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

9068 53 510 47 454 -18.42 48.85 52.30 244.59 0.8324 -246.4 -71.9


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

SOHO MDI 2000-07-10 19:11:31 UT
No observation available


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

1 0 4 0 4 -16.22 52.80 56.25 248.42 0.8606 -241.0 -352.6
2 0 2 0 2 -15.92 52.01 55.46 248.52 0.8533 -594.0 -556.1
3 12 187 11 178 -17.83 52.27 55.72 246.45 0.8601 -567.4 -226.4
4 5 -3 4 -3 -17.96 51.52 54.97 246.08 0.8542 -769.6 999999
5 4 -3 4 -3 -17.87 50.76 54.21 245.93 0.8476 -766.0 999999
6 0 12 0 11 -16.65 50.16 53.61 247.12 0.8392 -874.0 -572.3
7 0 2 0 2 -18.18 49.55 53.00 245.17 0.8382 -530.0 -442.9
8 0 3 0 2 -17.47 48.90 52.35 245.77 0.8304 -682.0 -573.5
9 11 33 10 30 -20.02 49.56 53.01 243.09 0.8437 -680.5 -360.7
10 0 2 0 2 -18.15 48.30 51.75 244.76 0.8272 -502.0 -445.8
11 6 31 5 27 -17.58 47.93 51.39 245.29 0.8221 -414.1 -182.7
12 0 2 0 2 -18.64 47.90 51.35 244.06 0.8251 -526.0 -469.7
13 0 14 0 12 -19.02 47.79 51.25 243.58 0.8254 -29.0 -144.5
14 0 1 0 1 -20.27 47.88 51.33 242.19 0.8302 -365.0 -365.0
15 2 89 2 74 -17.33 46.39 49.84 245.02 0.8071 724.7 239.2
16 0 4 0 4 -19.33 47.19 50.64 243.00 0.8211 174.0 125.0
17 0 3 0 3 -20.65 47.72 51.17 241.70 0.8301 145.0 -64.7
18 0 5 0 4 -20.89 47.50 50.95 241.33 0.8291 300.0 203.6
19 0 10 0 9 -19.96 46.93 50.39 242.17 0.8209 -642.0 -458.7
20 2 18 2 15 -18.97 46.19 49.64 243.01 0.8108 529.4 602.6
21 0 5 0 4 -17.36 45.44 48.89 244.61 0.7983 613.0 528.0
22 2 -20 2 -20 -19.03 45.76 49.21 242.77 0.8071 840.3 999999
23 0 6 0 5 -21.33 45.90 49.35 240.18 0.8168 273.0 179.6
24 9 51 7 43 -20.41 44.98 48.43 240.85 0.8051 704.7 99.6
25 0 11 0 9 -19.90 44.39 47.84 241.18 0.7978 646.0 411.9
26 0 3 0 2 -21.30 44.72 48.18 239.70 0.8063 30.0 103.3
27 0 3 0 2 -20.18 43.93 47.39 240.65 0.7947 552.0 522.9
28 0 9 0 7 -21.46 44.41 47.86 239.38 0.8041 360.0 316.6


  		• 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.