Перегляд архіву середа, 6 грудня 2023

Щоденний бюлетень про сонячну та геомагнітну активність від SIDC

Випущено: 2023 Dec 06 1243 UTC

Прогноз SIDC

Сонячні спалахи

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

Геомагнетизм

Quiet (A<20 and K<4)

Сонячні протони

Quiet

	10 см потік	Ap
06 Dec 2023	142	017
07 Dec 2023	142	017
08 Dec 2023	142	017

Сонячно-активні області та спалахи

Solar flaring activity was moderated over past 24 hours with several M-class flares. The M-class flares were produced by the bipolar active region NOAA 3513. This new region also produced several C-class flares. The currently most complex region, NOAA 3511, with a beta-gamma magnetic class, showis goring and has produced several C-class flares. The other regions, NOAA 3500, and 3510 continue to produce C-class flares. C-class flares are expected in the next 24 hours with some chances of M-class flare from NOAA 3513 and possibly NOAA 3511.

Корональні викиди маси

No Earth directed coronal mass ejection was identified in the currently available SOHO/LASCO-C2 coronographe images.

Корональні діри

The large equatorial coronal hole (negative polarity) is currently on the geoeffective location of the Sun (on the West side near longitudes 45-55 degrees).

Сонячний вітер

The Solar Wind (SW) conditions near Earth are affected by the High-Speed Stream (HSS) from the large equatorial coronal hole that crossed the central meridian on Saturday 2 of December. The SW speed ranged between 505 km/s and 665 km/s, the total interplanetary magnetic field (Bt) decreased to values below 6.5 nT. The North-South magnetic component (Bz) ranged between -4.5 and 4.6 nT. The interplanetary magnetic field phi angle was negative (directed towards the Sun) during the past 24 hours. The SW conditions are expected to remain strongly affected by the said HSS during the next 24 hours.

Геомагнетизм

Geomagnetic conditions were mainly unsettle both globally and locally (NOAA-Kp and K-BEL 1 to 3) during the last 24 hours. We expect mainly unsettled condition in the next 24 hours in response to the ongoing fast solar wind conditions, possibly with short periods of active conditions.

Рівні потоку протонів

The greater than 10 MeV proton flux was at nominal levels over the past 24 hours and is expected to remain so for the next 24 hours.

Потоки електронів на геостаціонарній орбіті

The greater than 2 MeV electron flux, as measured by the GOES-16 satellite, was below the 1000 pfu alert threshold during the last 24 hours and it is expected to remain mostly below 1000 pfu during the next 24 hours, however, due to the ongoing fast solar wind condition we expect the greater than 2 MeV electron flux to show some increases. The 24h electron fluence was at low levels during the past 24 hours and is expected to remain at these levels for the following 24 hours with also some increases due to the ongoing solar wind conditions.

Розрахунок міжнародної кількості сонячних плям станом на сьогодні (ISN): 143, за даними 09 станцій.

Сонячні індекси за 05 Dec 2023

Число Вольфа, Катанія	///
Сонячний потік 10 см	142
AK Chambon La Forêt	022
AK Wingst	015
Розрахунковий індекс Ap	043
Розрахункова міжнародна кількість сонячних плям	132 - За даними 06 станцій

Зведення помітних подій

Надано Центром Аналізу Даних Сонячного Впливу (SIDC)© - SIDC - Оброблено SpaceWeatherLive

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