Viewing archive of Sunday, 7 July 2024

Daily bulletin on solar and geomagnetic activity from the SIDC

Issued: 2024 Jul 07 1231 UTC

SIDC Forecast

Solar flares

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

Geomagnetism

Quiet (A<20 and K<4)

Solar protons

Quiet

10cm fluxAp
07 Jul 2024162008
08 Jul 2024158010
09 Jul 2024154010

Solar Active Regions and flaring

Solar flaring activity over the past 24 hours was at moderate levels, with one M-class flares recorded. The largest flare was a M1.0-flare, with peak time 23:15 UTC on July 06 associated with active region NOAA AR 3738 (beta-gamma-delta). There are currently 8 numbered active regions on the visible disk. NOAA AR 3738 (beta-gamma- delta) was the largest and most magnetically complex regions on disk. Most of the flaring activity in the last 24 hours came from NOAA AR 3738 (beta- gamma-delta) and NOAA AR 3729 (beta). NOAA AR 3733 and NOAA AR 3729 have started to rotate over the west limb. The solar flaring activity is likely to be at moderate levels over the coming days with C-class flares expected, M-class flares likely and a small chance for an X-class flare.

Coronal mass ejections

No Earth-directed Coronal Mass Ejections (CMEs) have been detected in the available coronagraph images.

Coronal holes

An equatorial positive polarity coronal hole is crossing the central meridian. A high-speed stream emanating from this coronal hole may impact the earth on July 10.

Solar wind

Slow solar wind conditions were recorded over the past 24 hours. The solar wind speed varied within 309 – 362 km/s. The interplanetary magnetic field varied between 2 nT and 6 nT, with the Bz reaching a minimum value of -5 nT. The phi-angle was mainly in the positive sector (directed away from the Sun) with periods in the negative sector. Slow solar wind conditions are expected in the next 24 hours.

Geomagnetism

Geomagnetic conditions were globally quiet (Kp 1-2) and locally quiet to unsettled (K_Bel 1-3). Quiet to unsettled conditions are expected in the next 24 hours.

Proton flux levels

Over the past 24 hours the greater than 10 MeV GOES proton flux was at background levels and is expected to remain so over the next days.

Electron fluxes at geostationary orbit

The greater than 2 MeV electron flux measured by GOES 16 was below the 1000 pfu threshold and is expected to remain so in the upcoming days. The 24h electron fluence was at nominal level and is expected to remain so in the next days.

Today's estimated international sunspot number (ISN): 126, based on 09 stations.

Solar indices for 06 Jul 2024

Wolf number Catania///
10cm solar flux166
AK Chambon La Forêt008
AK Wingst004
Estimated Ap004
Estimated international sunspot number121 - Based on 19 stations

Noticeable events summary

DayBeginMaxEndLocStrengthOP10cmCatania/NOAARadio burst types
06225223152335----M1.085/3738

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

All times in UTC

<< Go to daily overview page

Latest news

Support 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! Subscriptions
Donations
Support SpaceWeatherLive.com! Donate
Support SpaceWeatherLive with our merchandise
Check out our merchandise

Latest alerts

Get instant alerts!

Space weather facts

Last X-flare2026/02/04X4.21
Last M-flare2026/02/25M2.4
Last geomagnetic storm2026/03/03Kp5 (G1)
Spotless days
Last 365 days3 days
20263 days (5%)
Last spotless day2026/02/24
Monthly mean Sunspot Number
February 202678.2 -34.3
March 202675 -3.2
Last 30 days55.6 -70.1

This day in history*

Solar flares
12001M8.22
22011M7.57
32011M6.29
41999M3.73
52011M2.14
DstG
11970-284G5
21978-99G1
31994-87G2
41989-75G2
51986-64G1
*since 1994

Social networks