Viendo archivo del martes, 19 agosto 2025

Daily bulletin on solar and geomagnetic activity from the SIDC

Emitido: 2025 Aug 19 1231 UTC

SIDC Forecast

Llamarada solar

C-class flares expected, (probability >=50%)

Geomagnetism

Active conditions expected (A>=20 or K=4)

Protones solares

Quiet

10cm fluxAp
19 Aug 2025116019
20 Aug 2025116021
21 Aug 2025118012

Solar Active Regions and flaring

Solar flaring activity was moderate over the past 24 hours, with 1 M-class flare identified. A total of 7 numbered sunspot groups were identified on the disk over the past 24 hours, having all Alpha or Beta magnetic configuration. The largest flare was a M1.1 flare (SIDC Flare 5177) peaking on August 19 at 04:39 UTC, which was produced by SIDC Sunspot Group 572 (NOAA Active Region 4188), who has a Alpha magnetic configuration and was growing over the past 24 hours. Solar flaring activity is expected to be low over the next 24 hours, with C-class flares likely and a small chance for M-class flares.

Eyección de masa coronal

No new Earth-directed Coronal Mass Ejections (CMEs) have been detected in the available coronagraph images.

Viento solar

The solar wind conditions at Earth were mainly slow over the past 24 hours. The speed started to increase slightly from 350km/s to 420 km/s. The interplanetary magnetic field reached a maximum of 16 nT with the Bz reaching a minimum value of -7 nT. The solar wind speed is expected to become enhanced in the next 24 hours, due to the potential arrival of the high-speed stream (HSS) associated with the SIDC coronal hole 116.

Geomagnetism

Geomagnetic activity was quiet to unsettled over the past 24 hours both globally and locally. In response to the expected arrival of high-speed stream, geomagnetic conditions are expected to reach active level in the next 24 hours.

Proton flux levels

The greater than 10 MeV proton flux remained below the 10 pfu threshold and is expected to remain so over the next days.

Electron fluxes at geostationary orbit

The greater than 2 MeV electron flux measured by GOES 18 and GOES 19 has dropped below the 1000 pfu threshold. Electron flux levels are expected to remain below the 1000 pfu threshold over the next 24 hours. The 24-hour electron fluence returned to normal levels and is expected to remain so over the next 24 hours.

Today's estimated international sunspot number (ISN): 038, based on 19 stations.

Solar indices for 18 Aug 2025

Wolf number Catania049
10cm solar flux114
AK Chambon La Forêt016
AK Wingst011
Estimated Ap010
Estimated international sunspot number057 - Based on 32 stations

Noticeable events summary

DayBeginMaxFinLocStrengthOP10cmCatania/NOAARadio burst types
19035104390507----M1.1--/----

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

All times in UTC

< < Ir a la visión general diaria

Últimas noticias

Apoye a SpaceWeatherLive.com!

A lot of people come to SpaceWeatherLive to follow the Solar activity or if there is a chance to see the aurora, but with more traffic comes higher costs to keep the servers online. If you like SpaceWeatherLive and want to support the project you can choose a subscription for an ad-free site or consider a donation. With your help we can keep SpaceWeatherLive online!

No Ads on SWL Pro!
No Ads on SWL Pro! Suscripciones
Donations
Apoye a SpaceWeatherLive.com! Donar
Apoya a SpaceWeatherLive con nuestro merchandise
Échale un ojo a nuestro merchandise

Hechos clima espacial

Último evento clase X08/12/2025X1.1
Último evento clase M31/12/2025M7.11
Últimas tormentas geomagnéticas02/01/2026Kp5 (G1)
Días sin manchas
Último día sin manchas08/06/2022
Promedio de manchas solares mensuales
diciembre 2025124 +32.2
enero 2026122 -2
Last 30 days111.1 +8.3

Efemérides*

Llamarada solar
12025X1.2
22025X1.1
32025M5.8
41998M3.7
52025M2.3
DstG
11988-66
21968-63
31979-59
41990-51G1
51957-50
*desde 1994

Redes sociales