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Information
is compiled through the following agencies or sites.
NOAA
/ SWPC / SOHO / GOES / POES
/ ESA / NASA / ACE / SSC / SDO / AIA
consortium / HMI consortium
/ SWENET / U.S.A.F. / Lockheed Martin
/ SWAP / SIDC / GONG
The
Information contains the latest Solar and Geophysical Activity
from the NOAA Space Weather Prediction Center.
Information
is provided by synchronization using Siber
Systems, Inc GoodSync through several government FTP servers
to Scientific Frontline servers on a 03 minute interval.
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| Solar Region Summary |
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| Current Solar Videos |
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Videos
update every 3 hrs. Corresponding images update every 05 minutes
Requires
JAVA Scripts and Pop Up Windows Enabled Select individual movies below |
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| Combined and Event Tracking videos update every 12 to 24 hrs. Requires JAVA Scripts and Pop Up Windows Enabled | |||
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| Combined Solar | Event Tracking 1 | Event Tracking 2 | Event Tracking 3 |
| Space Weather Alerts Issued in the last 24 hours |
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| Geophysical Alert Message | |
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Click
Image for larger view
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| Solar and Geophysical Activity Summary |
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Satellite Environment 3 Day
Plot
Click
Image for larger view
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| Wing Kp Predicted Activity Index |
The top panel plot shows the two 1-hour and 4-hour Kp index model predictions and the corresponding confidence level. The solid horizontal green bar shows the 3-hour interval over which the latest predictions are valid. Error bars are plotted to show the 50% confidence interval. 1-hour prediction, plotted with filled-in circles 4-hour prediction, plotted in plus (+) symbols. Prediction points in the top panel are plotted at the model valid time (run time + Propagation time), which is usually 30-90 minutes into the future for the 1-hour prediction and 210-270 minutes into the future for the 4-hour prediction. The solid blue line is the Estimated Kp index. The dashed red line indicates the lowest alert level, G1 (minor), on the NOAA Space Weather Scale for Geomagnetic Storms. The predictions are color coded according to the amount of solar wind data that was available for each model run; green (most data) and yellow (little data). The bottom Lead Time panel shows an estimate of the actual lead time for the 1-hour and 4-hour predictions. The left plot legend shows the 1-hour lead time and the 4-hour lead time is shown on the right. The actual lead time depends on solar wind speed and can be greater than or less than one hour depending on the solar wind speed. The predictions are calculated using the ACE Real-Time solar wind speed data. The lead time is the time for the solar wind to propagate from the ACE satellite, at L1, to the Earth. Missing Kp values, Lead Time values, or model output indicates the data is not available. |
| Solar Wind Plasma |
| ACE DATA May 2012 |
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Scroll to end for current data |
| STEREO A DATA |
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Scroll to end for current data |
| STEREO B DATA |
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Scroll to end for current data |
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ACE 2
Hour Plot Magnetic field and Plasma Updated every 10 minutes
Click Image for
larger View
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Real-Time Solar
Wind data dials
Dials are updated
every 10 minutes with data averaged over last 15 minutes. The data are the Real-Time Solar Wind data broadcast from NASA's ACE satellite.
