Viendo archivo del martes, 28 julio 2020

Daily bulletin on solar and geomagnetic activity from the SIDC

Emitido: 2020 Jul 28 1231 UTC

SIDC Forecast

Valid from 1230 UTC, 28 Jul 2020 until 30 Jul 2020
Llamarada solar

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

Geomagnetism

Quiet (A<20 and K<4)

Protones solares

Quiet

10cm fluxAp
28 Jul 2020071006
29 Jul 2020071004
30 Jul 2020071003

Bulletin

The solar activity remained at very low levels with no significant solar flares over the past 24 hours. The visible unipolar sunspot region (Catania 37, N0AA-AR 2767) remained stable and continued to decay. A new currently unclassified sun spot group is now appearing on the solar disc from the north-east limb. The X-ray flux is observed below B-class level and the solar activity is expected to remain at low levels over the next 24 hours.

No Earth directed Coronal Mass Ejections (CMEs) were observed in the available coronagraph imagery.

The greater than 10 MeV proton flux was at background levels over the past 24 hours and is expected to remain so for the next 24 hours. The greater than 2 MeV electron flux was at moderate to background levels over the past 24 hours and is expected to remain so in the next 24 hours. The solar wind parameters (ACE and DSCOVR) were at low to slightly enhanced levels over the past 24 hours. The total interplanetary magnetic field was weak with values of 3-7 nT. The north-south Bz component fluctuated between -4 nT and 5 nT. In the past 24 hours the Phi angle remained mostly negative under the ongoing influence of the negative polarity equatorial coronal hole which crossed the central meridian on July 23rd. The solar wind speed gradually varied between 360 km/s and 440 km/s, reaching maximum at 22:00 UTC last night. This interval coincides with the switch of polarity of the Bz component from positive to negative direction and the beginning of an isolated period of positive Phi angle. The solar wind conditions are expected to remain quiet to slightly enhanced for the next day under the remaining influence of the HSS, originating from the discussed negative polarity coronal hole.

The geomagnetic conditions were quiet with maximum global Kp-NOAA and local K-Dourbes indices equal to 2. Mostly quiet conditions are expected for the next 24 hours.

Today's estimated international sunspot number (ISN): 019, based on 21 stations.

Solar indices for 27 Jul 2020

Wolf number Catania///
10cm solar flux071
AK Chambon La Forêt009
AK Wingst004
Estimated Ap003
Estimated international sunspot number010 - Based on 34 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

< < Ir a la visión general diaria

Últimas noticias

Apoye a 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! Suscripciones
Donations
Apoye a SpaceWeatherLive.com! Donar
Apoya a SpaceWeatherLive con nuestro merchandise
Échale un ojo a nuestro merchandise

Hechos clima espacial

Último evento clase X18/01/2026X1.9
Último evento clase M21/01/2026M3.4
Últimas tormentas geomagnéticas22/01/2026Kp5+ (G1)
Días sin manchas
Último día sin manchas08/06/2022
Promedio de manchas solares mensuales
diciembre 2025124 +32.2
enero 2026119.1 -4.9
Last 30 days122.3 +12.7

Efemérides*

Llamarada solar
12023M4.65
21999M3.8
32023M2.0
41998M1.8
52023M1.4
DstG
12004-81G2
21957-81G1
32012-75
41974-66G2
51979-66G2
*desde 1994

Redes sociales