Prohlížíte si archiv úterý 18. srpna 2020

Daily bulletin on solar and geomagnetic activity from the SIDC

Vydáno: 2020 Aug 18 1237 UTC

SIDC Forecast

Valid from 1230 UTC, 18 Aug 2020 until 20 Aug 2020
Sluneční erupce

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

Geomagnetism

Quiet (A<20 and K<4)

Sluneční protony

Quiet

10cm fluxAp
18 Aug 2020071003
19 Aug 2020071008
20 Aug 2020071014

Bulletin

The solar activity was low over the past 24 hours. The N0AA-AR 2771 is still on the disk. The X-ray flux was at A-class level and the solar activity is expected to remain low.

The Coronal Mass Ejection (CME) that took place on Aug 16th 18:00UT has a small chance of a glancing blow from late Aug 19th.

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

The solar wind speed near Earth varied between 280 and 340km/s (DSCOVR). The polarity of the Interplanetary Magnetic Field (IMF) was predominantly oriented away the Sun (phi angle in the positive sector). Bz fluctuated between -6 and +5 nT. The magnitude of the magnetic field varied between 1 and 7 nT. A negative coronal hole crossed the central meridian on August 17th. An enhancement could be expected on Aug 20th, possibly combined with any effects from the CME. For the first part of the next 24 hours, the solar wind speed is expected to remain low, while by the end of Aug 19th to be enhanced as a response to the influence of the CME.

The geomagnetic conditions were quiet. The values registered for the past 24 hours were 0-2 for K Dourbes and NOAA Kp. Quiet geomagnetic conditions are expected for the next 24 hours. The solar wind speed near Earth varied between 280 and 340km/s (DSCOVR). The polarity of the Interplanetary Magnetic Field (IMF) was predominantly oriented away the Sun (phi angle in the positive sector). Bz fluctuated between -6 and +5 nT. The magnitude of the magnetic field varied between 1 and 7 nT. A negative Coronal hole crossed the central meridian on August 17th. An enhancement could be expected on Aug 20th, possibly combined with any effects from the CME. For the next 24 hours the solar wind speed is expected to remain low for the beginnig of that time period, while by the end of Aug 19th to be enhanced as a response to the influence of the CME.

Today's estimated international sunspot number (ISN): 012, based on 21 stations.

Solar indices for 17 Aug 2020

Wolf number Catania///
10cm solar flux071
AK Chambon La Forêt008
AK Wingst004
Estimated Ap003
Estimated international sunspot number000 - Based on 30 stations

Noticeable events summary

DayBeginMaxKonecLocStrengthOP10cmCatania/NOAARadio burst types
Žádný

Provided by the Solar Influences Data analysis Center© - SIDC - Processed by SpaceWeatherLive

Všechny časy v UTC

<< Přejít na stránku s denním přehledem

Poslední zprávy

Podpora SpaceWeatherLive.com!

Mnoho lidí přichází do SpaceWeatherLive, aby sledovali aktivitu Slunce nebo pokud je vidět polární záři, ale s větším provozem přicházejí i vyšší náklady na server. Zvažte dar, pokud vás baví SpaceWeatherLive, abychom mohli udržovat web online!

Darovat SpaceWeatherLive Pro
Podpořte naše zboží SpaceWeatherLive
Podívejte se na naše zboží

Fakta o počasí ve vesmíru

Poslední X-záblesk28. 03. 2025X1.1
Poslední M-záblesk15. 04. 2025M1.2
Poslední geomagnetická bouře16. 04. 2025Kp8- (G4)
Dny bez skvrn
Poslední den bez skvrn08. 06. 2022
Průměrný měsíční počet slunečních skvrn
března 2025134.2 -20.4
dubna 2025120.5 -13.7
Posledních 30 dnů118.3 -22.1

Tento den v historii*

Sluneční erupce
12014X1.05
22016M9.63
32024M2.2
42022M1.9
52024M1.6
DstG
11965-162G4
22002-127G3
32001-114G3
41990-95G1
51957-89G2
*od roku 1994

Sociální sítě