Viendo archivo del sábado, 22 septiembre 2018

Daily bulletin on solar and geomagnetic activity from the SIDC

Emitido: 2018 Sep 22 1230 UTC

SIDC Forecast

Valid from 1230 UTC, 22 Sep 2018 until 24 Sep 2018
Llamarada solar

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

Geomagnetism

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

Protones solares

Quiet

10cm fluxAp
22 Sep 2018067018
23 Sep 2018067011
24 Sep 2018066008

Bulletin

There are presently no sunspot groups observed on the visible side of the Sun. Accordingly, no flares were reported during last 24 hours and we expect such a quiet conditions to persist in the coming hours. No Earth directed CMEs were observed, and the solar protons remained at the background level.

The in situ observations indicate arrival of the fast solar wind associated with the low latitudinal extent of the northern polar coronal hole. The interplanetary magnetic field magnitude started to increased simultaneously with the density increase and the change of the phi angle in the late evening of the September 21. After about 23:00 UT on September 21, density decreased and solar wind speed started to increase simultaneously with the increase of the temperature. The solar wind speed is presently about 470 km/s and the interplanetary magnetic field magnitude is about 10 nT. The arrival of one more fast flow, associated with patchy equatorial coronal hole which reached central meridian on September 18, is expected this evening. The arrival of the fast solar wind induced disturbed geomagnetic conditions yesterday evening and this morning. Local station at Dourbes reported intervals of K=4 at about 03:00 UT this morning, while NOAA reported two intervals of Kp=5 starting from about 21:00 UT yesterday up to 03:00 UT this morning. Presently geomagnetic conditions are unsettled to active and we expect such a disturbed geomagnetic conditions to remain the coming hours. We might expect also isolated intervals of minor storm conditions starting from late this evening due to arrival of the fast flow associated with the equatorial coronal hole.

Today's estimated international sunspot number (ISN): 000, based on 20 stations.

Solar indices for 21 Sep 2018

Wolf number Catania000
10cm solar flux067
AK Chambon La Forêt028
AK Wingst009
Estimated Ap011
Estimated international sunspot number000 - Based on 32 stations

Noticeable events summary

DayBeginMaxFinLocStrengthOP10cmCatania/NOAARadio burst types
Ninguno

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 X03/02/2026X1.5
Último evento clase M03/02/2026M3.4
Últimas tormentas geomagnéticas28/01/2026Kp5+ (G1)
Días sin manchas
Último día sin manchas08/06/2022
Promedio de manchas solares mensuales
diciembre 2025124 +32.2
febrero 2026133 +9
Last 30 days120.6 +10.9

Efemérides*

Llamarada solar
12014M7.48
22014M5.51
32025M4.7
42000M4.36
52002M3.41
DstG
11983-172G4
21961-157G3
31992-101G1
41984-87G2
51957-86G1
*desde 1994

Redes sociales