groupProj. UProj. WSCorr. UCorr. WS BLLCMPos. angler MU MP

11156 21.89 105.78 11.31 54.76 -20.31 67.20 -9.94 146.43 0.2914 47.3 164.2


previous   or   next   observation for the same group / back to the solar disc

SDO HMI 2011-02-10 20:58:56 UT

No observation available
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!)


spotProj. UProj. WSCorr. UCorr. WSBLLCMPos. angler MU MP

1 7.61 17.44 3.90 8.95 -20.06 70.29 -6.85 154.35 0.2600 1224.1 884.4
2 0.00 1.62 0.00 0.84 -20.72 69.75 -7.39 153.82 0.2739 806.0 715.2
3 0.00 13.68 0.00 7.04 -20.38 69.48 -7.66 152.40 0.2709 1134.0 974.2
4 0.00 5.39 0.00 2.78 -20.62 68.99 -8.15 151.38 0.2782 373.0 453.3
5 0.00 1.28 0.00 0.66 -20.01 68.96 -8.18 150.13 0.2697 1052.0 835.5
6 0.00 1.20 0.00 0.62 -20.28 68.91 -8.23 150.52 0.2740 811.0 571.5
7 0.00 2.31 0.00 1.19 -19.95 68.74 -8.40 149.35 0.2706 1022.0 761.0
8 0.00 1.71 0.00 0.88 -20.19 68.73 -8.41 149.79 0.2742 822.0 569.0
9 0.00 1.03 0.00 0.53 -19.55 68.57 -8.57 148.04 0.2665 956.0 778.1
10 0.00 4.62 0.00 2.38 -19.94 68.45 -8.69 148.51 0.2730 698.0 674.4
11 0.00 2.05 0.00 1.05 -18.96 67.97 -9.17 145.00 0.2640 1050.0 799.4
12 0.00 1.80 0.00 0.93 -20.90 67.82 -9.32 148.65 0.2921 -1078.0 -852.3
13 0.00 0.94 0.00 0.48 -18.81 67.95 -9.20 144.58 0.2622 961.0 744.0
14 1.62 2.22 0.84 1.15 -21.20 67.51 -9.63 148.40 0.2989 851.5 625.3
15 1.80 4.02 0.93 2.08 -20.96 67.47 -9.68 147.81 0.2959 883.1 247.6
16 3.85 4.96 1.99 2.57 -20.68 67.00 -10.14 146.06 0.2963 929.5 708.0
17 0.00 1.54 0.00 0.80 -21.77 66.80 -10.34 147.65 0.3130 833.0 616.3
18 0.00 1.88 0.00 0.97 -19.52 66.86 -10.29 143.21 0.2823 -828.0 -570.1
19 0.00 2.57 0.00 1.32 -19.42 66.64 -10.50 142.44 0.2833 -939.0 -819.3
20 0.00 1.28 0.00 0.67 -21.42 66.14 -11.00 145.42 0.3143 -941.0 -815.2
21 0.00 0.77 0.00 0.40 -20.72 64.97 -12.17 141.31 0.3169 -790.0 -607.3
22 0.00 1.54 0.00 0.80 -20.39 64.84 -12.31 140.29 0.3141 -962.0 -779.3
23 0.00 0.77 0.00 0.40 -20.26 64.56 -12.59 139.40 0.3155 -823.0 -663.9
24 7.01 9.83 3.65 5.12 -19.98 64.51 -12.63 138.70 0.3127 -1031.7 -721.5
25 0.00 1.88 0.00 0.99 -20.70 63.97 -13.17 139.11 0.3272 -887.0 -730.1
26 0.00 1.11 0.00 0.58 -20.30 63.78 -13.37 137.85 0.3245 -818.0 -593.8
27 0.00 2.14 0.00 1.12 -20.69 63.68 -13.47 138.50 0.3302 -737.0 -612.0
28 0.00 1.97 0.00 1.03 -20.44 63.50 -13.64 137.62 0.3292 -1013.0 -753.0
29 0.00 1.45 0.00 0.76 -20.38 63.22 -13.92 136.90 0.3316 -779.0 -689.9
30 0.00 1.20 0.00 0.63 -20.46 63.08 -14.06 136.83 0.3342 -686.0 -587.6
31 0.00 8.55 0.00 4.50 -20.45 62.53 -14.61 135.74 0.3403 -1076.0 -894.5
32 0.00 1.03 0.00 0.54 -21.39 62.40 -14.74 137.51 0.3523 -744.0 -591.8


  • 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.