| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 21.13 | 65.66 | 11.16 | 34.86 | 24.12 | 79.39 | -8.96 | 23.22 | 0.3590 | -663.6 | -421.3 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2011-07-23 12:59:11 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 |
| 8.80 | 45.71 | 4.64 | 24.15 | 23.66 | 80.73 | -7.62 | 20.81 | 0.3434 | -1025.2 | -458.9 | |
| 12.33 | -1.00 | 6.52 | -1.00 | 23.85 | 80.21 | -8.14 | 21.85 | 0.3493 | -1092.6 | 999999 | |
| 0.00 | 2.54 | 0.00 | 1.34 | 23.94 | 79.70 | -8.65 | 22.96 | 0.3539 | -833.0 | -681.0 | |
| 0.00 | 4.17 | 0.00 | 2.21 | 23.61 | 78.75 | -9.60 | 25.59 | 0.3554 | -1065.0 | -803.8 | |
| 0.00 | 1.27 | 0.00 | 0.68 | 25.40 | 77.61 | -10.73 | 25.75 | 0.3890 | -781.0 | -719.1 | |
| 0.00 | 1.00 | 0.00 | 0.53 | 24.98 | 77.55 | -10.80 | 26.41 | 0.3835 | -893.0 | -732.8 | |
| 0.00 | 1.90 | 0.00 | 1.02 | 25.27 | 77.38 | -10.96 | 26.38 | 0.3887 | -699.0 | -562.8 | |
| 0.00 | 1.36 | 0.00 | 0.73 | 25.62 | 77.32 | -11.03 | 26.07 | 0.3942 | -645.0 | -514.5 | |
| 0.00 | 2.90 | 0.00 | 1.55 | 24.32 | 77.30 | -11.05 | 27.79 | 0.3762 | -840.0 | -705.5 | |
| 0.00 | 1.18 | 0.00 | 0.65 | 26.71 | 74.17 | -14.18 | 30.51 | 0.4327 | 738.0 | 612.4 | |
| 0.00 | 1.18 | 0.00 | 0.65 | 26.44 | 73.82 | -14.53 | 31.47 | 0.4321 | 882.0 | 708.3 | |
| 0.00 | 1.18 | 0.00 | 0.65 | 26.40 | 73.47 | -14.87 | 32.10 | 0.4344 | 619.0 | 562.5 | |
| 0.00 | 1.27 | 0.00 | 0.70 | 25.84 | 73.27 | -15.08 | 33.23 | 0.4291 | 692.0 | 542.9 | |
| 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. | |