| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 80.29 | 340.22 | 61.15 | 256.49 | 19.54 | 192.19 | -46.53 | 65.19 | 0.7542 | -235.8 | -111.2 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2011-11-25 11:58:57 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 |
| 2.57 | 203.99 | 1.85 | 146.43 | 19.11 | 194.69 | -44.03 | 64.87 | 0.7278 | -709.5 | -369.2 | |
| 10.10 | -1.00 | 7.24 | -1.00 | 18.74 | 194.77 | -43.95 | 65.34 | 0.7256 | -982.9 | 999999 | |
| 23.28 | -1.00 | 16.74 | -1.00 | 18.33 | 194.51 | -44.21 | 65.97 | 0.7271 | -988.5 | 999999 | |
| 3.77 | 19.95 | 2.77 | 14.69 | 19.12 | 193.45 | -45.27 | 65.31 | 0.7412 | -596.0 | -394.0 | |
| 0.00 | 0.60 | 0.00 | 0.44 | 19.52 | 193.08 | -45.64 | 64.93 | 0.7463 | -426.0 | -381.6 | |
| 3.34 | -4.00 | 2.45 | -4.00 | 18.65 | 193.34 | -45.38 | 65.96 | 0.7408 | -614.4 | 999999 | |
| 0.60 | -4.00 | 0.44 | -4.00 | 19.14 | 193.13 | -45.60 | 65.39 | 0.7447 | -379.7 | 999999 | |
| 4.97 | -4.00 | 3.66 | -4.00 | 18.86 | 193.14 | -45.59 | 65.75 | 0.7437 | -569.5 | 999999 | |
| 0.00 | 1.46 | 0.00 | 1.08 | 19.20 | 192.66 | -46.07 | 65.49 | 0.7498 | -421.0 | -254.0 | |
| 0.00 | 0.60 | 0.00 | 0.45 | 19.48 | 192.55 | -46.17 | 65.16 | 0.7518 | -442.0 | -358.1 | |
| 0.00 | 1.11 | 0.00 | 0.84 | 19.54 | 192.39 | -46.33 | 65.14 | 0.7536 | -383.0 | -424.2 | |
| 2.91 | 7.19 | 2.16 | 5.35 | 18.58 | 192.65 | -46.07 | 66.29 | 0.7479 | -430.8 | -95.4 | |
| 0.00 | 0.51 | 0.00 | 0.39 | 19.47 | 192.24 | -46.49 | 65.28 | 0.7551 | -393.0 | -331.3 | |
| 1.37 | 1.97 | 1.04 | 1.50 | 19.93 | 191.78 | -46.94 | 64.84 | 0.7612 | -302.5 | -233.3 | |
| 0.00 | 0.77 | 0.00 | 0.58 | 19.28 | 192.03 | -46.69 | 65.59 | 0.7566 | -308.0 | -211.4 | |
| 0.00 | 1.03 | 0.00 | 0.77 | 19.09 | 192.06 | -46.67 | 65.82 | 0.7558 | -340.0 | -283.4 | |
| 2.82 | 7.88 | 2.18 | 6.07 | 20.33 | 191.21 | -47.52 | 64.54 | 0.7683 | -411.2 | -318.9 | |
| 0.00 | 0.94 | 0.00 | 0.73 | 20.67 | 191.02 | -47.70 | 64.17 | 0.7712 | -348.0 | -271.6 | |
| 0.00 | 2.40 | 0.00 | 1.84 | 19.73 | 191.30 | -47.42 | 65.25 | 0.7655 | 535.0 | 507.9 | |
| 0.00 | 0.86 | 0.00 | 0.66 | 19.51 | 191.25 | -47.47 | 65.55 | 0.7654 | 397.0 | 506.3 | |
| 2.14 | 7.45 | 1.65 | 5.76 | 19.54 | 190.77 | -47.95 | 65.67 | 0.7703 | 660.4 | 503.6 | |
| 1.54 | 17.21 | 1.21 | 13.56 | 19.90 | 190.15 | -48.57 | 65.41 | 0.7776 | 629.9 | 542.7 | |
| 3.68 | -22.00 | 2.92 | -22.00 | 20.39 | 189.80 | -48.92 | 64.91 | 0.7825 | 711.7 | 999999 | |
| 0.00 | 3.68 | 0.00 | 2.98 | 21.61 | 188.96 | -49.76 | 63.68 | 0.7941 | 742.0 | 634.7 | |
| 1.11 | 4.71 | 0.94 | 3.98 | 21.69 | 186.99 | -51.73 | 64.17 | 0.8127 | 617.9 | 639.9 | |
| 10.61 | 51.62 | 9.13 | 44.61 | 22.28 | 186.37 | -52.35 | 63.64 | 0.8198 | 839.1 | 486.1 | |
| 4.28 | -26.00 | 3.72 | -26.00 | 22.53 | 185.98 | -52.75 | 63.46 | 0.8240 | 629.0 | 999999 | |
| 1.20 | -26.00 | 1.05 | -26.00 | 22.78 | 185.62 | -53.10 | 63.27 | 0.8277 | 336.8 | 999999 | |
| 0.00 | 1.03 | 0.00 | 0.91 | 23.18 | 185.23 | -53.50 | 62.90 | 0.8322 | 241.0 | 172.6 | |
| 0.00 | 0.94 | 0.00 | 0.83 | 22.42 | 185.23 | -53.49 | 63.80 | 0.8303 | 408.0 | 280.1 | |
| 0.00 | 0.86 | 0.00 | 0.75 | 22.04 | 185.28 | -53.44 | 64.23 | 0.8290 | 315.0 | 290.0 | |
| 0.00 | 1.46 | 0.00 | 1.29 | 22.22 | 184.91 | -53.81 | 64.12 | 0.8327 | 272.0 | 296.6 | |
| 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. | |