How
to read and understand the ACE Solar Wind dials
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| GONG Farside Image |
These
images are whole-Sun maps of magnetic activity. They show 360
degrees of longitude in the Carrington coordinate system normally
used for solar observations. The map extent is from south pole to
north pole in an equal area projection. The solar equator and
each 60 degrees of longitude are marked.The Earthside, or near-side, data are smoothed magnetic flux as measured by GONG. The images are shown to 70 degrees from disk center. Each magnetogram takes only one minute to observe. The farside images are maps of wave speed variations with locations of faster wave speed shown darker. These darker regions indicate locations where there is an accumulation of magnetic field on the far surface. The farside images can only be computed out to 45 degrees from the farside disk center as (un)seen from Earth. A full 24-hours of GONG surface velocity data is used to compute each image. |
| Current Space Weather Indices |
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| Auroral Activity |
Northern
Hemisphere
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Southern
Hemisphere
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This plot shows the
current extent and position of the auroral oval in the northern
and southern hemisphere, extrapolated from measurements taken
during the most recent polar pass of the NOAA POES satellite. The red arrow points toward the noon meridian. The statistical pattern depicting the auroral oval is appropriate to the auroral activity level determined from the power flux observed during the most recent polar satellite pass. The power fluxes in the statistical pattern are color coded on a scale from 0 to 10 ergs .cm-2.sec-1 according to the color bar on the right. The pattern has been oriented with respect to the underlying geographic map using the current universal time, updated every ten minutes. This presentation provides an estimate of the location, extent, and intensity of aurora on a global basis. For example, the presentation gives a guide to the possibility that the aurora is located near a given location in the northern and southern hemisphere under the conditions that existed at the time of the most recent polar satellite pass. Normalization factor (n) A normalization factor of less than 2.0 indicates a reasonable level of confidence in the estimate of power. The more the value of n exceeds 2.0, the less confidence should be placed in the estimate of hemispheric power and the activity level. The process to estimate the hemispheric power, and the level of auroral activity, involves using this normalization factor which takes into account how effective the satellite was in sampling the aurora during its transit over the polar region. A large (> 2.0) normalization factor indicates that the transit through the aurora was not very effective and the resulting estimate of auroral activity has a lower confidence. |
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| Report of Solar-Geophysical Activity |
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| Weekly Highlights and Forecasts |
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| Solar, Earth Atmospheric and Climate Gallery |
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Aqua
Series Intro
NEW
Jan.
16, 2012 An introduction to the groundbreaking scientific and practical applications of the Aqua satellite. |
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The
Solar Cycle
NEW
Jan.
13, 2012 The number of sunspots increases and decreases over time in a regular, approximately 11-year cycle, called the sunspot cycle. The exact length of the cycle can vary. It has been as short as eight years and as long as fourteen, but the number of sunspots always increases over time, and then returns to low again. |
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X-Class:
A Guide to Solar Flares
NEW
Jan.
11, 2012 Flares happen when the powerful magnetic fields in and around the sun reconnect. They're usually associated with active regions, often seen as sun spots, where the magnetic fields are strongest. Flares are classified according to their strength. The smallest ones are B-class, followed by C, M and X, the largest. |
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The
Truth About 2012
NEW
Jan.
10, 2012 Heliophysicist Alex Young explains why we won't need to worry about killer solar storms. |
| Latest Space Weather News |
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SDO:
Commissioning and Handover
May 18, 2010 In order to provide the clearest scientific data for its entire 5 year mission, SDO had to undergo a rigorous, 2 month testing phase. After giving it an all-clear, the team of people who designed, built and tested the satellite now have to say goodbye as they hand it over to the scientists who will begin collecting data. |
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Shocking
recipe for making killer electrons
Mar. 11, 2010 Take a bunch of fast-moving electrons, place them in orbit and then hit them with the shock waves from a solar storm. What do you get? Killer electrons. That’s the shocking recipe revealed by ESA’s Cluster mission. Killer electrons are highly energetic particles trapped in Earth's outer radiation belt, which extends from 12 000 km to 64 000 km above the planet’s surface. |
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| Other Current Data |
| Coming Soon |
| Special Notices |
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GOES 15 Designated
Primary X-ray Satellite
October 28, 2010 --
GOES 15 replaced GOES 14 as the Primary SWPC GOES
X-ray Satellite. GOES
14 is being moved into storage. There is no
Secondary SWPC GOES
X-ray satellite.
X-ray ascii data files use the file naming convention 'Gp' for GOES Primary, this means only header lines changes. ========================================================================= At 0000UT OCTOBER 28 GOES 15 Will Replace GOES 14 as Primary Satellite for XRS data October 13, 2010: At 0000 UT October 28 GOES 15 will replace GOES 14 as the Primary SWPC GOES X-ray Satellite. GOES 14 is being moved into storage. There is no Secondary SWPC GOES X-ray satellite. X-ray ascii data files use the file naming convention 'Gp' for GOES Primary, this means only header lines changes. |
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