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

12135 102.52 588.94 53.63 307.33 13.01 130.35 -16.78 65.60 0.3104 -234.4 -162.6


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

SDO HMI 2014-08-10 08:00:39 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 0.27 414.08 0.14 213.62 14.54 133.26 -13.88 58.02 0.2750 -988.0 -441.6
2 0.99 -1.00 0.51 -1.00 14.41 133.14 -14.00 58.63 0.2757 -1042.2 999999
3 62.51 -1.00 32.24 -1.00 14.09 132.70 -14.43 60.36 0.2794 -1434.8 999999
4 2.35 -1.00 1.21 -1.00 13.42 132.71 -14.43 62.55 0.2743 -911.3 999999
5 1.45 -1.00 0.75 -1.00 13.74 132.27 -14.87 62.14 0.2831 -904.1 999999
6 0.00 5.15 0.00 2.67 13.04 131.12 -16.02 65.93 0.2957 -942.0 -822.8
7 0.00 1.81 0.00 0.95 15.20 129.55 -17.59 61.50 0.3333 -589.0 -498.5
8 0.00 1.26 0.00 0.66 10.39 129.53 -17.61 75.84 0.3082 -866.0 -615.6
9 0.00 1.08 0.00 0.57 12.53 126.86 -20.28 71.41 0.3585 860.0 702.2
10 0.00 0.99 0.00 0.52 8.11 126.98 -20.15 83.82 0.3446 905.0 732.6
11 0.00 2.44 0.00 1.30 11.84 126.45 -20.69 73.54 0.3621 953.0 737.7
12 0.00 0.90 0.00 0.48 10.47 126.55 -20.59 77.24 0.3561 839.0 608.8
13 0.00 0.72 0.00 0.38 12.11 126.33 -20.81 72.89 0.3650 914.0 696.0
14 0.00 2.44 0.00 1.29 10.58 126.24 -20.90 77.08 0.3613 872.0 746.4
15 0.00 1.08 0.00 0.58 10.83 126.23 -20.91 76.42 0.3622 847.0 683.1
16 0.00 0.99 0.00 0.53 11.19 126.07 -21.07 75.53 0.3658 847.0 715.1
17 0.00 1.63 0.00 0.87 10.60 125.88 -21.26 77.20 0.3671 880.0 709.3
18 1.17 5.33 0.63 2.84 11.54 125.74 -21.40 74.76 0.3721 1008.2 733.2
19 0.00 8.04 0.00 4.28 10.29 125.67 -21.47 78.14 0.3696 919.0 796.3
20 0.00 3.16 0.00 1.69 10.55 125.51 -21.62 77.48 0.3727 1019.0 938.2
21 2.44 5.33 1.30 2.85 10.15 125.28 -21.86 78.65 0.3754 1011.5 798.9
22 3.34 83.20 1.79 44.69 10.78 125.03 -22.11 77.10 0.3809 1181.1 581.6
23 3.52 -22.00 1.89 -22.00 10.56 124.85 -22.29 77.75 0.3832 1139.6 999999
24 0.00 1.63 0.00 0.87 10.30 124.57 -22.57 78.51 0.3870 902.0 737.5
25 0.00 0.90 0.00 0.49 10.09 124.51 -22.63 79.09 0.3874 837.0 761.4
26 18.43 -22.00 9.91 -22.00 10.69 124.40 -22.74 77.58 0.3906 965.0 999999
27 0.00 1.26 0.00 0.68 10.17 124.37 -22.77 78.91 0.3898 885.0 791.6
28 5.78 41.55 3.11 22.37 9.86 124.26 -22.88 79.74 0.3909 1164.2 401.5
29 0.00 1.26 0.00 0.68 10.32 124.20 -22.94 78.61 0.3929 672.0 607.8
30 0.27 -28.00 0.15 -28.00 9.70 124.07 -23.07 80.20 0.3936 831.7 999999
31 0.00 0.81 0.00 0.44 10.67 123.87 -23.27 77.84 0.3989 358.0 221.0
32 0.00 1.90 0.00 1.03 10.57 123.67 -23.47 78.16 0.4017 499.0 429.7


  • 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.