Weekly forecast
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Activity level: mostly low to moderate X-ray background flux (1.0-8.0 A): in the range B6.0 - C1.0 Radio flux (10.7 cm): a fluctuation in the range 135-150 (Apr 1 - 3) and 105-125 (Apr 4 - 7) Events: class C (2-14/day), class M (2-8/period), class X (0-1/period), proton (0-1/period) Relative sunspot number (Ri): in the range 55-200 Martina Pavelkova and Simona Beerova RWC Prague, Astronomical Institute, Solar Dept., Ondrejov, Czech Republic e-mail: sunwatch(at)asu.cas.cz
Quiet: Apr 2 - 3, 6 Unsettled: Apr 1 - 5, 7 Active: Apr 1, 4, 7 Minor storm: possible Apr 7 Major storm: 0 Severe storm: 0 Geomagnetic activity summary: Within the next 24 hours, we expect the coming storming event culmination. The other active event with possible stroming event is also possible at the end of currently forecasted period, about Thursday, April 7. Unlikely, an another active event is also possible about Monday, April 4. Other days, we expected quiet to unsettled conditions mostly near the higher level. Quiet to unsettled conditions closer the quieter level is expected about Sunday, April 3, and Wednesday, April 6. Tomas Bayer RWC Prague Institute of Geophysics of the ASCR, Prague Department of Geomagnetism Budkov observatory (BDV)
(Free continuation of my Earth's magnetic field activity predictions, published between 1978 - 2021.) We have a week of somewhat wilder development behind us. Its first indication were two sunspot groups on the northeastern limb of the solar disc on March 24. The second of them, region No. 2976 was larger, but smaller. Region No. 2975 had a more complex magnetic structure and gradually grew. A proton solar flare was observed there on March 28 at 11:29 UT, accompanied by a significant increase in proton levels. And above all - it was followed by CME heading to Earth! Exactly as predicted, the arrival of CME caused a geomagnetic disturbance on March 31. Its positive phase of development was accompanied, especially in the UTC morning hours, by a significant improvement in the shortwave propagation conditions on a global scale. Another solar flare was observed in the same area on March 30 with a maximum at 17:37 UT. Although X-ray levels rose more than on March 28, followed by CME again (albeit weaker, at 18:23 UT), there is no expectation that it would be followed by a similar increase in gemagnetic activity F. K. Janda, A.R.S. OK1HH Emails: ok1hh(at)crk.cz, ok1hh(at)rsys.cz Pmail: OK1HH(at)OK0NAG.#BOH.CZE.EU
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