Viendo archivo del sábado, 2 junio 2012
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 2012 Jun 02 2200 UTCPreparado por NOAA © SWPC y procesado por SpaceWeatherLive.com
Informe conjunto USAF/NOAA de actividad Solar y Geofísica
SDF Número 154 Publicado el 2200Z a las 02 Jun 2012IA. Análisis de regiones solares activas y de actividad desde 01-2100Z hasta 02-2100Z Solar activity was low. A C3 flare was observed from
the west limb at 01/2241Z. It was accompanied by a Type II radio
emission (936 km/s) and a non-earth-directed CME. Region 1498
(N08E55) produced a C2 flare at 02/0105Z and 1493 (N15E35) produced
C1 flare at 02/0431Z. New flux emerged near S12W40 and N17E65. All
eight regions on the disk exhibited simple beta magnetic
characteristics.
IB. Pronóstico de la actividad solar
Solar activity is expected to be low
with a slight chance for an M-class flare.
IIA. Resumen de la actividad geofísica 01-2100Z a 02-2100Z
The geomagnetic field was primarily quiet for the first half of the
day, increasing to unsettled levels during the 15-18Z synoptic
period. At the ACE spacecraft, low energy particles detected by the
EPAM instrument began rising about 02/06Z, finally leveling off
around 02/14Z. Bz began turning southward around 02/1410Z,
decreasing to around -7 nT where it remained. The solar sector
switched from negative to positive at the same time. Solar wind
speed ranged between 340 and 360 km/s.
IIB. Pronóstico de la actividad geofísica
The geomagnetic field is
expected to begin at quiet to unsettled levels, with a chance for an
isolated active period on day one (3 June). Activity is expected to
increase to unsettled levels on day two (4 June) and active levels
on day three (5 June), with a chance for minor storm periods both
days. The disturbance is expected as a recurrent coronal hole high
speed stream becomes geoeffective.
III. Probabilidades del evento 03 Jun a 05 Jun
| Clase M | 10% | 10% | 10% |
| Clase X | 01% | 01% | 01% |
| Protón | 01% | 01% | 01% |
| PCAF | green | ||
IV. Penticton 10.7cm flujo
Observado 02 Jun 129 Previsto 03 Jun-05 Jun 130/130/130 Media de 90 Días 02 Jun 117
V. Índices Geomagnéticos A
Observado Afr/Ap 01 Jun 006/006 Estimado Afr/Ap 02 Jun 006/007 Previsto Afr/Ap 03 Jun-05 Jun 009/010-013/015-015/020
VI. Probabilidades de Actividad Geomagnética 03 Jun a 05 Jun
| A. Latitudes Medias | |||
|---|---|---|---|
| Activo | 20% | 35% | 35% |
| Tormenta Menor | 10% | 20% | 20% |
| Tormenta Mayor-Severa | 01% | 05% | 05% |
| B. Latitudes Altas | |||
|---|---|---|---|
| Activo | 15% | 10% | 10% |
| Tormenta Menor | 25% | 30% | 25% |
| Tormenta Mayor-Severa | 30% | 50% | 50% |
< < Ir a la visión general diaria
Últimas noticias
lunes, 22 abril 2024
Lot's of sunspots! Big chance for major flare activity?
sábado, 23 marzo 2024
X1.1 solar flare with earth-directed CME
miércoles, 20 marzo 2024
Sunspot region 3615, G1 watch
Últimos mensajes del foro
IMF - BT strength 2What are these long and thin eruptions? 3AR 3637, 3638, 3643 89Unproven theories 341Space Weather Memes 338
Más temasApoye 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!
Hechos clima espacial
| Último evento clase X | 2024/03/28 | X1.1 |
| Último evento clase M | 2024/04/25 | M1.3 |
| Últimas tormentas geomagnéticas | 2024/04/19 | Kp7 (G3) |
| Días sin manchas | |
|---|---|
| Último día sin manchas | 2022/06/08 |
| Promedio de manchas solares mensuales | |
|---|---|
| marzo 2024 | 104.9 -19.8 |
| Last 30 days | 133.9 +26.6 |