0 | 504.5 | |
| 0.88 | 1.76 | 0.72 | 1.44 | -13.73 | 163.41 | 49.04 | 247.27 | 0.7976 | -420.9 | -312.4 | |
| 1.93 | 3.95 | 1.54 | 3.14 | -12.05 | 162.59 | 48.23 | 248.96 | 0.7838 | 647.0 | 541.3 | |
| 0.00 | 1.23 | 0.00 | 0.97 | -11.56 | 162.34 | 47.98 | 249.46 | 0.7795 | 587.0 | 530.6 | |
| 1.41 | 2.99 | 1.10 | 2.34 | -11.23 | 162.18 | 47.81 | 249.79 | 0.7767 | -439.0 | -302.7 | |
| 0.00 | 4.66 | 0.00 | 3.62 | -11.39 | 161.80 | 47.44 | 249.45 | 0.7734 | 564.0 | 521.0 | |
| 2.90 | 4.92 | 2.23 | 3.79 | -10.92 | 161.47 | 47.11 | 249.90 | 0.7684 | -574.1 | -381.1 | |
| 0.00 | 0.79 | 0.00 | 0.61 | -11.55 | 161.56 | 47.20 | 249.15 | 0.7715 | 484.0 | 395.1 | |
| 0.00 | 0.88 | 0.00 | 0.68 | -11.65 | 161.59 | 47.22 | 249.04 | 0.7721 | 594.0 | 465.1 | |
| 2.11 | 3.51 | 1.61 | 2.69 | -10.95 | 161.08 | 46.71 | 249.70 | 0.7643 | -753.0 | -631.4 | |
| 16.78 | 27.07 | 12.70 | 20.50 | -11.27 | 160.38 | 46.02 | 249.02 | 0.7581 | -795.3 | -337.8 | |
| 0.00 | 0.97 | 0.00 | 0.74 | -12.28 | 160.56 | 46.20 | 247.83 | 0.7638 | -313.0 | -202.7 | |
| 0.00 | 1.67 | 0.00 | 1.26 | -11.74 | 160.09 | 45.72 | 248.30 | 0.7568 | -550.0 | -315.4 | |
| 0.00 | 1.23 | 0.00 | 0.92 | -11.72 | 159.77 | 45.41 | 248.20 | 0.7534 | -311.0 | -349.0 | |
| 0.00 | 1.23 | 0.00 | 0.94 | -14.37 | 159.74 | 45.37 | 244.90 | 0.7636 | -470.0 | -340.1 | |
| 0.00 | 0.62 | 0.00 | 0.46 | -13.97 | 159.20 | 44.83 | 245.13 | 0.7564 | -319.0 | -325.9 | |
| 0.00 | 1.14 | 0.00 | 0.84 | -12.15 | 158.18 | 43.82 | 246.93 | 0.7380 | -698.0 | -593.2 | |
| 0.00 | 0.88 | 0.00 | 0.65 | -13.21 | 158.36 | 44.00 | 245.68 | 0.7445 | -646.0 | -580.6 | |
| 0.88 | 2.64 | 0.65 | 1.95 | -13.65 | 158.04 | 43.68 | 244.96 | 0.7430 | -698.9 | -553.3 | |
| 0.00 | 0.53 | 0.00 | 0.38 | -12.43 | 157.73 | 43.36 | 246.36 | 0.7343 | -443.0 | -369.0 | |
| 0.00 | 2.81 | 0.00 | 2.03 | -12.22 | 157.47 | 43.11 | 246.50 | 0.7306 | -803.0 | -636.8 | |
| 0.00 | 1.93 | 0.00 | 1.40 | -12.58 | 157.34 | 42.97 | 245.97 | 0.7307 | -779.0 | -699.3 | |
| 0.00 | 0.62 | 0.00 | 0.43 | -12.38 | 155.55 | 41.19 | 245.32 | 0.7102 | -544.0 | -502.3 | |
| 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. | |