| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 95.94 | 432.29 | 122.22 | 554.29 | -20.68 | 36.81 | -66.05 | 112.05 | 0.9226 | 112.8 | -42.0 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2011-05-29 00:59:10 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 |
| 2.26 | 202.71 | 2.51 | 229.54 | -20.18 | 40.68 | -62.17 | 112.08 | 0.8975 | 740.7 | 273.4 | |
| 19.95 | -1.00 | 22.32 | -1.00 | -19.69 | 40.46 | -62.39 | 111.50 | 0.8985 | 837.0 | 999999 | |
| 10.02 | -1.00 | 11.51 | -1.00 | -20.07 | 39.77 | -63.09 | 111.80 | 0.9039 | 533.8 | 999999 | |
| 1.71 | 3.34 | 2.09 | 4.06 | -21.80 | 38.41 | -64.44 | 113.48 | 0.9149 | 415.1 | 389.7 | |
| 5.32 | -1.00 | 6.24 | -1.00 | -20.61 | 39.22 | -63.64 | 112.31 | 0.9082 | 496.6 | 999999 | |
| 4.15 | 6.41 | 5.14 | 7.94 | -22.12 | 37.98 | -64.88 | 113.75 | 0.9180 | 389.3 | 239.0 | |
| 6.50 | 26.80 | 7.93 | 33.06 | -21.38 | 38.23 | -64.62 | 112.99 | 0.9156 | 542.9 | -169.2 | |
| 3.79 | -1.00 | 4.45 | -1.00 | -20.19 | 39.17 | -63.68 | 111.84 | 0.9081 | 380.2 | 999999 | |
| 0.00 | 0.99 | 0.00 | 1.27 | -22.37 | 37.20 | -65.66 | 113.90 | 0.9232 | -261.0 | -215.3 | |
| 2.35 | -7.00 | 2.91 | -7.00 | -21.53 | 37.87 | -64.99 | 113.10 | 0.9181 | 305.5 | 999999 | |
| 2.62 | 9.48 | 3.34 | 12.23 | -21.88 | 37.08 | -65.77 | 113.36 | 0.9234 | 187.9 | -251.0 | |
| 0.00 | 3.25 | 0.00 | 4.11 | -21.56 | 37.29 | -65.56 | 113.04 | 0.9218 | 223.0 | 39.4 | |
| 0.00 | 1.26 | 0.00 | 1.57 | -20.36 | 37.59 | -65.26 | 111.79 | 0.9187 | -487.0 | -441.9 | |
| 0.00 | 0.81 | 0.00 | 1.00 | -19.91 | 37.80 | -65.06 | 111.33 | 0.9169 | -190.0 | -182.7 | |
| 0.81 | 10.74 | 1.05 | 13.77 | -21.06 | 36.60 | -66.25 | 112.40 | 0.9256 | -479.3 | -529.5 | |
| 2.44 | -15.00 | 3.15 | -15.00 | -20.86 | 36.61 | -66.24 | 112.20 | 0.9253 | -460.2 | 999999 | |
| 0.00 | 0.99 | 0.00 | 1.36 | -21.95 | 35.35 | -67.51 | 113.19 | 0.9338 | -643.0 | -532.2 | |
| 0.90 | 2.44 | 1.18 | 3.19 | -20.66 | 36.29 | -66.56 | 111.94 | 0.9271 | -437.3 | -318.0 | |
| 0.00 | 1.71 | 0.00 | 2.30 | -20.78 | 35.68 | -67.17 | 111.99 | 0.9309 | -521.0 | -421.0 | |
| 0.00 | 0.36 | 0.00 | 0.49 | -20.94 | 35.20 | -67.66 | 112.09 | 0.9338 | -244.0 | -193.8 | |
| 1.71 | 15.52 | 2.63 | 23.86 | -23.00 | 32.84 | -70.01 | 113.97 | 0.9481 | -569.7 | -369.1 | |
| 0.00 | 0.90 | 0.00 | 1.22 | -20.36 | 35.56 | -67.30 | 111.52 | 0.9313 | -668.0 | -649.0 | |
| 0.00 | 0.45 | 0.00 | 0.61 | -20.58 | 35.35 | -67.50 | 111.73 | 0.9326 | -559.0 | -564.0 | |
| 11.10 | 110.20 | 15.21 | 157.67 | -20.16 | 35.05 | -67.80 | 111.24 | 0.9341 | -570.2 | -375.3 | |
| 0.00 | 1.35 | 0.00 | 2.05 | -22.01 | 33.09 | -69.76 | 112.97 | 0.9462 | -529.0 | -390.6 | |
| 1.81 | -24.00 | 2.59 | -24.00 | -20.89 | 34.09 | -68.76 | 111.90 | 0.9400 | 228.2 | 999999 | |
| 2.80 | -24.00 | 4.02 | -24.00 | -20.76 | 34.04 | -68.81 | 111.76 | 0.9402 | -573.1 | 999999 | |
| 5.23 | -24.00 | 7.50 | -24.00 | -20.43 | 34.08 | -68.77 | 111.42 | 0.9398 | -544.6 | 999999 | |
| 1.81 | 32.58 | 2.91 | 52.99 | -22.12 | 31.78 | -71.08 | 112.94 | 0.9529 | -362.5 | -4.9 | |
| 1.62 | -29.00 | 2.64 | -29.00 | -22.12 | 31.58 | -71.28 | 112.91 | 0.9539 | 271.4 | 999999 | |
| 3.61 | -24.00 | 5.44 | -24.00 | -20.61 | 32.98 | -69.88 | 111.48 | 0.9459 | -462.0 | 999999 | |
| 1.53 | -29.00 | 2.51 | -29.00 | -21.86 | 31.48 | -71.38 | 112.63 | 0.9542 | 453.9 | 999999 | |
| 1.90 | -24.00 | 2.95 | -24.00 | -20.99 | 32.38 | -70.48 | 111.82 | 0.9492 | -415.2 | 999999 | |
| 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. | |