Space Weather Observations, Alerts, and Forecast

3-day Solar-Geophysical Forecast issued Jun 05 22:00 UTC

Solar Activity Forecast:
Solar activity is expected to remain very low with only a slight chance for an isolated C-class flare.

Geophysical Activity Forecast:
The geomagnetic field is expected to remain mostly quiet with isolated periods of unsettled conditions on day 1 (6 June) due to elevated solar wind speeds and brief periods of Bz south. Quiet to unsettled with intermittent periods of active conditions are expected on days 2 and 3 (7-8 June). The increase in activity is due in part to weak coronal hole effects expected on 7 June as well as the possible arrival of a slow moving CME on 8 June. The CME is from a filament that disappeared on 3 June. A weak halo can be observed on LASCO C3 coronagraph images from early 4 June as well as STEREO A and B coronagraphs from the same period.

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Real Time Images of the Sun

Click for time-lapse image of the sun
SOHO EIT 284 image of the sun
Mauna Loa Solar Image
Latest Mauna Loa image of the Sun

The sun is constantly monitored for sun spots and coronal mass ejections. EIT (Extreme ultraviolet Imaging Telescope) images the solar atmosphere at several wavelengths, and therefore, shows solar material at different temperatures. In the images taken at 304 Angstrom the bright material is at 60,000 to 80,000 degrees Kelvin. In those taken at 171 Angstrom, at 1 million degrees. 195 Angstrom images correspond to about 1.5 million Kelvin, 284 Angstrom to 2 million degrees. The hotter the temperature, the higher you look in the solar atmosphere.

Real Time Solar X-ray and Solar Wind

Solar Cycle Progression
Graph showing current solar cycle progression
Solar Cycle chart updated using the latest ISES predictions.
Real-Time Solar Wind
Graph showing Real-Time Solar Wind
Real-Time Solar Wind data broadcast from NASA's ACE satellite.

The Solar Cycle is observed by counting the frequency and placement of sunspots visible on the Sun. Solar minimum occurred in December, 2008. Solar maximum is expected to occur in May, 2013.

Solar X-ray Flux
Graph showing Real-Time Solar X-ray Flux
This plot shows 3-days of 5-minute solar x-ray flux values measured on the SWPC primary and secondary GOES satellites.
Satellite Environment Plot
Graph showing Real-Time Satellite Environment Plot
The Satellite Environment Plot combines satellite and ground-based data to provide an overview of the current geosynchronous satellite environment.

Auroral Activity Extrapolated from NOAA POES

Northern Hemi Auroral Map
Current Northern hemispheric power input map
Southern Hemi Auroral Map
Current Southern hemispheric power input map

Instruments on board the NOAA Polar-orbiting Operational Environmental Satellite (POES) continually monitor the power flux carried by the protons and electrons that produce aurora in the atmosphere. SWPC has developed a technique that uses the power flux observations obtained during a single pass of the satellite over a polar region (which takes about 25 minutes) to estimate the total power deposited in an entire polar region by these auroral particles. The power input estimate is converted to an auroral activity index that ranges from 1 to 10.

3 Day Report of Solar & Geophysical Activity

Prepared jointly by the U.S. Dept. of Commerce, NOAA,
Space Weather Prediction Center and the U.S. Air Force.

Updated 2014 Nov 28 2200 UTC

Joint USAF/NOAA Solar Geophysical Activity Report and Forecast
SDF Number 332 Issued at 2200Z on 28 Nov 2014

IA.  Analysis of Solar Active Regions and Activity from 27/2100Z to
28/2100Z: Solar activity has been at low levels for the past 24 hours.
The largest solar event of the period was a C7 event observed at
28/0040Z from Region 2222 (S20E44). There are currently 8 numbered
sunspot regions on the disk.

IB.  Solar Activity Forecast: Solar activity is expected to be low with
a chance for M-class flares on days one, two, and three (29 Nov, 30 Nov,
01 Dec).

IIA.  Geophysical Activity Summary 27/2100Z to 28/2100Z: The geomagnetic
field has been at quiet to unsettled levels for the past 24 hours. Solar
wind speed, as measured by the ACE spacecraft, reached a peak speed of
412 km/s at 28/1242Z. Total IMF reached 13 nT at 28/1459Z. The maximum
southward component of Bz reached -11 nT at 28/1215Z. Electrons greater
than 2 MeV at geosynchronous orbit reached a peak level of 439 pfu.

IIB.  Geophysical Activity Forecast: The geomagnetic field is expected
to be at quiet levels on days one and two (29 Nov, 30 Nov) and quiet to
active levels on day three (01 Dec).

III.  Event probabilities 29 Nov-01 Dec
Class M    40/45/50
Class X    05/05/05
Proton     05/05/05
PCAF       green

IV.  Penticton 10.7 cm Flux
Observed           28 Nov 181
Predicted   29 Nov-01 Dec 185/185/185
90 Day Mean        28 Nov 151

V.  Geomagnetic A Indices
Observed Afr/Ap 27 Nov  007/005
Estimated Afr/Ap 28 Nov  004/006
Predicted Afr/Ap 29 Nov-01 Dec  006/005-006/005-011/015

VI.  Geomagnetic Activity Probabilities 29 Nov-01 Dec
A.  Middle Latitudes
Active                10/10/25
Minor Storm           01/01/05
Major-severe storm    01/01/01
B.  High Latitudes
Active                15/15/15
Minor Storm           20/20/25
Major-severe storm    10/10/30

Photo compliments of NOAA


Space Weather Images and Information (excluded from copyright) courtesy of: NOAA / NWS Space Weather Prediction Center, Mauna Loa Solar Observatory (HAO/NCAR), and SOHO (ESA & NASA).

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