SDO HMI 2011-11-10 23:58:58 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 |
| 67.01 | 431.08 | 34.13 | 220.47 | 16.38 | 64.33 | -5.51 | 21.27 | 0.2462 | -749.9 | -402.4 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2011-11-10 23:58:58 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 | 2.24 | 0.00 | 1.14 | 16.77 | 69.72 | -0.12 | 0.50 | 0.2328 | -980.0 | -749.3 | |
| 0.00 | 2.41 | 0.00 | 1.21 | 12.65 | 65.46 | -4.38 | 24.79 | 0.1785 | -538.0 | -397.7 | |
| 59.52 | 375.61 | 30.30 | 191.25 | 15.97 | 65.21 | -4.63 | 19.57 | 0.2328 | -1422.1 | -491.0 | |
| 0.95 | -3.00 | 0.48 | -3.00 | 15.51 | 65.09 | -4.74 | 20.73 | 0.2262 | -1112.2 | 999999 | |
| 2.58 | 4.31 | 1.32 | 2.20 | 17.00 | 64.59 | -5.25 | 20.34 | 0.2528 | -892.9 | -709.0 | |
| 1.46 | -3.00 | 0.75 | -3.00 | 16.36 | 64.55 | -5.29 | 21.47 | 0.2429 | -928.0 | 999999 | |
| 1.21 | 4.13 | 0.62 | 2.12 | 17.25 | 64.52 | -5.32 | 20.24 | 0.2570 | -674.3 | -650.1 | |
| 0.00 | 0.78 | 0.00 | 0.40 | 17.80 | 64.51 | -5.33 | 19.54 | 0.2658 | -496.0 | -431.8 | |
| 0.00 | 2.84 | 0.00 | 1.46 | 17.58 | 64.32 | -5.51 | 20.44 | 0.2635 | -1042.0 | -768.4 | |
| 0.00 | 1.03 | 0.00 | 0.53 | 17.64 | 64.10 | -5.74 | 21.10 | 0.2657 | -739.0 | -604.7 | |
| 0.00 | 2.41 | 0.00 | 1.23 | 15.75 | 64.13 | -5.71 | 24.04 | 0.2361 | -838.0 | -656.3 | |
| 1.29 | -3.00 | 0.66 | -3.00 | 16.57 | 63.73 | -6.11 | 24.03 | 0.2515 | -925.4 | 999999 | |
| 0.00 | 1.12 | 0.00 | 0.58 | 17.82 | 63.56 | -6.27 | 22.60 | 0.2719 | -829.0 | -661.5 | |
| 0.00 | 1.46 | 0.00 | 0.78 | 22.90 | 60.85 | -8.99 | 23.26 | 0.3661 | -841.0 | -625.4 | |
| 0.00 | 1.46 | 0.00 | 0.79 | 23.54 | 58.67 | -11.17 | 27.19 | 0.3904 | -968.0 | -758.9 | |
| 0.00 | 2.24 | 0.00 | 1.17 | 17.96 | 58.09 | -11.74 | 37.43 | 0.3200 | 784.0 | 676.8 | |
| 0.00 | 2.07 | 0.00 | 1.09 | 19.74 | 57.77 | -12.07 | 34.80 | 0.3463 | 826.0 | 601.9 | |
| 0.00 | 1.38 | 0.00 | 0.73 | 19.34 | 57.64 | -12.20 | 35.80 | 0.3423 | 816.0 | 640.1 | |
| 0.00 | 1.38 | 0.00 | 0.73 | 19.36 | 56.84 | -13.00 | 37.48 | 0.3504 | 907.0 | 723.1 | |
| 0.00 | 3.36 | 0.00 | 1.78 | 20.29 | 56.66 | -13.18 | 36.18 | 0.3639 | 713.0 | 585.0 | |
| 0.00 | 2.76 | 0.00 | 1.46 | 18.86 | 56.26 | -13.58 | 39.59 | 0.3501 | 853.0 | 695.1 | |
| 0.00 | 0.78 | 0.00 | 0.42 | 22.90 | 55.72 | -14.12 | 33.78 | 0.4059 | -532.0 | -541.3 | |
| 0.00 | 1.55 | 0.00 | 0.82 | 19.65 | 55.71 | -14.13 | 39.18 | 0.3655 | 798.0 | 646.9 | |
| 0.00 | 1.46 | 0.00 | 0.79 | 20.25 | 54.15 | -15.69 | 40.95 | 0.3888 | 949.0 | 717.3 | |
| 0.00 | 1.38 | 0.00 | 0.75 | 21.65 | 53.90 | -15.94 | 38.96 | 0.4078 | 1106.0 | 850.8 | |
| 0.00 | 7.75 | 0.00 | 4.22 | 22.02 | 53.52 | -16.32 | 38.97 | 0.4159 | 650.0 | 575.4 | |
| 0.00 | 1.38 | 0.00 | 0.75 | 21.08 | 51.60 | -18.24 | 43.58 | 0.4255 | 659.0 | 502.0 | |
| 0.00 | 2.58 | 0.00 | 1.40 | 18.07 | 51.16 | -18.68 | 49.87 | 0.4000 | 589.0 | 535.9 | |
| 0.00 | 0.69 | 0.00 | 0.38 | 18.85 | 50.11 | -19.73 | 49.79 | 0.4202 | 701.0 | 557.6 | |
| 0.00 | 0.52 | 0.00 | 0.29 | 20.10 | 47.81 | -22.03 | 50.34 | 0.4594 | 750.0 | 640.5 | |
| 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. | |