Przeglądasz Archiwum z niedziela, 4 lipca 2021

Codzienne wiadomości na temat aktywności słonecznej i geomagnetycznej z SIDC

Odnotowany: 2021 Jul 04 1239 UTC

Prognoza SIDC

Rozbłyski słoneczne

M-class flares expected (probability >=50%)

Geomagnetyzm

Quiet (A<20 and K<4)

Monitoring przepływu protonów

Quiet

	strumień 10cm	Ap
04 Jul 2021	093	008
05 Jul 2021	091	013
06 Jul 2021	088	017

Skrót wiadomości

After yesterdays M2.7 flare the new and rapidly emerging region in the North West (NOAA 2838) produced an X1.5 flare peaking at 14:29UT, then followed by another M1 and M1.2 flare peaking at 17:03UT and 5:09UT. This marks the first X flare since September 2017, and the first of the current Solar cycle. The region is currently disappearing behind the West limb, but it may still produce flaring activity effective to Earth. The largest region remaining on disc, NOAA region 2835 is in the process of loosing its trailing spots and decreasing in size but also remains a strong candidate for further flaring activity. Both regions 2836 (unipolar) and 2837 (bipolar) are in decay. Another region is emerging near N19E45. Overall there is a significant possibility of another M flare occurring, from the region disappearing over the limb but also from region 2835 on disc.

A number of Westward CMEs are visible in SoHO/LASCO coronagraph data with the following approximate timings of first appearance in the C2 field of view: July 2: 15:36UT, July 3: 3:24UT, 7:48UT, 14:48UT and July 4 6:00UT. They are all assessed to not be geoeffective.

The greater than 10 MeV proton flux showed a slight enhancement following the X flare, but remained below 1 pfu and thus well below the 10 pfu event threshold. It is expected to be at nominal levels for the next 24 hours. The greater than 2 MeV electron flux was below the 1000 pfu event threshold. The 24h electron fluence was at normal levels and electron fluence is expected to remain at normal levels over the next days.

Solar wind has returned to nominal slow Solar wind conditions with Solar wind speed now down to 335km/s. Total magnetic field decreased from around 5nT to well below 5nT with a variable Bz. The magnetic field phi angle switched into the sector with magnetic field away from the Sun around 15UT, but since 6UT it switched back into the sector with magnetic field towards the Sun. There are no signs of the June 29 CME and it is now not expected any more. Solar wind is expected to be at nominal slow Solar wind conditions until tomorrow when enhancements may be expected associated to the small equatorial coronal hole that passed central meridian July 2.

Geomagnetic conditions were quiet to unsettled (NOAA Kp 0-1 and local K Dourbes 0-3). Geomagnetic conditions are expected to be quiet over the next 24 hours, increasing tomorrow to unsettled conditions as Solar wind enhancements are expected by that time.

Dzisiejsza szacunkowa międzynarodowa liczba plam na Słońcu (ISN): 052, na podstawie 10 stacji.

Indeksy solarne na 03 Jul 2021

Liczba Wolfa z Katanii	///
10cm solar flux	094
AK Chambon La Forêt	009
AK Wingst	004
Szacunkowa Ap	004
Szacowana międzynarodowa liczba plam słonecznych	060 - Na podstawie stacji 23

Podsumowanie wydarzeń godnych uwagi

Dostarczone przez Centrum Analizy Danych Wpływów Słonecznych© - SIDC - Przetworzone przez SpaceWeatherLive

Wszystkie czasy w UTC

<< Idź do codziennego przeglądu