NOAA Space Environmental Data Paper 2.3 - AMS W.F. Denig National Geophysical Data Center Boulder, CO Monday, 03 Feb 14 / 2:00 PM.

Slides:



Advertisements
Similar presentations
NOAAs Comprehensive Large-data Array Stewardship System (CLASS) Robert Rank NOAA CLASS Program Chris Elvidge – NOAA-NGDC January 22, 2006.
Advertisements

Cosmic Rays and Space Weather
Space Weather in CMA Xiaonong Shen Deputy Administrator China Meteorological Administration 17 May 2011 WMO Cg-XVI Side Event Global Preparedness for Space.
Space Weather Effects on Satellite Communications Tim Deaver Vice President, Hosted Payload Development June 21, 2011.
Terrance G Onsager and Rodney Viereck
Cosmic Ray Using for Monitoring and Forecasting Dangerous Solar Flare Events Lev I. Dorman (1, 2) 1. Israel Cosmic Ray & Space Weather Center and Emilio.
Flare Luminosity and the Relation to the Solar Wind and the Current Solar Minimum Conditions Roderick Gray Research Advisor: Dr. Kelly Korreck.
Future Plans for Space Weather Observations – U.S. NOAA Perspective Terry Onsager National Oceanic and Atmospheric Administration Space Weather Prediction.
DSCOVR Overview Mike Simpson and Doug Biesecker COPC November 4, 2014.
GOES-R Space Weather L2+ Algorithms GOES-R3 Review William F. Denig, Chief Solar & Terrestrial Physics Division NOAA/NESDIS/NGDC
Earth’s Radiation Belt Xi Shao Department of Astronomy, University Of Maryland, College Park, MD
Solar Activities and Halloween Storms Ahmed Hady Astronomy Department Cairo University, Egypt.
From Geo- to Heliophysical Year: Results of CORONAS-F Space Mission International Conference «50 Years of International Geophysical Year and Electronic.
Solar Energetic Particles -acceleration and observations- (Two approaches at the highest energy) Takashi SAKO Solar-Terrestrial Environment Laboratory,
Ground Systems Data in the World Data Center Archives Justin Mabie (NGDC) and Anatoly Soloviev (GCRAS) 2 July
NGDC’s Solar and Space Weather Program Eric A. Kihn and William Denig.
FORBUSH RECORDS Scott E. Forbush ( ) was an earlier pioneer in the field of study commonly referred to solar-terrestrial physics. A unique holding.
U.S. Department of Commerce National Oceanic & Atmospheric Administration National Geophysical Data Center (NGDC) Stewarding data from the surface of the.
Remote Sensing Space-based Earth exploration and planetary exploration began with the International Geophysical Year (IGY) which was also the beginning.
Solar Irradiance Variability Rodney Viereck NOAA Space Environment Center Derived Total Solar Irradiance Hoyt and Schatten, 1993 (-5 W/m 2 ) Lean et al.,
New Operational Algorithms for Charged Particle Data from Low-Altitude Polar-Orbiting Satellites J. L. Machol 1,2 *, J.C. Green 1, J.V. Rodriguez 3,4,
1 AFWA Visit – 27 February 2014 Solar & Terrestrial Physics William Denig Solar & Terrestrial Physics Division NOAA/NESDIS/NGDC
Satellite Observations for Future Space Weather Forescasting
Space Weather Major sources of space weather ● Solar wind – a stream of plasma consisting of high energy charged particles released from the upper atmosphere.
By: Kiana and Meagan. Purpose  To measure solar magnetic fields  To understand how energy generated by magnetic-field changes in the lower solar atmosphere.
NOAA Satellite Conference April 8-12, 2013 Mary Kicza Assistant Administrator for Satellite & Information Services.
RELEC project (Relativistic ELECtrons). Unified platform “Karat” for small spacecraft 2 MICROSATELLITE KARAT FOR PLANETARY MISSIONS, ASTROPHYSICAL AND.
1 NOAA Agency Report Highlights of Activities SHINE Workshop July 2010 Safeguarding Our Nation’s Advanced Technologies Customer Growth – Rising from Solar.
Moving Beyond IGY: An electronic Geophysical Year (eGY) Concept D.N. Baker Laboratory for Atmospheric and Space Physics University of Colorado - Boulder.
Solar Weather and Tropical Cyclone Activity Abstract Worldwide tropical cyclone energy and frequency data was obtained from the Unisys Weather database.
NOAA Operational Space Env Monitoring Paper J1.2 - AMS W.F. Denig 1 & P Mulligan 2 1 National Geophysical Data Center 2 Office of Systems Development Wednesday,
K9LA Vancouver 2003 Disturbances to Propagation Carl Luetzelschwab K9LA CQ DX?Where’d everybody go?
National Aeronautics and Space Administration NASA Goddard Space Flight Center Software Engineering Division Overview of Significant SWx Events.
SATELLITE METEOROLOGY BASICS satellite orbits EM spectrum
Effect of Geomagetic Activity on Cosmic Ray Muon Rate Mendon High School Regents Physics Honors Period 9 Class A group of Honors physics students plotted.
