Viendo archivo del jueves, 19 junio 2003

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 2003 Jun 19 2200 UTC
Preparado por NOAA © SWPC y procesado por SpaceWeatherLive.com

Informe conjunto USAF/NOAA de actividad Solar y Geofísica

SDF Número 170 Publicado el 2200Z a las 19 Jun 2003

IA. Análisis de regiones solares activas y de actividad desde 18-2100Z hasta 19-2100Z

Solar activity decreased to very low levels. Flare activity was limited to several B-class flares. Region 386 (S07E30) lost penumbral coverage over the period although it does retain a delta magnetic structure in the dominant lead spot. Region 387 (N18E49) grew in both penumbral coverage and magnetic complexity since yesterday, a gamma structure is now evident in the trailing portion of the spot group. Newly numbered Region 388 (S03E08) produced a minor B-class flare early in the period.
IB. Pronóstico de la actividad solar
Solar activity is expected to be at moderate levels. Region 386 remains capable of producing an isolated major flare.
IIA. Resumen de la actividad geofísica 18-2100Z a 19-2100Z
The geomagnetic field was at predominantly active levels today. Minor storm conditions were observed at both middle and high latitudes between 19/0000 and 0300Z due to the influence of a recurrent high speed coronal hole stream. The greater than 10 MeV proton flux exceeded event threshold at 18/2050Z (reached a max of 24 pfu at 19/0450Z), ended at 19/1900Z and after careful review the event is believed to have been the result of the M6.8 x-ray flare from June 17. The greater than 2 MeV electron flux reached moderate levels today.
IIB. Pronóstico de la actividad geofísica
The geomagnetic field is expected to be at predominantly unsettled to active levels through the interval. Minor storm conditions may exist due to a transient passage during the first half of day one in response to the M6.8 x-ray flare from June 17.
III. Probabilidades del evento 20 Jun a 22 Jun
Clase M50%50%50%
Clase X15%15%15%
Protón25%15%15%
PCAFgreen
IV. Penticton 10.7cm flujo
  Observado       19 Jun 123
  Previsto   20 Jun-22 Jun  125/125/125
  Media de 90 Días        19 Jun 124
V. Índices Geomagnéticos A
  Observado Afr/Ap 18 Jun  036/054
  Estimado     Afr/Ap 19 Jun  023/025
  Previsto    Afr/Ap 20 Jun-22 Jun  020/025-020/025-012/020
VI. Probabilidades de Actividad Geomagnética 20 Jun a 22 Jun
A. Latitudes Medias
Activo40%40%25%
Tormenta Menor15%15%10%
Tormenta Mayor-Severa10%10%05%
B. Latitudes Altas
Activo50%50%40%
Tormenta Menor20%20%15%
Tormenta Mayor-Severa10%10%10%
PLAIN GOES Protons: To ensure continued operational monitoring of important energetic particle data, it is necessary to reassign primary/secondary designations for the GOES Space Environment Monitor (SEM) detectors. GOES 11 (113W) is now the primary satellite for protons. GOES 12 will continue as the primary satellite for magnetometer, X-ray, and electron measurements. GOES 10 (135W) will be the secondary satellite for all SEM sensors - magnetometer, X-ray, and energetic particles. Because of the degraded state of the proton data on GOES-10, its designation as the secondary source for proton data is a short-term solution. More permanent solutions have been identified and are being evaluated. Users will be notified when we define and schedule a permanent fix. Further details can be found at http://www.sec.noaa.gov/GOES.html. K-Indices: On 16 June, it was determined that a scaling problem exists with the Boulder magnetometer instrument. While this problem, and its fix are being investigated the primary instrument for Boulder K-indices has been switched to the Boulder USGS (via Domsat) magnetometer, effective 1500 UTC on 16 June. 99999

< < Ir a la visión general diaria

Últimas noticias

Apoye a SpaceWeatherLive.com!

Mucha gente viene a SpaceWeatherLive para seguir la actividad del Sol o previsión de aurora, pero con esta cantidad de tráfico se incrementan los costos del servidor. ¡Considere hacer una donación si disfruta de SpaceWeatherLive para que podamos mantener el sitio web en línea!

44%
Apoya a SpaceWeatherLive con nuestro merchandise
Échale un ojo a nuestro merchandise

Hechos clima espacial

Último evento clase X2024/03/28X1.1
Último evento clase M2024/04/19M1.0
Últimas tormentas geomagnéticas2024/04/19Kp7 (G3)
Días sin manchas
Último día sin manchas2022/06/08
Promedio de manchas solares mensuales
marzo 2024104.9 -19.8

Efemérides*

Llamarada solar
12022X2.25
22022M7.29
32001M5.99
41998M1.96
52022M1.9
ApG
1200270G3
2201843G2
3201728G2
4201422G1
5201116G1
*desde 1994

Redes sociales