| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 14.10 | 102.62 | 7.85 | 57.26 | 13.90 | 49.76 | -17.49 | 39.21 | 0.4622 | 10.1 | 37.7 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2014-03-05 23:00:28 UT
See sunspots with tool (Click here to study sunspot positions and configurations with tool using white-light and magnetogram images and polarity drawing) (It is recommended to set high resolution on your display!) |
| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 3.54 | 0.00 | 1.92 | 13.69 | 55.34 | -11.91 | 29.45 | 0.4094 | -768.0 | -661.8 | |
| 0.95 | 3.89 | 0.52 | 2.13 | 13.63 | 53.21 | -14.04 | 33.74 | 0.4263 | -981.8 | -759.2 | |
| 0.00 | 1.47 | 0.00 | 0.81 | 13.65 | 52.79 | -14.45 | 34.49 | 0.4301 | -905.0 | -625.8 | |
| 0.00 | 0.78 | 0.00 | 0.42 | 11.44 | 52.67 | -14.58 | 37.92 | 0.4031 | -677.0 | -512.3 | |
| 0.00 | 1.73 | 0.00 | 0.96 | 14.62 | 52.32 | -14.92 | 34.06 | 0.4468 | -804.0 | -706.2 | |
| 0.00 | 2.16 | 0.00 | 1.19 | 14.33 | 52.31 | -14.94 | 34.46 | 0.4432 | -1061.0 | -850.3 | |
| 0.00 | 1.12 | 0.00 | 0.62 | 14.95 | 52.14 | -15.11 | 33.97 | 0.4526 | -597.0 | -456.8 | |
| 0.00 | 1.38 | 0.00 | 0.76 | 14.47 | 52.11 | -15.14 | 34.64 | 0.4467 | -605.0 | -518.9 | |
| 0.00 | 0.95 | 0.00 | 0.52 | 12.69 | 52.10 | -15.15 | 37.12 | 0.4243 | -729.0 | -616.0 | |
| 0.00 | 1.99 | 0.00 | 1.10 | 13.78 | 51.90 | -15.34 | 35.94 | 0.4398 | -719.0 | -623.0 | |
| 0.61 | 2.07 | 0.33 | 1.14 | 13.14 | 51.88 | -15.37 | 36.86 | 0.4320 | -1006.9 | -816.2 | |
| 0.00 | 0.61 | 0.00 | 0.33 | 11.35 | 51.76 | -15.48 | 39.76 | 0.4110 | -677.0 | -495.9 | |
| 0.00 | 1.47 | 0.00 | 0.82 | 15.43 | 51.33 | -15.91 | 34.74 | 0.4657 | -896.0 | -717.6 | |
| 0.00 | 0.78 | 0.00 | 0.42 | 11.35 | 51.60 | -15.64 | 40.03 | 0.4127 | -718.0 | -533.2 | |
| 6.48 | 10.29 | 3.57 | 5.66 | 13.22 | 51.40 | -15.85 | 37.60 | 0.4376 | -910.1 | -535.8 | |
| 0.00 | 2.77 | 0.00 | 1.55 | 15.70 | 51.05 | -16.19 | 34.87 | 0.4715 | -781.0 | -572.8 | |
| 0.00 | 1.30 | 0.00 | 0.70 | 11.02 | 51.28 | -15.97 | 41.16 | 0.4120 | -486.0 | -464.1 | |
| 0.52 | 2.59 | 0.29 | 1.44 | 14.49 | 50.67 | -16.58 | 37.08 | 0.4601 | 445.3 | 330.9 | |
| 0.00 | 3.37 | 0.00 | 1.87 | 13.69 | 50.66 | -16.58 | 38.18 | 0.4504 | -686.0 | -564.4 | |
| 0.00 | 2.33 | 0.00 | 1.31 | 14.71 | 50.01 | -17.24 | 37.86 | 0.4689 | -869.0 | -642.7 | |
| 0.00 | 1.82 | 0.00 | 1.01 | 14.30 | 49.94 | -17.30 | 38.53 | 0.4645 | -813.0 | -635.7 | |
