SDO HMI 2014-06-30 19:00:40 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!)
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 51.56 | 113.83 | 38.27 | 85.05 | 13.66 | 275.72 | -47.78 | 74.19 | 0.7494 | -132.5 | 31.1 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2014-06-30 19:00:40 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 | 0.64 | 0.00 | 0.43 | 13.18 | 281.90 | -41.60 | 73.46 | 0.6766 | -758.0 | -662.3 | |
| 0.00 | 0.91 | 0.00 | 0.62 | 13.34 | 281.06 | -42.44 | 73.44 | 0.6873 | -198.0 | -255.1 | |
| 8.44 | 13.53 | 5.69 | 9.12 | 11.11 | 281.20 | -42.30 | 76.63 | 0.6810 | -837.2 | -556.2 | |
| 0.00 | 1.54 | 0.00 | 1.11 | 16.67 | 278.36 | -45.13 | 69.54 | 0.7270 | 613.0 | 473.7 | |
| 0.00 | 1.27 | 0.00 | 0.92 | 16.51 | 278.23 | -45.27 | 69.80 | 0.7281 | 381.0 | 294.6 | |
| 0.00 | 0.73 | 0.00 | 0.51 | 12.19 | 279.06 | -44.44 | 75.53 | 0.7091 | -518.0 | -453.5 | |
| 16.43 | 24.33 | 12.02 | 17.81 | 13.45 | 276.80 | -46.70 | 74.25 | 0.7377 | -797.5 | -471.1 | |
| 5.45 | 8.44 | 3.97 | 6.16 | 12.02 | 276.73 | -46.77 | 76.19 | 0.7361 | -584.2 | -338.8 | |
| 0.00 | 0.82 | 0.00 | 0.61 | 14.67 | 276.00 | -47.49 | 72.79 | 0.7489 | -390.0 | -322.9 | |
| 0.00 | 1.36 | 0.00 | 1.00 | 13.15 | 276.32 | -47.18 | 74.74 | 0.7426 | -556.0 | -447.2 | |
| 0.54 | 1.54 | 0.40 | 1.14 | 13.40 | 276.12 | -47.38 | 74.46 | 0.7453 | -437.3 | -409.9 | |
| 0.00 | 0.45 | 0.00 | 0.34 | 13.35 | 275.80 | -47.70 | 74.57 | 0.7488 | -170.0 | -173.4 | |
| 0.00 | 1.54 | 0.00 | 1.18 | 15.70 | 275.03 | -48.47 | 71.65 | 0.7615 | -35.0 | -69.5 | |
| 0.00 | 0.64 | 0.00 | 0.48 | 13.90 | 275.47 | -48.03 | 73.91 | 0.7534 | -166.0 | -308.3 | |
| 0.00 | 0.91 | 0.00 | 0.69 | 15.82 | 274.80 | -48.70 | 71.55 | 0.7642 | -556.0 | -361.4 | |
| 0.00 | 0.45 | 0.00 | 0.35 | 15.42 | 274.88 | -48.62 | 72.06 | 0.7626 | -333.0 | -326.4 | |
| 0.00 | 1.54 | 0.00 | 1.19 | 16.04 | 274.63 | -48.87 | 71.31 | 0.7664 | -491.0 | -381.3 | |
| 0.91 | 10.80 | 0.68 | 8.14 | 12.74 | 275.30 | -48.20 | 75.47 | 0.7534 | 847.8 | 587.6 | |
| 0.00 | 1.72 | 0.00 | 1.35 | 16.13 | 273.82 | -49.68 | 71.36 | 0.7752 | -561.0 | -423.7 | |
| 0.64 | -18.00 | 0.48 | -18.00 | 12.85 | 274.66 | -48.84 | 75.44 | 0.7606 | 563.6 | 999999 | |
| 0.00 | 1.45 | 0.00 | 1.11 | 13.58 | 274.36 | -49.13 | 74.53 | 0.7650 | -510.0 | -408.0 | |
| 0.00 | 1.09 | 0.00 | 0.84 | 14.04 | 273.94 | -49.55 | 74.02 | 0.7702 | 516.0 | 396.8 | |
| 0.00 | 2.36 | 0.00 | 1.85 | 15.37 | 273.53 | -49.97 | 72.39 | 0.7768 | 197.0 | 238.4 | |
| 6.08 | 29.23 | 4.76 | 22.90 | 14.80 | 273.42 | -50.08 | 73.14 | 0.7770 | 730.2 | 543.5 | |
| 0.00 | 1.18 | 0.00 | 0.92 | 13.78 | 273.73 | -49.77 | 74.39 | 0.7721 | 295.0 | 276.8 | |
| 10.62 | -24.00 | 8.34 | -24.00 | 14.51 | 273.31 | -50.19 | 73.53 | 0.7777 | 765.5 | 999999 | |
| 0.00 | 0.82 | 0.00 | 0.63 | 12.81 | 273.75 | -49.75 | 75.63 | 0.7705 | -457.0 | -477.0 | |
| 2.45 | -24.00 | 1.93 | -24.00 | 14.26 | 273.19 | -50.31 | 73.87 | 0.7786 | 600.9 | 999999 | |
| 0.00 | 1.27 | 0.00 | 1.00 | 13.54 | 273.26 | -50.24 | 74.77 | 0.7768 | -413.0 | -266.3 | |
| 0.00 | 2.54 | 0.00 | 2.03 | 15.12 | 272.67 | -50.83 | 72.88 | 0.7854 | 436.0 | 389.8 | |
| 0.00 | 0.73 | 0.00 | 0.62 | 17.64 | 270.05 | -53.45 | 70.25 | 0.8156 | 275.0 | 246.4 | |
| 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. | |