SDO HMI 2011-11-10 11:58:58 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!)
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 72.72 | 373.80 | 38.68 | 198.99 | 9.59 | 55.88 | -20.58 | 72.14 | 0.3654 | -543.8 | -349.1 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2011-11-10 11:58:58 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 |
| 0.00 | 1.55 | 0.00 | 0.80 | 6.88 | 60.07 | -16.39 | 77.33 | 0.2884 | -804.0 | -627.1 | |
| 0.00 | 0.95 | 0.00 | 0.50 | 12.50 | 57.16 | -19.30 | 63.42 | 0.3623 | 762.0 | 581.7 | |
| 46.00 | 290.23 | 24.31 | 153.49 | 9.41 | 56.86 | -19.60 | 71.92 | 0.3497 | -1281.8 | -432.7 | |
| 0.00 | 0.95 | 0.00 | 0.50 | 7.12 | 56.94 | -19.51 | 78.38 | 0.3399 | -702.0 | -613.9 | |
| 1.90 | 2.67 | 1.01 | 1.42 | 11.23 | 56.67 | -19.78 | 67.18 | 0.3617 | -879.6 | -720.6 | |
| 0.00 | 1.12 | 0.00 | 0.59 | 10.66 | 56.52 | -19.94 | 68.82 | 0.3609 | -668.0 | -529.0 | |
| 2.15 | -3.00 | 1.14 | -3.00 | 9.76 | 56.23 | -20.23 | 71.46 | 0.3610 | -745.5 | 999999 | |
| 1.21 | -3.00 | 0.64 | -3.00 | 10.09 | 56.14 | -20.31 | 70.66 | 0.3638 | -730.9 | 999999 | |
| 0.00 | 1.81 | 0.00 | 0.96 | 10.62 | 56.04 | -20.42 | 69.34 | 0.3680 | -904.0 | -686.1 | |
| 0.00 | 0.69 | 0.00 | 0.37 | 8.20 | 56.00 | -20.46 | 75.83 | 0.3584 | -459.0 | -423.6 | |
| 0.00 | 1.64 | 0.00 | 0.87 | 10.50 | 55.79 | -20.66 | 69.86 | 0.3712 | -704.0 | -552.2 | |
| 1.46 | -3.00 | 0.78 | -3.00 | 9.78 | 55.74 | -20.71 | 71.77 | 0.3686 | -668.4 | 999999 | |
| 0.00 | 2.58 | 0.00 | 1.37 | 8.94 | 55.67 | -20.79 | 74.04 | 0.3663 | -410.0 | -339.4 | |
| 0.00 | 0.95 | 0.00 | 0.51 | 10.70 | 55.45 | -21.00 | 69.62 | 0.3773 | -658.0 | -519.6 | |
| 1.90 | 15.94 | 1.01 | 8.51 | 9.05 | 55.14 | -21.31 | 74.08 | 0.3748 | -736.0 | -385.5 | |
| 0.00 | 0.52 | 0.00 | 0.28 | 12.19 | 54.85 | -21.61 | 66.47 | 0.3943 | -686.0 | -553.3 | |
| 1.90 | -15.00 | 1.01 | -15.00 | 9.10 | 54.88 | -21.57 | 74.10 | 0.3791 | -702.5 | 999999 | |
| 0.00 | 1.46 | 0.00 | 0.78 | 8.47 | 54.73 | -21.73 | 75.82 | 0.3793 | 971.0 | 804.9 | |
| 0.00 | 1.12 | 0.00 | 0.60 | 9.27 | 54.19 | -22.26 | 74.10 | 0.3905 | 465.0 | 350.5 | |
| 9.82 | 12.06 | 5.27 | 6.48 | 8.58 | 54.20 | -22.25 | 75.82 | 0.3879 | 852.4 | 654.9 | |
| 0.00 | 3.10 | 0.00 | 1.69 | 12.06 | 53.31 | -23.14 | 68.01 | 0.4163 | 854.0 | 620.7 | |
| 4.14 | 4.57 | 2.27 | 2.50 | 9.99 | 51.84 | -24.62 | 73.70 | 0.4292 | -925.0 | -709.2 | |
| 0.00 | 2.15 | 0.00 | 1.18 | 9.95 | 51.64 | -24.81 | 73.88 | 0.4321 | -469.0 | -499.1 | |
| 0.00 | 1.29 | 0.00 | 0.72 | 13.31 | 51.12 | -25.34 | 66.92 | 0.4546 | 631.0 | 464.7 | |
| 0.00 | 2.15 | 0.00 | 1.18 | 9.83 | 51.39 | -25.07 | 74.29 | 0.4355 | -880.0 | -703.4 | |
| 0.00 | 1.55 | 0.00 | 0.85 | 9.79 | 51.16 | -25.30 | 74.49 | 0.4389 | -758.0 | -628.8 | |
| 0.00 | 4.57 | 0.00 | 2.52 | 9.72 | 50.76 | -25.69 | 74.83 | 0.4446 | -658.0 | -666.5 | |
| 2.24 | 7.84 | 1.24 | 4.36 | 11.10 | 50.54 | -25.92 | 71.96 | 0.4530 | 901.2 | 657.2 | |
| 0.00 | 2.24 | 0.00 | 1.24 | 10.67 | 50.38 | -26.08 | 72.96 | 0.4538 | 879.0 | 622.8 | |
| 0.00 | 1.03 | 0.00 | 0.59 | 12.69 | 47.17 | -29.28 | 70.53 | 0.5082 | 787.0 | 635.2 | |
| 0.00 | 3.88 | 0.00 | 2.26 | 13.07 | 45.82 | -30.63 | 70.48 | 0.5287 | 273.0 | 521.2 | |
| 0.00 | 1.64 | 0.00 | 0.96 | 11.24 | 44.99 | -31.46 | 74.20 | 0.5341 | 646.0 | 514.1 | |
| 0.00 | 1.55 | 0.00 | 0.91 | 10.99 | 44.60 | -31.86 | 74.80 | 0.5390 | 783.0 | 600.8 | |
| 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. | |