SOHO MDI 2000-11-01 23:59:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 109 | 671 | 57 | 353 | -10.41 | 275.83 | -12.15 | 141.91 | 0.3286 | -368.4 | -199.0 | |
|
previous
or next observation for the same group /
back to the solar disc SOHO MDI 2000-11-01 23:59:32 UT |
| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0 | 5 | 0 | 3 | -9.31 | 282.03 | -5.95 | 156.31 | 0.2556 | -526.0 | -478.5 | |
| 0 | 5 | 0 | 3 | -12.43 | 280.34 | -7.64 | 155.55 | 0.3150 | -808.0 | -578.5 | |
| 0 | 5 | 0 | 3 | -11.35 | 280.22 | -7.76 | 153.64 | 0.2997 | -743.0 | -534.4 | |
| 35 | 326 | 18 | 168 | -9.29 | 279.60 | -8.38 | 148.24 | 0.2746 | -2116.3 | -711.1 | |
| 16 | -4 | 8 | -4 | -9.73 | 279.39 | -8.59 | 148.45 | 0.2826 | -1493.5 | 999999 | |
| 0 | 6 | 0 | 3 | -9.78 | 278.36 | -9.62 | 145.59 | 0.2928 | -730.0 | -695.9 | |
| 0 | 8 | 0 | 4 | -7.43 | 277.32 | -10.66 | 137.48 | 0.2728 | -740.0 | -588.7 | |
| 7 | 51 | 3 | 26 | -9.44 | 276.90 | -11.08 | 141.04 | 0.3028 | -1077.7 | -765.5 | |
| 4 | -8 | 2 | -8 | -9.49 | 276.54 | -11.44 | 140.24 | 0.3072 | -717.7 | 999999 | |
| 2 | 18 | 1 | 9 | -11.36 | 276.43 | -11.55 | 143.64 | 0.3326 | 1187.6 | 893.9 | |
| 0 | 9 | 0 | 5 | -8.54 | 276.41 | -11.57 | 137.83 | 0.2967 | -716.0 | -481.5 | |
| 2 | -10 | 1 | -10 | -11.36 | 276.15 | -11.83 | 142.99 | 0.3354 | 786.0 | 999999 | |
| 0 | 4 | 0 | 2 | -9.49 | 276.14 | -11.84 | 139.28 | 0.3116 | -538.0 | -429.3 | |
| 4 | 24 | 2 | 13 | -10.53 | 275.82 | -12.16 | 140.66 | 0.3280 | 1120.3 | 726.2 | |
| 3 | 9 | 2 | 5 | -9.04 | 274.88 | -13.10 | 135.41 | 0.3202 | 815.6 | 502.5 | |
| 0 | 5 | 0 | 3 | -10.28 | 274.39 | -13.59 | 136.99 | 0.3405 | -796.0 | -697.5 | |
| 0 | 4 | 0 | 2 | -6.64 | 272.60 | -15.38 | 125.13 | 0.3236 | -691.0 | -577.9 | |
| 0 | 4 | 0 | 2 | -12.18 | 271.19 | -16.79 | 134.64 | 0.3985 | 809.0 | 632.0 | |
| 0 | 8 | 0 | 4 | -13.29 | 270.17 | -17.82 | 134.92 | 0.4223 | -592.0 | -271.6 | |
| 0 | 3 | 0 | 2 | -13.94 | 270.07 | -17.91 | 135.87 | 0.4305 | -481.0 | -532.1 | |
| 0 | 8 | 0 | 4 | -16.06 | 269.72 | -18.26 | 138.69 | 0.4581 | -726.0 | -558.0 | |
| 0 | 4 | 0 | 2 | -14.67 | 269.80 | -18.18 | 136.66 | 0.4416 | 823.0 | 726.2 | |
| 12 | 111 | 7 | 60 | -11.70 | 269.49 | -18.49 | 131.01 | 0.4133 | 1731.1 | 741.4 | |
| 0 | 4 | 0 | 2 | -13.10 | 269.39 | -18.59 | 133.39 | 0.4292 | 636.0 | 547.9 | |
| 12 | -23 | 7 | -23 | -11.94 | 269.14 | -18.84 | 130.95 | 0.4200 | 1177.0 | 999999 | |
| 0 | 5 | 0 | 3 | -13.08 | 268.89 | -19.09 | 132.59 | 0.4346 | 1002.0 | 801.5 | |
| 12 | 40 | 6 | 22 | -13.17 | 268.17 | -19.81 | 131.72 | 0.4441 | 1153.8 | 754.8 | |
| 0 | 2 | 0 | 1 | -7.21 | 268.31 | -19.68 | 120.08 | 0.3877 | 230.0 | 404.5 | |
| 0 | 3 | 0 | 2 | -13.36 | 267.10 | -20.89 | 130.57 | 0.4585 | 894.0 | 762.2 | |
| 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. | |