Viendo archivo del jueves, 28 marzo 2019

Daily bulletin on solar and geomagnetic activity from the SIDC

Emitido: 2019 Mar 28 1230 UTC

SIDC Forecast

Valid from 1230 UTC, 28 Mar 2019 until 30 Mar 2019
Llamarada solar

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

Geomagnetism

Quiet (A<20 and K<4)

Protones solares

Quiet

10cm fluxAp
28 Mar 2019069010
29 Mar 2019068010
30 Mar 2019067008

Bulletin

There are no active regions, presently observed on the visible side of the solar disc, and accordingly solar flaring activity is very low. We expect such a low level of the solar activity, without C-class and even B-class flares, to persist in the coming hours. There were no wide and/or Earth directed CMEs reported and the solar protons remained at the background level.

At about 03:40 UT this morning, interplanetary magnetic field magnitude increased (to the value of about 14 nT) simultaneously with the increase of the solar wind speed and decrease of the temperature indicating arrival of possibly either ICME (still unclear what would be its solar counterpart) or a structure at the boundary between the slow and the fast solar wind. More will be reported later, when larger part of the structure becomes visible in the in situ observations. The solar wind speed is presently about 430 km/s and the interplanetary magnetic field magnitude is presently 9 nT. The fast solar wind associated with the negative polarity equatorial coronal hole which reached central meridian on March 25 is expected at the Earth tomorrow. The geomagnetic conditions are quiet to unsettled (both local station at Dourbes and NOAA reported only K=3 and Kp=3, respectively) and we expect them to stay so in the coming hours.

Today's estimated international sunspot number (ISN): 000, based on 14 stations.

Solar indices for 27 Mar 2019

Wolf number Catania///
10cm solar flux069
AK Chambon La Forêt011
AK Wingst008
Estimated Ap008
Estimated international sunspot number000 - Based on 25 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

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