Перегляд архіву пʼятниця, 31 липня 2020

Щоденний бюлетень про сонячну та геомагнітну активність від SIDC

Випущено: 2020 Jul 31 1231 UTC

Прогноз SIDC

Сонячні спалахи

Quiet conditions (<50% probability of C-class flares)

Геомагнетизм

Quiet (A<20 and K<4)

Сонячні протони

Quiet

	10 см потік	Ap
31 Jul 2020	073	003
01 Aug 2020	073	006
02 Aug 2020	073	010

Бюлетень

The solar activity remained at very low levels over the past 24 hours. The two visible sunspot regions (Catania 37/N0AA-AR 2767 and N0AA-AR 2768, both classified as alpha/Hsx now) remained stable and did not produce any significant flares. The observed X-ray flux remained below B-class level. The solar activity is expected to remain at low levels over the next 24 hours.

No Earth-directed Coronal Mass Ejections (CMEs) were observed in the available coronagraph imagery.

The greater than 10 MeV proton flux was at background levels over the past 24 hours and is expected to remain so for the next 24 hours. The greater than 2 MeV electron flux over the past 24 hours was at background to moderate levels and is expected to remain so over the next 24 hours.

Over the past 24 hours the solar wind conditions as reported by ACE and DSCOVR remained very quiet. The total interplanetary magnetic field was very weak with values between 1 nT and 6 nT. The north-south Bz component fluctuated between -5 nT and 3 nT. The Phi angle showed several long-term intervals with positive and negative orientation.

In the past 24 hours the solar wind speed remained at nominal levels typical for undisturbed slow solar wind, with values gradually increasing from 312 km/s to 370 km/s. The solar wind conditions are expected to remain quiet over the next 24 hours.

The geomagnetic conditions remained very quiet with maximum Kp-NOAA index equal to 1 and maximum K-Dourbes index equal to 2. The geomagnetic conditions are expected to remain quiet over the next 24 hours.

The recurrent positive polarity northern coronal hole (CH 64) continues to reside on the central meridian and has now become an extension of the northern polar coronal hole. The HSS emanating from this coronal hole is expected to reach the Earth from tomorrow on, causing enhancements in the solar wind speed and possibly intervals with unsettled geomagnetic conditions. These enhancements are expected to last for a few days after their onset.

Розрахунок міжнародної кількості сонячних плям станом на сьогодні (ISN): 021, за даними 32 станцій.

Сонячні індекси за 30 Jul 2020

Число Вольфа, Катанія	///
Сонячний потік 10 см	073
AK Chambon La Forêt	008
AK Wingst	004
Розрахунковий індекс Ap	004
Розрахункова міжнародна кількість сонячних плям	020 - За даними 38 станцій

Зведення помітних подій

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

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