Space Weather Guide


For updates and breaking Space Weather news follow Space Weather on Twitter.

What is Space Weather?

Most of the time space, weather is of little concern in our everyday lives. However, when the space environment is disturbed by the variable output of particles and radiation from the Sun, technologies that we depend on in our daily life, in space orbit as well as on the ground, can be affected. Some of the most dramatic space weather effects occur in association with eruptions of material from the solar atmosphere into interplanetary space. Thus, our space weather is a consequence of the behavior of the Sun, the nature of Earth's magnetic field and atmosphere, and our location in the solar system. The increasing deployment of radiation -current- and field sensitive technological systems over the last few decades and the increasing presence of complex systems in space combine to make society more vulnerable to solar-terrestrial disturbances. This has been emphasized by the large number of problems associated with the severe magnetic storms between 1989 and 1991 as the 11 year solar activity cycle peaked.

SOHO Real-time View of the Sun

Space Weather Outlook

Joint USAF/NOAA Solar Geophysical Activity Report and Forecast 1 February 2015

 

Joint USAF/NOAA Solar Geophysical Activity Report and Forecast

SDF Number 32 Issued at 2200Z on 01 Feb 2015

 

IA.  Analysis of Solar Active Regions and Activity from 31/2100Z to 01/2100Z: Solar activity has been at low levels for the past 24 hours. The largest solar event of the period was a C3 event observed at 01/1133Z from Region 2268 (S11W57). There are currently 6 numbered sunspot regions on the disk.

 

IB.  Solar Activity Forecast: Solar activity is likely to be moderate with a slight chance for an X-class flare on days one, two, and three (02 Feb, 03 Feb, 04 Feb).

 

IIA.  Geophysical Activity Summary 31/2100Z to 01/2100Z: The geomagnetic field has been at quiet to active levels for the past 24 hours. Solar wind speed, as measured by the ACE spacecraft, reached a peak speed of 748 km/s at 01/2006Z. Total IMF reached 14 nT at 01/0548Z. The maximum southward component of Bz reached -9 nT at 01/1946Z.

 

IIB.  Geophysical Activity Forecast: The geomagnetic field is expected to be at unsettled to minor storm levels on day one (02 Feb), quiet to active levels on day two (03 Feb) and quiet to unsettled levels on day three (04 Feb). Protons have a slight chance of crossing threshold on day one (02 Feb) and have a slight chance of crossing threshold on days two and three (03 Feb, 04 Feb).

 

III.  Event probabilities 02 Feb-04 Feb

Class M    60/55/55

Class X    20/15/15

Proton     20/15/15

PCAF       green

 

IV.  Penticton 10.7 cm Flux

Observed           01 Feb 142

Predicted   02 Feb-04 Feb 135/125/125

90 Day Mean        01 Feb 153

 

V.  Geomagnetic A Indices

Observed Afr/Ap 31 Jan  006/006

Estimated Afr/Ap 01 Feb  015/019

Predicted Afr/Ap 02 Feb-04 Feb  016/020-012/015-010/012

 

VI.  Geomagnetic Activity Probabilities 02 Feb-04 Feb

A.  Middle Latitudes

Active                45/35/20

Minor Storm           25/10/05

Major-severe storm    05/01/01

B.  High Latitudes

Active                10/15/20

Minor Storm           25/35/35

Major-severe storm    70/45/30

 

NOAA/SEC Satellite Environment

GOES X-Ray Flux

Dst Geomagnetic Index Estimate

Auroral Activity Extrapolated from NOAA POES

Low:

Dst > -20 nT

Medium:

-20 nT > Dst > -50 nT

High:

High: -50 nT > Dst > -100 nT

Extreme:

Dst < -100 nT

SOHO CELIAS/MTOF Proton Monitor

ACE Solar Wind Real-Time Data



Note: Images and text on this page are provided by NASA/ESA SOHO website. Space Weather Today from NOAA's Space Environment Center.