Viendo archivo del viernes, 16 junio 2017

Daily bulletin on solar and geomagnetic activity from the SIDC

Emitido: 2017 Jun 16 1242 UTC

SIDC Forecast

Valid from 1230 UTC, 16 Jun 2017 until 18 Jun 2017
Llamarada solar

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

Geomagnetism

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

Protones solares

Quiet

10cm fluxAp
16 Jun 2017077017
17 Jun 2017078011
18 Jun 2017079014

Bulletin

The only reported flare in the last 24 hours was the B2.9 flare which peaked at 17:00 UT on June 15. There are presently two sunspot groups observed on the visible side of the solar disc, Catania 32 and 33 (NOAA AR 2662 and 2663). The fast evolving Catania sunspot group 33 has presently beta-gamma configuration of its photospheric magnetic field and might be the source of B-class and possibly also isolated C-class flares in the coming hours. No Earth directed CMEs have been observed and the solar protons remained at background level in the past 24 hours.

The in situ observations indicate arrival of the fast solar wind (associated with the large equatorial coronal hole which reached central meridian in the morning of June 13), as expected, in the morning of June 16. At about 03:00 UT this morning the sudden increase of the interplanetary magnetic field (IMF) and the density increase was observed, soon followed with the change of the phi angle.The oscillations of the IMF and its Bz component were followed by sudden increase of the solar wind speed and temperature, and density decrease, marking the interaction region between the slow and fast solar wind. The solar wind speed is presently about 500 km/s and the IMF is about 13nT. Due to the negative value of the Bz component (down to -10nT) and increased solar wind speed (about 550 km/s) active geomagnetic conditions were reported today (Dourbes reported K=4 and NOAA Kp=4). The fast solar wind associated with two large coronal holes (one on the north and one on the south solar hemisphere) which reached central meridian in the evening of June 14 is expected to arrive at the Earth early in the morning of June 18. The geomagnetic conditions are presently active and we expect them to stay so in the coming hours.

Today's estimated international sunspot number (ISN): 031, based on 21 stations.

Solar indices for 15 Jun 2017

Wolf number Catania035
10cm solar flux077
AK Chambon La Forêt009
AK Wingst006
Estimated Ap004
Estimated international sunspot number032 - Based on 34 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 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 2026111.2 -12.8
Last 30 days106.5 -1.5

Efemérides*

Llamarada solar
12014X1.79
22004X1.19
32014X1.04
42003M7.07
52004M6.53
DstG
12015-107G2
21979-100G2
31998-77G2
41988-77G2
52005-71G4
*desde 1994

Redes sociales