SOHO MDI 2000-07-11 01:35:31 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 41 | 388 | 41 | 388 | -18.47 | 49.56 | 56.54 | 245.93 | 0.8677 | -280.2 | -115.6 | |
|
previous
or next observation for the same group /
back to the solar disc SOHO MDI 2000-07-11 01:35:31 UT |
| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 11 | 183 | 12 | 195 | -17.92 | 52.37 | 59.35 | 247.39 | 0.8886 | -515.9 | -190.2 | |
| 6 | -1 | 6 | -1 | -17.92 | 51.72 | 58.70 | 247.21 | 0.8838 | -702.1 | 999999 | |
| 0 | 3 | 0 | 3 | -16.73 | 50.25 | 57.24 | 248.12 | 0.8698 | -575.0 | -503.8 | |
| 0 | 5 | 0 | 5 | -17.07 | 48.16 | 55.14 | 247.12 | 0.8535 | -332.0 | -358.3 | |
| 10 | 29 | 10 | 29 | -20.09 | 49.60 | 56.58 | 244.20 | 0.8726 | -664.7 | -386.8 | |
| 0 | 22 | 0 | 21 | -17.52 | 47.93 | 54.91 | 246.54 | 0.8527 | -393.0 | -156.0 | |
| 0 | 3 | 0 | 3 | -18.99 | 47.75 | 54.73 | 244.82 | 0.8551 | -249.0 | -109.1 | |
| 0 | 5 | 0 | 4 | -16.81 | 46.62 | 53.60 | 246.93 | 0.8396 | 211.0 | 220.4 | |
| 0 | 17 | 0 | 16 | -19.40 | 47.44 | 54.42 | 244.26 | 0.8537 | -38.0 | -38.2 | |
| 0 | 4 | 0 | 4 | -20.06 | 47.70 | 54.68 | 243.61 | 0.8576 | -700.0 | -574.9 | |
| 1 | 42 | 1 | 38 | -17.72 | 46.30 | 53.28 | 245.78 | 0.8394 | 509.2 | 144.9 | |
| 0 | 5 | 0 | 5 | -17.38 | 45.68 | 52.66 | 245.95 | 0.8330 | 728.0 | 652.2 | |
| 3 | 12 | 3 | 12 | -20.05 | 46.83 | 53.81 | 243.32 | 0.8505 | -587.5 | -460.6 | |
| 0 | 9 | 0 | 8 | -18.90 | 46.13 | 53.11 | 244.38 | 0.8413 | 332.0 | 421.2 | |
| 0 | 3 | 0 | 3 | -19.00 | 45.61 | 52.60 | 244.09 | 0.8372 | 679.0 | 661.7 | |
| 0 | 4 | 0 | 4 | -21.21 | 45.99 | 52.97 | 241.73 | 0.8471 | 262.0 | 115.0 | |
| 10 | 39 | 9 | 35 | -20.37 | 44.87 | 51.85 | 242.26 | 0.8351 | 656.8 | 66.0 | |
| 0 | 1 | 0 | 1 | -20.10 | 44.00 | 50.98 | 242.22 | 0.8268 | 601.0 | 451.3 | |
| 0 | 2 | 0 | 2 | -21.19 | 44.17 | 51.16 | 241.05 | 0.8320 | 356.0 | 279.3 | |
| 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. | |