Space Weather from the SEM-N Sensor Suite for Operational Use W.F. Denig 1, P. Purcell 1,2 & C.D. Reimer 3 1 NOAA National Geophysical Data Center 2 CSU.
High Data Volume Transfer Issues at NOAA Christopher D. Elvidge Earth Observation Group National Oceanic and Atmospheric Administration National Geophysical.
Comparison of Magnesium II Core-to-Wing Ratio Measurements J. Machol 1,2*, M. Snow 3, R. Viereck 4, M. Weber 5, E. Richard 3, L. Puga 4 1 NOAA/National.
1 IGY The ALERT signal of ground level enhancements of solar cosmic rays: physics basis, the ways of realization and development Anashin V., Belov A.,
Data Service at the World Data Center for Geomagnetism, Kyoto T. Iyemori, M. Takeda, M. Nose and Y. Odagi World Data Center for Geomagnetism, Kyoto Graduate.
Contact Information: Dr. Howard J. Singer, Chief Research and Development Division NOAA Space Environment Center 325 Broadway Boulder, CO
Space Environment SSE-120 Please type in your questions and raise your hand so we can answer it during class.
1 Contact Information: Dr. Howard J. Singer, Chief Science and Technology Infusion Branch NOAA Space Environment Center 325 Broadway Boulder, CO
Cosmic Rays Long Term Record Cosmic ray database begins in They have an inverse solar cycle behavior. Earlier data exist. FY07 Cosmic Rays -- new.
Exploitation of Space Ionizing Radiation Monitoring System in Russian Federal Space Agency STRUCTURE OF THE MONITORING SYSTEM The Monitoring System includes.
1 Solar / Geophysics – 23 February 2015 Solar / Geophysics W. Denig, Chief Solar & Terrestrial Physics Division NOAA/NESDIS/NGDC
Cosmic Ray Intensity Variation and Its Connection with the Total and Spectral Solar Irradiance Gigolashvili Marina, Kapanadze Natela Georgian National.
Nishu Karna Mentor:Dr. William Dean Pesnell Code: 671 SESI Program-2009 Goddard Space Flight Center St. Cloud State University Date: August 5, 2009 RELATIVISTIC.
Cosmic Rays2 The Origin of Cosmic Rays and Geomagnetic Effects.
SOLSTICE II -- Magnesium II M. Snow 1*, J. Machol 2,3, R. Viereck 4, M. Weber 5, E. Richard 1 1 Laboratory for Atmospheric and Space Physics, University.
1 Space technology course : Space Radiation Environment and its Effects on Spacecraft Components and Systems Space radiation environment Space Radiation.
Radiation Storms in the Near Space Environment Mikhail Panasyuk, Skobeltsyn Institute of Nuclear Physics of Lomonosov Moscow State University.
1 Thomas J Bogdan Space Weather Program Manager Space Weather Prediction Center Director Safeguarding Our Nation’s Advanced Technologies State of the Space.
Contact Information: Dr. Howard J. Singer, Chief Research and Development Division NOAA Space Environment Center 325 Broadway Boulder, CO
Solar weather consists of the Sun’s effects upon its planetary system and the solar activities it causes. Solar activities, such as flares and CMEs, form.
It is considered that until now in the 24th cycle of solar activity 2 ground level enhancements of solar cosmic rays (GLEs) are registered: on May 17,
What is a geomagnetic storm? A very efficient exchange of energy from the solar wind into the space environment surrounding Earth; These storms result.
Simulations of the effects of extreme solar flares on technological systems at Mars Paul Withers, Boston University Monday
1 SPACE WEATHER SPACE WEATHER. 2 Causes of space weather Space weather is caused mainly by storms and eruptions in our volatile Sun sending potentially.
Agency, version?, Date 2012 Coordination Group for Meteorological Satellites - CGMS Add CGMS agency logo here (in the slide master) Coordination Group.
Space Weather Services to Build Global Resilience Expert Meeting on Space Weather Services February 3, 2015 – UNCOPUOS STSC Assembly Goal: Foster greater.
Bringing 93,000,000 Miles to 40,000 Feet: Space Weather & Aviation An introduction to Space Weather What is it? Where does it come from? What does it do?
National Oceanic and Atmospheric Administration, April 2015 Coordination Group for Meteorological Satellites - CGMS NOAA: Space Weather Overview Presented.
NOAA, version 01, Date: 04/26/2015 Coordination Group for Meteorological Satellites - CGMS Spacecraft Anomaly Database NOAA Presented to CGMS-43 ad-hoc.
KMA Space Weather Service Presented to CGMS-44 on Working Group SWTT.
GOES Data Status Mutual Benefits of NASA THEMIS and NOAA GOES
JMA Report on Satellite-based Space Weather Activities in Japan
2016 Solar Storms with NASA/NOAA GOES-R Satellite Primed to Support Space Weather Predictive Capabilities On 20 December 2016 Earth encountered a stream.
Hiroko Watanabe (Kyoto Univ.)
THEMIS and Space Weather
Presentation transcript:

