Real Time Solar Wind (RTSW)
Geomagnetic storms are a natural hazard, like hurricanes and tsunamis,
which the
National Oceanic and Atmospheric Administration (NOAA)
forecasts for the public's benefit. Severe geomagnetic storms cause
communications problems, abruptly increase drag on spacecraft, and can
cause electric utility blackouts over a wide area. The location of ACE at
the L1 libration point between the earth and the sun enables ACE to
give about a one hour advance warning of impending geomagnetic activity.
NOAA has arranged for the transmission of a subset of data from four
ACE instruments during the times when ACE is not transmitting it's full
telemetry to the Deep Space Network. For about 21 of 24 hours per day,
ACE will send data (~464 bps) to NOAA operated ground stations. During the
other three hours when NASA is getting high rate data through the Deep
Space Network, NOAA gets a copy of the real time data. NOAA
processes the data (using algorithms provided by the ACE experimenters)
at its Space Environment Services Center (SESC) in Boulder, Colorado,
which will issue any alerts of impending high geomagnetic activity.
The four ACE instruments and the data they will supply are:
- EPAM - Energetic Ions and Electrons
- SWEPAM - Solar Wind Ions
- MAG - Magnetic Field Vectors
- SIS - High Energy Particle Fluxes
Return to ACE Home Page
Author and Curator: Eric R.
Christian (erc@cosmicra.gsfc.nasa.gov)
Responsible NASA Official: Tycho von Rosenvinge
(tycho@lheamail.gsfc.nasa.gov)
A service of the
Laboratory for High Energy Astrophysics (LHEA) at
NASA's
GSFC
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This file was last modified on
Thursday, 15-Feb-2001 11:50:24 EST