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Contact Information: Dr. Howard J. Singer, Chief Research and Development Division NOAA Space Environment Center 325 Broadway Boulder, CO 80305 303-497-6959.

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Presentation on theme: "Contact Information: Dr. Howard J. Singer, Chief Research and Development Division NOAA Space Environment Center 325 Broadway Boulder, CO 80305 303-497-6959."— Presentation transcript:

1 Contact Information: Dr. Howard J. Singer, Chief Research and Development Division NOAA Space Environment Center 325 Broadway Boulder, CO 80305 303-497-6959 303-497-5388 howard.singer@noaa.gov

2 GOES Space Environment Monitor (SEM) NOAA Space Environment Center (SEC) Current GOES SEM Instruments and Societal Benefits GOES-R+ SEM Instrument Baseline and Improvements Trade Studies and User Input GOES Users’ Conference Boulder, CO May 22, 2001 H. J. Singer, NOAA Space Envrionment Center

3 SEC Mission Statement The Space Environment Center is the Nation’s official source of space weather alerts and warnings. The Center continually monitors and forecasts Earth’s space environment; provides accurate, reliable, and useful solar terrestrial information; and leads programs to improve services. To serve the Nation and reduce the adverse effects of space weather disturbances on human activities: SEC synthesizes and disseminates information about past, present, and future conditions in the space environment for space weather users and private industry vendors; we prepare the data we acquire for the national archive. SEC leads in development and implementation of programs in solar-terrestrial physics and space environment services by conducting research and developing techniques that improve monitoring and forecasting. SEC uses its expertise to advise and educated those who operate systems affected by disturbances in the space environment and those who have general interest in our science. GOES Observations are a Key Component of SEC Mission

4 Space Weather Operations Forecast Center Nation’s official source of Space Weather alerts, warnings, and forecasts Synthesis of space environment data and information Works together with Research and Development to bring new understanding, models, and data into operations GOES Observations Critical to Space Weather Operations

5 NOAA Space Weather Scale Summary Extreme Severe Strong Moderate Minor Geomagnetic Storms Solar Radiation Storms Radio Blackouts  High Radiation Hazard  Power Grid Instability  HF Blackout for an Hour  Infrequent SEU  Minor Impact on Satellites Measures: Kp Geomagnetic GOES >10 MeV p GOES X-Rays Index

6 GOES Space Environment Monitor Measurements of energetic particles, magnetic field, solar x-rays, and solar EUV provide data of practical benefit to commercial and government activities and for extensive basic research.

7 NOAA Geostationary Operational Environmental Satellite (GOES) Instrumentation for SEC Satellites: GOES 8 (Launch: 4/13/94, Operational) GOES 9 (Launch: 5/23/95, On-orbit storage) (Launch: 4/25/97, Operational) GOES 11 (Launch 5/13/00, On-orbit storage) GOES M (Launch planned July 01) GOES NO/PQ (HSC in production, launch start 03) GOES 10 Space Environment Monitor (SEM) Energetic Particle Sensor (EPS) Monitors the energetic electron, proton, and alpha particle fluxes e: 0.03-4.0 MeV, p: 0.08-700 MeV, a: 4-3400 MeV Magnetometer (MAG) Monitors the vector magnetic field 0.512 second samples, ~0.1 nT sensitivity, +/- 1000 nT X-Ray & Extreme UltraViolet Sensors (XRS/EUV) Monitors whole-Sun x-ray brightness in two bands 1 - 8 Angstroms and 0.5 - 4 Angstroms 5 EUV Bands

8 GOES Energetic Particle Sensor: Mitigation of International Space Station Radiation Risks Space Radiation Analysis Group NASA Johnson Space Center Michael J. Golightly GOES Measurements of Radiation to Astronauts: Radiation Belt Enhancements: electrons: > 500 keV Solar Energetic Protons: protons: > 10 MeV Heavy Ion Measurements Needed: C-N-O and Iron “Highest priority space weather need for NASA SRAG is a “Healthy” NOAA SEC…” M. Golightly, NASA/SRAG

9 YOHKOH GOES Magnetometer Monitors Solar Wind Shock Impact and Magnetopause Crossings at Geosynchronous Orbit Magnetopause Crossings Shock Geosynchronous Assets Magnetopause crossings interfere with satellite operations. As of a May 2000 report, 138 insured satellites in geosynchronous orbit valued at $20.1 B. “Space weather suggested as cause or contributor to over $500 M in insurance claims in past 4 years. “ U.S. Aviation Underwriters, Inc

10 movie GOES 8 During July 2000 Geomagnetic Storm Model movie illustrating extreme changes in magnetic field and plasma environment at geosynchronous.

11 XRS Products and User Needs Status: XRS provides the primary standard for solar flare magnitude Real-time XRS data provides the first indications of solar flare activity Prediction of probability of energetic proton event Estimation of region and severity of short-wave radio fade Used by both NOAA/SEC and the Air Force 55 th Weather Squadron Forecast Alerts and Warnings are sent out based on the initial XRS measurements of a flare. - Alerts and Warnings are sent when XRS sees flux of >M5.0 and >X1.0 Solar Proton Prediction Product: http://sec.noaa.gov/~sgreer/gprot/index.html HF Absorption Product: http://sec.noaa.gov/rt_plots/dregion.html

12 Extreme UltraViolet Sensor (EUV) Recent Improvement (GOES NOPQ) - Include five EUV channels Enhanced Services - Improved orbit prediction for low- earth orbit - Improved ionospheric parameterization for navigation and communication - Better predictions of ionospheric and thermospheric conditions USA Japan ESA Ionosphere L1 L2 GPS Receiver GPS Hubble Thermospheric Density variations cause orbit instabilities or even re-entry Ionospheric variations cause navigation errors in GPS 1995 2000 2005 Altitude (nautical miles) Year 200 260 320 Predicted Hubble Altitude G. Withbroe, NASA

13 GOES R+ SEM Instrument Proposed Improvements MeasurementSpecificationsProducts Magnetospheric Energetic Particles (EPEAD, MAGPD, MAGED) Protons: 30 * keV (was 80 KeV) to 0.8 MeV (*spec was in initial GOES NO/PQ requirement) Improved specification of medium energy radiation environment responsible for spacecraft charging Earth’s Magnetic Field (MAG) No Changes Soft x-ray emissions from the integrated solar disk (XRS) Dynamic Range 200,000 (was 100,000) Improved quality covering full solar dynamic range Extreme ultraviolet emissions from the integrated solar disk (EUVS) Eight EUV bands between 5 and 120 nm (was 5 bands) Improved height resolution in calculations of thermospheric heating rates and ionization rates; critical components in the modeling of the ionosphere and thermosphere

14  GOES Space Environment Monitor measurements provide crucial data to our nation and the world for commercial and government applications and for basic research  NOAA services must expand to meet the needs of our nation’s increasing use of and reliance on the space environment  Baseline requirements and proposed enhancements have been defined  Plans are underway for additional trade studies and User / Instrument-provider / Partnership workshops that are needed to determine the highest priority needs and implementation strategy Summary


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