Viendo archivo del martes, 15 enero 2002
Informe actividad solar
Any mentioned solar flare in this report has a scaling factor applied by the Space Weather Prediction Center (SWPC). Because of the SWPC scaling factor, solar flares are reported as 42% smaller than for the science quality data. The scaling factor has been removed from our archived solar flare data to reflect the true physical units.
Informe de actividad Solar-Geofísica 2002 Jan 15 2200 UTCPreparado por NOAA © SWPC y procesado por SpaceWeatherLive.com
Informe conjunto USAF/NOAA de actividad Solar y Geofísica
SDF Número 015 Publicado el 2200Z a las 15 Jan 2002IA. Análisis de regiones solares activas y de actividad desde 14-2100Z hasta 15-2100Z Solar activity has been moderate. Region 9775 (S06W69)
was most active, producing an M1/Sf event at 14/2246 UTC, and
several other subfaint C-class flares during the period. This
region is exhibiting some growth in magnetic complexity and areal
coverage as it approaches the west limb. Other sources of weak
C-class flare activity during the period included Regions 9782
(N06E20) and 9773 (N16W80).
IB. Pronóstico de la actividad solar
Solar activity is expected to be low
to moderate.
IIA. Resumen de la actividad geofísica 14-2100Z a 15-2100Z
The geomagnetic field has been quiet. Particle fluxes for both >2MeV
electrons and >10MeV protons reached event levels during the period.
>2MeV electrons briefly exceeded 1000 pfu at geosynchronous orbit
near local noon, as measured on GOES-8, during 15/1405-1615 UTC. A
proton event for >10MeV flux reached event threshold of 10 pfu at
15/1435 UTC, and remains in progress with a current flux of about 12
pfu. The slow enhancement in proton flux is likely from the west
limb CME event of 14 January, with the delay in enhancement due to
the intervening effects of a coronal hole high speed stream.
IIB. Pronóstico de la actividad geofísica
Geomagnetic field activity is
expected to be mainly quiet with some isolated unsettled periods.
The >10MeV proton event is expected to end during the first day of
the period.
III. Probabilidades del evento 16 Jan a 18 Jan
| Clase M | 75% | 75% | 75% |
| Clase X | 20% | 15% | 15% |
| Protón | 90% | 30% | 15% |
| PCAF | yellow | ||
IV. Penticton 10.7cm flujo
Observado 15 Jan 218 Previsto 16 Jan-18 Jan 220/215/220 Media de 90 Días 15 Jan 224
V. Índices Geomagnéticos A
Observado Afr/Ap 14 Jan 007/008 Estimado Afr/Ap 15 Jan 006/007 Previsto Afr/Ap 16 Jan-18 Jan 007/010-010/010-010/008
VI. Probabilidades de Actividad Geomagnética 16 Jan a 18 Jan
| A. Latitudes Medias | |||
|---|---|---|---|
| Activo | 15% | 20% | 20% |
| Tormenta Menor | 10% | 10% | 10% |
| Tormenta Mayor-Severa | 01% | 01% | 01% |
| B. Latitudes Altas | |||
|---|---|---|---|
| Activo | 25% | 25% | 20% |
| Tormenta Menor | 15% | 15% | 10% |
| Tormenta Mayor-Severa | 01% | 01% | 01% |
All times in UTC
< < Ir a la visión general diaria
Últimas noticias
miércoles, 31 diciembre 2025
Happy New Year! Celebrate with an M7.1 solar flare!
domingo, 7 diciembre 2025
M8.1 solar flare with earth-directed CME
lunes, 1 diciembre 2025
X1.9 solar flare, Coronal hole faces Earth
Últimos mensajes del foro
Más temasApoye 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!
Hechos clima espacial
| Último evento clase X | 08/12/2025 | X1.1 |
| Último evento clase M | 31/12/2025 | M7.11 |
| Últimas tormentas geomagnéticas | 02/01/2026 | Kp5 (G1) |
| Días sin manchas | |
|---|---|
| Último día sin manchas | 08/06/2022 |
| Promedio de manchas solares mensuales | |
|---|---|
| diciembre 2025 | 124 +32.2 |
| enero 2026 | 112.1 -11.9 |
| Last 30 days | 104.6 -5 |