NOAA Space Environmental Data Paper AMS W.F. Denig National Geophysical Data Center Boulder, CO Monday, 03 Feb 14 / 2:00 PM / Rm C110

2 AMS – Feb 2014 REFERENCE ONLY NOT PRESENTED ABSTRACT AMS – 02/2014 Stewardship of NOAA Space Environmental Data (Paper 2.3) W.F. Denig 1 1 NOAA National Geophysical Data Center, Boulder, CO The National Geophysical Data Center (NGDC) is the steward of NOAA's space environmental data. Currently NGDC has prime responsible for stewarding space weather data from the GOES and POES satellite systems. These data are available directly from NGDC and via various data portals such as the NASA Space Physics Data Facility (SPDF) and the Virtual Radiation Belt Observatory (VIRBO). NGDC also stewards operational space weather products from the USAF's Solar Electro-Optical Network (SEON) along with numerous other solar and space environmental datasets tied to NGDC's heritage as the World Data Center for Solar-Terrestrial Physics. In this talk I will review the range of space environmental datasets available from NGDC and describe how to acquire and use the data. I will also discuss my perceived value for the historical datasets and solicit input on how to prioritize them in light of declining budgets and available manpower. Finally, I will discuss new space weather datasets coming online including data from the next- generation GOES satellites and NOAA's operational DSCOVR mission at L1.

3 AMS – Feb 2014 NGDC provides stewardship, products and services for geophysical data from our Sun to Earth and Earth's sea floor and solid earth environment, including Earth observations from space. The STP Division is responsible for the archive and access of solar and space environmental data and derived products collected by NOAA observing systems and acquired through the former World Data Center for Solar and Terrestrial Physics (Boulder). Data Stewardship NOAA National Geophysical Data Center NOAA Observing Systems: GOES & POES-MetOp (Current)

4 AMS – Feb 2014 NRC Whitepaper Benefits of Operational SWx Monitors Over 30 years of operational space environmental data is available for heliophysics research. For the most part the measurement parameters have remained the same except for some improvements in sensor design and performance – sometimes, much to the angst of the operational agencies: NOAA GOES – particles, fields, solar observation Date range: 1974 – present # of satellites: 15 (not counting 1 failure) Availability: on-line NOAA POES – energetic charged particles Date range: 1978 – present # of satellites: 12 (not counting 1 failure) Availability: on-line USAF DMSP – particles & fields, UV imagery Date range: 1976 – present # of satellites: 17 (not counting 1 failure) Availability: on-line (F6 and beyond only) DOE LANL – particles (GEO and GPS) Data range: 1976 – present # of satellites: Unknown Availability: restricted It keeps going and going and going

5 AMS – Feb 2014 Current NOAA Observing Systems GOES Satellites - Geostationary Solar X-ray Imager Data available since 2003 Full sun solar image (~1 per minute) Space Environment Monitor Geosynchronous Orbit, Since 1974 Parameters:In Situ Magnetic Fields Whole Sun X-ray Flux Energetic Particles

6 AMS – Feb 2014 Current NOAA Observing Systems GOES – Extreme Events (Survey Plots)Extreme Events Numerous X-class flares starting on 28 Oct 2003 Halloween Storm – Oct/Nov 2003 Solar proton event – S4 on NOAA Space Weather Scale Neutron Monitor Forbush Decrease (Moscow) In-situ GEO magnetic field structure See AMS Poster 313 “Extreme Space Weather Events Measured by GOES – ”

7 AMS – Feb 2014 Current NOAA Observing Systems POES/MetopPOES/Metop Satellite System Measurement Description & Data Availability POES/SEM-1 – TIROS-N/NOAA to 2004 POES/SEM-2 – NOAA 15-19/MetOp – 1998 – present TEDions50 eV to 20 keV16 channels / 2 FOV e-50 eV to 20 keV16 channels / 2 FOV MEPEDp+30 keV to 200 MeV10 channels / 2 FOV e-30 keV to 1 MeV3 channels / 2 FOV METOP – Will carry on after POES – Same SEM-2 POES on Orbit Data from POES/MetOp SEM can be used to assess the LEO radiation environment. After MetOp the availability of energetic particle measurements in LEO will be very limited. VIIRS Anomalies

