Het archief bekijken van maandag 18 november 2024

Dagelijks bulletin over zonne- en geomagnetische activiteit van het SIDC

Datum verslag: 2024 Nov 18 1246 UTC

SIDC Prognose

Zonnevlammen

M-class flares expected (probability >=50%)

Geomagnetisme

Quiet (A<20 and K<4)

Proton Flux monitor

Quiet

10cm fluxAp
18 Nov 2024156015
19 Nov 2024160011
20 Nov 2024170010

Zonnevlekkengebieden en zonnevlammen

Solar flaring activity was high over the past 24 hours, with 5 M-class flares. The largest flare was an M2.5 flare peaking on November 18 at 10:58 UTC from an as yet unnumbered region rotating over the south-east limb. SIDC Sunspot Group 288 (NOAA Active Region 3889) the other largest region on disk also produced C-class flaring activity but is now approaching the east limb. The solar flaring activity is expected to be moderate over the next 24 hours, with M-class flares likely and a small chance for X-class flares.

Coronale massa uitstoten

No Earth-directed coronal mass ejections (CMEs) have been detected in the available coronagraph imagery over the past 24 hours.

Coronale gaten

SIDC Coronal Hole 79 (mid-latitude coronal hole with a negative polarity) has begun to cross the central meridian on November 18.

Zonnewind

Over the past 24 hours the solar wind conditions reflected a slow solar wind regime. The interplanetary magnetic field continued to be slightly elevated, ranging between 5 and 9nT, with a minimum Bz of -7 nT. The solar wind speed ranged between 310 and 380 km/s. The interplanetary magnetic field phi angle remained predominantly in the positive sector (directed towards the Sun). The solar wind speed is expected to become slightly elevated over the next 24 hours due to the possible high-speed stream arrival associated with SIDC Coronal Hole 78, although this is low confidence.

Geomagnetisme

The geomagnetic conditions over the past 24 hours were quiet to unsettled. Quiet to unsettled geomagnetic conditions are expected for the next 24 hours with isolated active conditions possible due to any high- speed stream influence.

Proton flux niveaus

Over the past 24 hours the greater than 10 MeV GOES proton flux was below the 10 pfu threshold. The greater than 10 MeV GOES proton flux is expected to continue to be below this threshold over the 24 hours.

Elektronenfluxen in geostationaire baan

The greater than 2 MeV electron flux as measured by GOES 18 crossed the 1000 pfu threshold briefly and is expected to again be at or near this threshold over the next 24 hours. The 24h electron fluence was at nominal levels and is expected to remain so in the next 24 hours.

Het geschatte internationale zonnevlekkengetal (ISN) van vandaag: 110, gebaseerd op 12 stations.

Zon indexen voor 17 Nov 2024

Wolfgetal Catania///
10cm zonneflux146
AK Chambon La Forêt011
AK Wingst006
Geschatte Ap006
Geschat internationaal zonnevlekkengetal085 - Gebaseerd op 14 stations

Overzicht opvallende gebeurtenissen

DagStartMaxEindeLocatieSterkteOP10cmCatania/NOAASoorten radio-uitbarstingen
18051305220527----M1.0--/3901
18072507320736S07E76M1.7SF--/3901
18075407570801S07E76M1.21--/3901III/2
18104110581102S07E76M2.5SF--/3901
18110611121119----M1.6--/----III/2

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

Alle tijden in UTC

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Deze dag in de geschiedenis*

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12024M2.41
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DstG
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