SOHO MDI 2000-11-05 16:13:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 59 | 462 | 34 | 272 | 2.41 | 271.85 | 32.31 | 268.51 | 0.5358 | 1451.6 | 566.8 | |
|
previous
or next observation for the same group /
back to the solar disc SOHO MDI 2000-11-05 16:13:32 UT |
| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 16 | 381 | 9 | 226 | 2.23 | 273.51 | 33.97 | 268.35 | 0.5608 | 1362.6 | 676.9 | |
| 12 | -1 | 7 | -1 | 2.06 | 273.14 | 33.60 | 267.99 | 0.5555 | 1548.4 | 999999 | |
| 0 | 4 | 0 | 3 | 3.95 | 272.83 | 33.29 | 271.41 | 0.5500 | 597.0 | 481.3 | |
| 5 | -1 | 3 | -1 | 1.92 | 272.72 | 33.18 | 267.69 | 0.5496 | 1351.8 | 999999 | |
| 6 | -1 | 3 | -1 | 2.23 | 272.54 | 33.00 | 268.24 | 0.5467 | 1499.8 | 999999 | |
| 20 | -1 | 12 | -1 | 2.70 | 272.37 | 32.83 | 269.08 | 0.5438 | 1827.5 | 999999 | |
| 0 | 6 | 0 | 4 | 3.57 | 271.62 | 32.08 | 270.66 | 0.5323 | 1120.0 | 856.8 | |
| 0 | 4 | 0 | 2 | -0.19 | 271.33 | 31.79 | 263.53 | 0.5323 | 659.0 | 617.7 | |
| 0 | 4 | 0 | 3 | 0.58 | 271.24 | 31.70 | 264.97 | 0.5296 | 604.0 | 583.2 | |
| 0 | 6 | 0 | 3 | 0.78 | 269.93 | 30.40 | 265.08 | 0.5099 | 206.0 | 280.1 | |
| 0 | 11 | 0 | 6 | 2.26 | 269.38 | 29.84 | 267.92 | 0.4996 | 642.0 | 534.3 | |
| 0 | 5 | 0 | 3 | 6.01 | 266.45 | 26.91 | 275.80 | 0.4544 | -556.0 | -518.5 | |
| 0 | 9 | 0 | 5 | 3.83 | 266.05 | 26.52 | 270.96 | 0.4474 | 592.0 | 587.2 | |
| 0 | 3 | 0 | 1 | 2.17 | 263.67 | 24.13 | 266.81 | 0.4109 | -705.0 | -602.7 | |
| 0 | 3 | 0 | 2 | 2.68 | 263.25 | 23.72 | 268.00 | 0.4038 | -793.0 | -720.6 | |
| 0 | 8 | 0 | 4 | 3.07 | 263.05 | 23.51 | 268.95 | 0.4002 | -943.0 | -811.4 | |
| 0 | 7 | 0 | 4 | 2.07 | 262.91 | 23.37 | 266.42 | 0.3989 | -671.0 | -695.3 | |
| 0 | 5 | 0 | 3 | 3.59 | 260.52 | 20.99 | 270.12 | 0.3590 | -736.0 | -587.8 | |
| 0 | 6 | 0 | 3 | 2.69 | 259.85 | 20.31 | 267.46 | 0.3486 | -860.0 | -751.8 | |
| 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. | |