8 AMS – Feb 2014 Improved SWx Monitoring NOAA Historical Solar Observations Observations of sunspots in white light made by Charles Anthony Schott of the Coast Survey, plus data from other providers. The daily sunspot number (SSN) from multiple sources has been a consistent solar index from the early 1800’s to present.Charles Anthony Schott providersSSN From 1967 to 1994 the NOAA Space Environment Center observed the sun in H-alpha (656.3 nm). Chromospheric observations of prominences, filaments, plague and the chromospheric network. Daily observations of the sun for SWx operations transitioned to the USAF starting in 1979.H-alpha USAF NOAA historical space weather data available through NGDCNGDC

9 AMS – Feb 2014 Current NOAA Archived Products Provider: Space Weather Prediction Center Boulder Composite Drawings Trained operator assembles data from multiple sources to describe features on the sun (1972-present).... Plus daily space weather reportsspace weather reports SWx models: US-TECUS-TEC, DRAP, Ovation, ENLIL 1DRAPOvationENLIL 1 Archived ENLIL runs available by request.request

10 AMS – Feb 2014 USAF SWx Observing Systems Defense Meteorological Satellite Program DMSP Space Weather Sensors (AFRL) Sensors: SSJ – Electron/Ion Spectrometer SSIES – Cold Plasma Sensor (Driftmeter) SSM – Magnetometer Satellites: F06-F18 (1982 – Present) Comment: Data provider: AFRL Image courtesy LMMS

11 AMS – Feb 2014 USAF SWx Observing Systems Solar Electro-Optical Network (SEON) Solar Observing Optical Network Daily solar sunspot drawings from 5 SOON sites from 1979 to present. Additional data on H-alpha flare reports.drawingsreports 13 March 1989 Holloman AFB Radio Solar Telescope Network (RSTN) Daily solar radio fixed frequency and spectral measurements from 5 RSTN sites from 2000 to present.fixed frequencyspectral

12 AMS – Feb 2014 Wendelstein Observatory ( ) Boulder Daily Composites (1972-present) Northwestern Observatory ( ) Fraunhoffer Institute ( ) Drawings from the IGY ( ) WDC for Solar-Terrestrial Physics A Legacy from the IGY Under the auspices of the former World Data Center for Solar-Terrestrial Physics (now the World Data Service for Geophysics) NGDC assumed responsibility for numerous datasets related to solar phenomena, the ionosphere, cosmic rays, geomagnetic field, aurora and airglow. Included here is a sample of available solar composite drawings.World Data Service for Geophysics

13 AMS – Feb 2014 WDC for Solar-Terrestrial Physics Interesting Historical Record – Scott Forbush Original dataset “rescued” from destruction were the original records of Scott Forbush, an early cosmic ray physicist.dataset 114 station-years of data from Cheltenham, Christchurch, Godhavn, Climax, Huancayo and Mexico City ( ) Discoveries attributed to Forbush include;  Decrease in cosmic rays during solar storms (Forbush Effect)  Anti-correlation between the 11-yr solar cycle and the cosmic ray flux  Association of increased cosmic radiation (solar energetic particles) correlated with solar flares Ionization Chamber – Huancayo (Peru) – 03 Jan1938

14 AMS – Feb 2014 Main Access Portal – SWx

15 AMS – Feb 2014 Concluding Thoughts NOAA SWx Data Stewardship 1. The NGDC Solar & Terrestrial Physics (STP) division within NGDC is responsible for stewarding NOAA’s SWx datasets and related information Current focus is the archive, access and assessment (AAA) of SWx data from NOAA’s fleet of operational environmental satellites STP also stewards operational SWx data provided from USAF satellites and ground systems. Division continues to manage a variety of historical SWx data collected through the World Data Service for Geophysics, formerly the WDC-STP (Boulder). 2. Challenges While the first priority is NOAA’s satellite data, retaining the personnel (number and skillsets) needed to steward the breadth of technical data available is difficult. There are limited opportunities to digitize historical paper, microfiche and film records 3. Some historical publications (available online) not discussed here: Solar Geophysical Data ( ) Upper Atmosphere Geophysics ( ) Greenwich Photo- heliographic Results ( ) Solar/Geomagnetic Indices Bulletins (1985-Present) International Geophysical Calendar (1957-Present)

16 AMS – Feb 2014 Thank You!