Viewing archive of Monday, 3 July 2017

Daily bulletin on solar and geomagnetic activity from the SIDC

Issued: 2017 Jul 03 1231 UTC

SIDC Forecast

Valid from 1230 UTC, 03 Jul 2017 until 05 Jul 2017
Solar flares

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

Geomagnetism

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

Solar protons

Quiet

10cm fluxAp
03 Jul 2017067011
04 Jul 2017065022
05 Jul 2017063007

Bulletin

NOAA 2664 is rotating over the west limb and remained quiet, no C-class flares in past 24 h. A small unnumbered AR south of AR 2664 has chances of producing C-class flares in the next 24 h.

No Earth directed Coronal Mass Ejections (CMEs) have been detected. Solar protons have remained at background levels over the past 24 hours.

Geomagnetic conditions are quiet and expected to remain so until the Earth is affected by the high speed stream from an equatorial coronal hole within 48 h, and by the glancing blow from the CME on June 28 (less likely). Active to minor storm conditions expected then.

Today's estimated international sunspot number (ISN): 000, based on 24 stations.

Solar indices for 02 Jul 2017

Wolf number Catania///
10cm solar flux071
AK Chambon La Forêt030
AK Wingst024
Estimated Ap023
Estimated international sunspot number012 - Based on 27 stations

Noticeable events summary

DayBeginMaxEndLocStrengthOP10cmCatania/NOAARadio burst types
None

Provided by the Solar Influences Data analysis Center© - SIDC - Processed by SpaceWeatherLive

All times in UTC

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Current data suggests there is a slight possibility for aurora to appear at the following high latitude regions in the near future

Arkhangelsk
The solar wind speed is currently moderately high (583.7 km/sec.)
The maximum X-ray flux of the past two hours is:
M1.99

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