SOHO MDI 2000-07-06 11:11:31 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 141 | 996 | 77 | 532 | -18.18 | 49.35 | -4.57 | 168.75 | 0.3810 | -743.1 | -226.5 | |
|
previous
or next observation for the same group /
back to the solar disc SOHO MDI 2000-07-06 11:11:31 UT |
| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 56 | 348 | 30 | 185 | -17.74 | 52.17 | -1.75 | 175.41 | 0.3656 | -2059.7 | -667.1 | |
| -1 | -1 | -1 | -1 | -17.87 | 51.75 | -2.17 | 174.36 | 0.3683 | 999999 | 999999 | |
| 0 | 10 | 0 | 5 | -15.76 | 50.99 | -2.93 | 171.54 | 0.3355 | -1200.0 | -869.5 | |
| 5 | 159 | 3 | 84 | -16.64 | 50.65 | -3.27 | 170.99 | 0.3507 | -1375.9 | -919.9 | |
| 9 | -4 | 5 | -4 | -17.19 | 50.52 | -3.41 | 170.89 | 0.3600 | -1780.4 | 999999 | |
| 5 | 34 | 3 | 18 | -18.56 | 50.07 | -3.85 | 170.39 | 0.3830 | -1246.2 | -757.7 | |
| 0 | 3 | 0 | 2 | -20.93 | 50.01 | -3.91 | 171.26 | 0.4207 | -639.0 | -617.6 | |
| 0 | 3 | 0 | 2 | -20.54 | 49.94 | -3.98 | 170.94 | 0.4148 | -588.0 | -443.0 | |
| 5 | -4 | 3 | -4 | -17.45 | 49.93 | -3.99 | 169.49 | 0.3657 | -1393.5 | 999999 | |
| 0 | 5 | 0 | 2 | -18.64 | 49.61 | -4.31 | 169.31 | 0.3857 | -858.0 | -767.1 | |
| 5 | 9 | 2 | 5 | -20.20 | 49.23 | -4.69 | 169.19 | 0.4113 | -1066.9 | -712.8 | |
| 5 | 90 | 3 | 48 | -18.90 | 49.18 | -4.74 | 168.42 | 0.3912 | -1183.0 | -755.0 | |
| 4 | -12 | 2 | -12 | -18.61 | 48.85 | -5.07 | 167.47 | 0.3876 | -1294.9 | 999999 | |
| 5 | 87 | 3 | 46 | -16.31 | 48.67 | -5.25 | 165.49 | 0.3521 | 1248.5 | 682.6 | |
| 10 | -14 | 5 | -14 | -16.49 | 48.17 | -5.75 | 164.31 | 0.3570 | 1487.2 | 999999 | |
| 5 | 11 | 3 | 6 | -20.03 | 47.79 | -6.13 | 165.91 | 0.4137 | -1006.5 | -693.5 | |
| 0 | 3 | 0 | 2 | -19.00 | 47.71 | -6.22 | 165.03 | 0.3981 | -534.0 | -399.4 | |
| 0 | 6 | 0 | 3 | -16.95 | 47.74 | -6.18 | 163.58 | 0.3662 | 786.0 | 669.6 | |
| 0 | 3 | 0 | 2 | -20.34 | 47.10 | -6.82 | 164.60 | 0.4212 | -252.0 | -277.6 | |
| 0 | 5 | 0 | 2 | -19.35 | 47.06 | -6.86 | 163.82 | 0.4062 | 434.0 | 172.8 | |
| 0 | 3 | 0 | 2 | -17.72 | 47.00 | -6.92 | 162.41 | 0.3816 | 836.0 | 682.0 | |
| 0 | 4 | 0 | 2 | -17.77 | 46.70 | -7.22 | 161.75 | 0.3838 | 739.0 | 627.7 | |
| 3 | 22 | 2 | 12 | -19.74 | 46.28 | -7.64 | 162.40 | 0.4158 | 1084.3 | 887.0 | |
| 0 | 17 | 0 | 9 | -20.78 | 46.10 | -7.82 | 162.81 | 0.4324 | 1002.0 | 643.8 | |
| 0 | 11 | 0 | 6 | -18.41 | 45.96 | -7.96 | 160.61 | 0.3974 | 1475.0 | 1123.0 | |
| 3 | -23 | 2 | -23 | -19.75 | 45.77 | -8.15 | 161.32 | 0.4184 | 1056.4 | 999999 | |
| 0 | 3 | 0 | 2 | -20.52 | 45.73 | -8.19 | 161.85 | 0.4303 | 749.0 | 735.2 | |
| 0 | 5 | 0 | 2 | -17.90 | 45.77 | -8.15 | 159.72 | 0.3908 | 831.0 | 900.9 | |
| 0 | 6 | 0 | 3 | -20.09 | 45.62 | -8.30 | 161.29 | 0.4244 | 846.0 | 742.5 | |
| 0 | 4 | 0 | 2 | -20.61 | 45.47 | -8.46 | 161.38 | 0.4329 | 1176.0 | 972.0 | |
| 6 | 101 | 3 | 55 | -19.15 | 45.50 | -8.42 | 160.24 | 0.4109 | 1552.5 | 1120.5 | |
| 2 | -31 | 1 | -31 | -18.93 | 45.22 | -8.70 | 159.44 | 0.4093 | 1375.4 | 999999 | |
| 0 | 3 | 0 | 2 | -20.75 | 45.07 | -8.85 | 160.69 | 0.4369 | 813.0 | 713.9 | |
| 4 | -31 | 2 | -31 | -19.93 | 44.86 | -9.06 | 159.58 | 0.4259 | 1300.5 | 999999 | |
| 3 | -31 | 2 | -31 | -19.32 | 44.86 | -9.07 | 159.02 | 0.4171 | 1447.9 | 999999 | |
| 0 | 4 | 0 | 2 | -20.36 | 44.58 | -9.34 | 159.38 | 0.4339 | 1093.0 | 911.7 | |
| 0 | 3 | 0 | 2 | -20.32 | 44.33 | -9.59 | 158.84 | 0.4347 | 1129.0 | 931.1 | |
| 0 | 4 | 0 | 2 | -21.11 | 44.06 | -9.86 | 159.00 | 0.4476 | 798.0 | 656.2 | |
| 6 | 13 | 3 | 7 | -19.38 | 43.62 | -10.30 | 156.53 | 0.4253 | 1330.7 | 858.1 | |
| 0 | 8 | 0 | 5 | -21.46 | 43.39 | -10.53 | 158.03 | 0.4566 | 715.0 | 677.1 | |
| 0 | 2 | 0 | 1 | -21.82 | 42.88 | -11.04 | 157.41 | 0.4646 | 632.0 | 531.4 | |
| 0 | 4 | 0 | 2 | -20.52 | 42.29 | -11.63 | 155.09 | 0.4501 | 687.0 | 503.6 | |
| 0 | 3 | 0 | 2 | -20.58 | 41.38 | -12.54 | 153.47 | 0.4570 | 623.0 | 586.2 | |
| 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. | |