| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 17.92 | 42.98 | 16.79 | 40.34 | 16.87 | 46.01 | -55.03 | 67.24 | 0.8524 | -185.2 | -109.0 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2011-05-01 22:59:07 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 |
| 4.64 | 7.40 | 4.25 | 6.78 | 18.00 | 47.39 | -53.66 | 65.51 | 0.8438 | -485.4 | -209.6 | |
| 1.16 | 2.14 | 1.05 | 1.94 | 17.15 | 47.59 | -53.45 | 66.41 | 0.8397 | -417.2 | -499.0 | |
| 0.00 | 1.07 | 0.00 | 1.00 | 18.26 | 46.89 | -54.15 | 65.39 | 0.8488 | -159.0 | -110.5 | |
| 7.85 | 19.53 | 7.28 | 17.99 | 16.35 | 46.47 | -54.57 | 67.69 | 0.8473 | -537.8 | -399.8 | |
| 0.62 | -4.00 | 0.59 | -4.00 | 16.60 | 46.09 | -54.95 | 67.52 | 0.8511 | -192.6 | 999999 | |
| 1.96 | 3.75 | 1.86 | 3.55 | 16.44 | 45.60 | -55.44 | 67.86 | 0.8548 | -381.7 | -249.9 | |
| 0.00 | 3.30 | 0.00 | 3.24 | 17.15 | 44.55 | -56.50 | 67.38 | 0.8652 | 441.0 | 463.6 | |
| 0.00 | 0.89 | 0.00 | 0.87 | 15.97 | 44.39 | -56.65 | 68.74 | 0.8638 | 437.0 | 471.8 | |
| 0.00 | 0.45 | 0.00 | 0.44 | 16.14 | 44.14 | -56.91 | 68.62 | 0.8662 | 453.0 | 416.0 | |
| 0.00 | 0.62 | 0.00 | 0.62 | 16.84 | 43.76 | -57.29 | 67.95 | 0.8708 | 288.0 | 371.0 | |
| 0.00 | 0.62 | 0.00 | 0.61 | 15.70 | 44.16 | -56.88 | 69.11 | 0.8650 | 364.0 | 301.4 | |
| 0.00 | 0.89 | 0.00 | 0.90 | 16.93 | 43.36 | -57.68 | 67.96 | 0.8742 | 397.0 | 290.4 | |
| 1.69 | 2.32 | 1.76 | 2.40 | 17.55 | 42.75 | -58.29 | 67.45 | 0.8802 | 348.1 | 330.1 | |
| 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. | |