Het archief bekijken van donderdag 28 maart 2019

Dagelijks bulletin over zonne- en geomagnetische activiteit van het SIDC

Datum verslag: 2019 Mar 28 1230 UTC

SIDC Prognose

Zonnevlammen

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

Geomagnetisme

Quiet (A<20 and K<4)

Proton Flux monitor

Quiet

	10cm flux	Ap
28 Mar 2019	069	010
29 Mar 2019	068	010
30 Mar 2019	067	008

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.

Het geschatte internationale zonnevlekkengetal (ISN) van vandaag: 000, gebaseerd op 14 stations.

Zon indexen voor 27 Mar 2019

Wolfgetal Catania	///
10cm zonneflux	069
AK Chambon La Forêt	011
AK Wingst	008
Geschatte Ap	008
Geschat internationaal zonnevlekkengetal	000 - Gebaseerd op 25 stations

Overzicht opvallende gebeurtenissen

Aangeboden door het Solar Influences Data Analysis Center© - SIDC - Verwerkt door SpaceWeatherLive

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