| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 84.20 | 345.01 | 70.52 | 284.62 | 17.36 | 62.57 | -52.34 | 71.03 | 0.7994 | -276.9 | -142.5 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2011-11-07 13:58:59 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 |
| 2.16 | 255.82 | 1.70 | 201.58 | 17.57 | 64.73 | -50.18 | 70.35 | 0.7798 | -607.8 | -263.6 | |
| 3.28 | -1.00 | 2.58 | -1.00 | 17.10 | 64.62 | -50.29 | 70.97 | 0.7802 | -602.3 | 999999 | |
| 2.07 | 15.09 | 1.65 | 12.06 | 17.89 | 64.31 | -50.60 | 70.03 | 0.7847 | -589.1 | -406.4 | |
| 3.88 | -3.00 | 3.11 | -3.00 | 18.18 | 64.05 | -50.86 | 69.72 | 0.7879 | -513.6 | 999999 | |
| 50.20 | -1.00 | 39.53 | -1.00 | 16.45 | 64.56 | -50.35 | 71.80 | 0.7796 | -837.7 | 999999 | |
| 0.00 | 1.38 | 0.00 | 1.13 | 18.64 | 63.20 | -51.71 | 69.32 | 0.7972 | 542.0 | 518.4 | |
| 0.00 | 1.55 | 0.00 | 1.26 | 18.21 | 63.23 | -51.68 | 69.85 | 0.7961 | -436.0 | -306.7 | |
| 2.07 | -1.00 | 1.67 | -1.00 | 17.14 | 63.56 | -51.35 | 71.12 | 0.7910 | -329.4 | 999999 | |
| 0.00 | 1.29 | 0.00 | 1.06 | 18.25 | 62.86 | -52.05 | 69.87 | 0.7999 | -267.0 | -197.5 | |
| 0.60 | 1.81 | 0.49 | 1.48 | 17.17 | 62.90 | -52.02 | 71.20 | 0.7977 | -250.6 | -143.0 | |
| 1.55 | 2.24 | 1.31 | 1.89 | 18.69 | 61.78 | -53.13 | 69.54 | 0.8111 | 554.1 | 482.8 | |
| 0.00 | 0.86 | 0.00 | 0.71 | 17.06 | 62.48 | -52.43 | 71.42 | 0.8017 | -157.0 | -176.0 | |
| 0.00 | 1.29 | 0.00 | 1.06 | 16.87 | 62.55 | -52.36 | 71.63 | 0.8007 | -391.0 | -280.2 | |
| 0.00 | 1.55 | 0.00 | 1.30 | 17.14 | 61.72 | -53.19 | 71.44 | 0.8092 | -456.0 | -305.3 | |
| 0.00 | 0.86 | 0.00 | 0.72 | 16.56 | 61.85 | -53.06 | 72.13 | 0.8071 | -449.0 | -364.4 | |
| 0.00 | 0.35 | 0.00 | 0.29 | 16.89 | 61.67 | -53.24 | 71.76 | 0.8094 | -295.0 | -277.0 | |
| 0.00 | 1.64 | 0.00 | 1.38 | 16.74 | 61.63 | -53.28 | 71.96 | 0.8096 | -493.0 | -375.2 | |
| 0.00 | 1.73 | 0.00 | 1.46 | 16.90 | 61.30 | -53.61 | 71.80 | 0.8130 | -394.0 | -263.9 | |
| 0.00 | 1.73 | 0.00 | 1.48 | 17.09 | 60.64 | -54.28 | 71.69 | 0.8196 | 119.0 | 53.1 | |
| 0.00 | 0.52 | 0.00 | 0.48 | 21.81 | 57.89 | -57.02 | 66.54 | 0.8510 | -296.0 | -260.0 | |
| 0.00 | 0.52 | 0.00 | 0.45 | 16.12 | 60.35 | -54.57 | 72.90 | 0.8212 | 401.0 | 426.0 | |
| 0.00 | 0.69 | 0.00 | 0.61 | 17.98 | 59.47 | -55.44 | 70.79 | 0.8317 | 550.0 | 470.4 | |
| 0.00 | 1.55 | 0.00 | 1.38 | 17.69 | 59.22 | -55.69 | 71.17 | 0.8336 | 522.0 | 435.5 | |
| 0.00 | 0.95 | 0.00 | 0.92 | 21.42 | 56.39 | -58.52 | 67.26 | 0.8629 | 618.0 | 505.9 | |
| 0.00 | 1.38 | 0.00 | 1.33 | 19.91 | 56.41 | -58.50 | 68.99 | 0.8608 | 577.0 | 522.1 | |
| 0.00 | 1.04 | 0.00 | 1.00 | 19.47 | 56.43 | -58.49 | 69.50 | 0.8602 | 525.0 | 514.8 | |
| 3.11 | 4.49 | 3.05 | 4.40 | 20.03 | 55.84 | -59.07 | 68.93 | 0.8656 | 585.8 | 469.8 | |
| 0.00 | 2.76 | 0.00 | 2.70 | 19.69 | 55.93 | -58.98 | 69.31 | 0.8646 | 633.0 | 418.6 | |
| 10.01 | 23.12 | 10.05 | 23.14 | 20.28 | 55.13 | -59.78 | 68.76 | 0.8717 | 681.1 | 439.6 | |
| 0.00 | 0.95 | 0.00 | 0.92 | 18.23 | 56.03 | -58.88 | 70.98 | 0.8621 | 605.0 | 531.6 | |
| 1.47 | 1.98 | 1.49 | 2.01 | 20.10 | 54.73 | -60.18 | 69.01 | 0.8746 | 429.6 | 398.5 | |
| 3.80 | 14.58 | 3.89 | 15.09 | 20.27 | 54.36 | -60.55 | 68.87 | 0.8777 | 463.9 | 379.6 | |
| 0.00 | 1.29 | 0.00 | 1.33 | 19.95 | 54.25 | -60.66 | 69.25 | 0.8783 | 318.0 | 272.6 | |
| 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. | |