Space Weather Guide


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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 2 August 2015

Joint USAF/NOAA Solar Geophysical Activity Report and Forecast
SDF Number 214 Issued at 2200Z on 02 Aug 2015

IA. Analysis of Solar Active Regions and Activity from 01/2100Z to 02/2100Z: Solar activity has been at very low levels for the past 24 hours. There are currently 4 numbered sunspot regions on the disk.

IB. Solar Activity Forecast: Solar activity is expected to be very low with a chance for a C-class flares on days one, two, and three (03 Aug, 04 Aug, 05 Aug).

IIA. Geophysical Activity Summary 01/2100Z to 02/2100Z: 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 674 km/s at 02/1106Z. Total IMF reached 6 nT at 02/0251Z. The maximum southward component of Bz reached -5 nT at 02/0126Z. Electrons greater than 2 MeV at geosynchronous orbit reached a peak level of 720 pfu.

IIB. Geophysical Activity Forecast: The geomagnetic field is expected to be at quiet to unsettled levels on days one and two (03 Aug, 04 Aug) and quiet levels on day three (05 Aug).

III. Event probabilities 03 Aug-05 Aug
Class M 05/01/01
Class X 01/01/01
Proton 01/01/01
PCAF green

IV. Penticton 10.7 cm Flux
Observed 02 Aug 102
Predicted 03 Aug-05 Aug 100/100/100
90 Day Mean 02 Aug 117

V. Geomagnetic A Indices
Observed Afr/Ap 01 Aug 009/010
Estimated Afr/Ap 02 Aug 011/012
Predicted Afr/Ap 03 Aug-05 Aug 009/010-007/008-006/005

VI. Geomagnetic Activity Probabilities 03 Aug-05 Aug
A. Middle Latitudes
Active 15/15/10
Minor Storm 05/05/05
Major-severe storm 01/01/01
B. High Latitudes
Active 20/20/15
Minor Storm 30/25/20
Major-severe storm 25/20/15

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.