| 0.61 | 2.07 | 0.34 | 1.16 | 13.93 | 49.62 | -17.62 | 39.56 | 0.4633 | 792.9 | 609.7 | |
| 0.00 | 1.73 | 0.00 | 0.97 | 14.60 | 49.57 | -17.68 | 38.72 | 0.4718 | -384.0 | -300.4 | |
| 0.61 | 5.45 | 0.34 | 3.03 | 13.58 | 49.55 | -17.69 | 40.17 | 0.4599 | 926.7 | 528.7 | |
| 0.00 | 2.68 | 0.00 | 1.49 | 13.10 | 49.55 | -17.69 | 40.86 | 0.4543 | 942.0 | 732.5 | |
| 1.47 | 3.20 | 0.82 | 1.79 | 13.91 | 49.27 | -17.98 | 40.15 | 0.4666 | -434.9 | -365.4 | |
| 0.00 | 2.68 | 0.00 | 1.49 | 13.50 | 49.24 | -18.01 | 40.79 | 0.4621 | 904.0 | 766.3 | |
| 0.00 | 0.78 | 0.00 | 0.43 | 12.97 | 48.99 | -18.26 | 41.96 | 0.4586 | 884.0 | 731.6 | |
| 0.00 | 2.42 | 0.00 | 1.35 | 13.32 | 48.89 | -18.35 | 41.58 | 0.4635 | 969.0 | 794.6 | |
| 0.00 | 1.21 | 0.00 | 0.68 | 13.81 | 48.73 | -18.52 | 41.13 | 0.4708 | -455.0 | -488.4 | |
| 0.00 | 1.30 | 0.00 | 0.72 | 12.57 | 48.66 | -18.58 | 43.06 | 0.4575 | 626.0 | 500.1 | |
| 0.00 | 1.47 | 0.00 | 0.83 | 15.26 | 48.41 | -18.84 | 39.61 | 0.4906 | 958.0 | 745.5 | |
| 0.00 | 1.47 | 0.00 | 0.84 | 15.40 | 48.26 | -18.98 | 39.64 | 0.4936 | 713.0 | 579.7 | |
| 0.00 | 0.52 | 0.00 | 0.29 | 12.65 | 48.40 | -18.84 | 43.35 | 0.4611 | 696.0 | 523.2 | |
| 0.00 | 0.78 | 0.00 | 0.44 | 13.32 | 48.28 | -18.96 | 42.52 | 0.4698 | 786.0 | 594.0 | |
| 0.00 | 3.80 | 0.00 | 2.16 | 14.21 | 47.46 | -19.79 | 42.44 | 0.4883 | 772.0 | 561.9 | |
| 0.00 | 1.04 | 0.00 | 0.59 | 15.48 | 47.17 | -20.07 | 41.10 | 0.5051 | 509.0 | 336.6 | |
| 0.00 | 1.04 | 0.00 | 0.58 | 11.88 | 47.36 | -19.88 | 46.09 | 0.4639 | 685.0 | 514.2 | |
| 0.00 | 3.37 | 0.00 | 1.91 | 14.01 | 47.15 | -20.09 | 43.18 | 0.4891 | 768.0 | 765.5 | |
| 0.00 | 1.90 | 0.00 | 1.09 | 15.58 | 46.97 | -20.28 | 41.25 | 0.5084 | 723.0 | 496.7 | |
| 0.00 | 1.21 | 0.00 | 0.68 | 12.52 | 47.02 | -20.23 | 45.57 | 0.4746 | 554.0 | 431.3 | |
| 0.00 | 0.43 | 0.00 | 0.25 | 14.54 | 46.61 | -20.63 | 43.18 | 0.5006 | 698.0 | 600.8 | |
| 0.00 | 1.56 | 0.00 | 0.89 | 15.03 | 46.46 | -20.78 | 42.70 | 0.5073 | 833.0 | 682.9 | |
| 0.00 | 1.38 | 0.00 | 0.78 | 12.64 | 46.55 | -20.69 | 46.05 | 0.4809 | 826.0 | 549.0 | |
| 0.78 | 3.46 | 0.45 | 1.99 | 14.85 | 46.28 | -20.96 | 43.20 | 0.5072 | 856.8 | 688.8 | |
| 0.00 | 2.16 | 0.00 | 1.24 | 15.20 | 46.25 | -21.00 | 42.76 | 0.5114 | 530.0 | 505.9 | |
| 2.07 | 5.10 | 1.19 | 2.91 | 14.08 | 46.16 | -21.08 | 44.44 | 0.5003 | 925.0 | 720.7 | |
| 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. | |