Preparing for the Maximum of Solar Cycle 24 Joseph Kunches Space - - PowerPoint PPT Presentation

preparing for the maximum of solar cycle 24
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Preparing for the Maximum of Solar Cycle 24 Joseph Kunches Space - - PowerPoint PPT Presentation

Preparing for the Maximum of Solar Cycle 24 Joseph Kunches Space Weather Prediction Center National Centers for Environmental Prediction National Oceanic and Atmospheric Administration Boulder, Colorado USA October 28, 2008 NAV 08/ILA 37,


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October 28, 2008 NAV 08/ILA 37, Church House, Westminster, London 1

Preparing for the Maximum

  • f Solar Cycle 24

Joseph Kunches Space Weather Prediction Center National Centers for Environmental Prediction National Oceanic and Atmospheric Administration Boulder, Colorado USA

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October 28, 2008 NAV 08/ILA 37, Church House, Westminster, London 2

Outline

 The problem – space weather  The question – Cycle 24: How strong?  The issues

 Science  Users

 The outlook

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October 28, 2008 NAV 08/ILA 37, Church House, Westminster, London 3

How Does Space Weather Affect Navigation Systems?

 Geomagnetic Storms  Solar Radiation Storms  Radio Blackouts

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October 28, 2008 NAV 08/ILA 37, Church House, Westminster, London 4

Eruptive Sun to Affected Earth

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October 28, 2008 NAV 08/ILA 37, Church House, Westminster, London 5

Cycle 24 – Just Beginning, Growing

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October 28, 2008 NAV 08/ILA 37, Church House, Westminster, London 6

Do No Spots = Weak Cycle 24?

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October 28, 2008 NAV 08/ILA 37, Church House, Westminster, London 7

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October 28, 2008 NAV 08/ILA 37, Church House, Westminster, London 8

Cycle 24 Predictions 4th Generation

Climatology and Recent Climatology Spectral and Neural Network Precursor Physics Based Pesnell

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October 28, 2008 NAV 08/ILA 37, Church House, Westminster, London 9

April 2007 Prediction

 Solar Minimum will be in March, 2008  Cycle 24 will be small

 Ri = 90  August, 2012

  • r

 Cycle 24 will be large

 Ri = 140  October, 2011

 The panel is split

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October 28, 2008 NAV 08/ILA 37, Church House, Westminster, London 10

Why is the Panel Split?

 The Sun recycles its magnetic fields in 1 solar cycle?  The Sun recycles its magnetic fields in 2-3 solar cycles?

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October 28, 2008 NAV 08/ILA 37, Church House, Westminster, London 11

What Would Break the Deadlock?

 Would small cycle proponents concede?

 What they said approx. one year ago

 If the polar field strength increases → increased Cycle 24  If geomagnetic activity increases → increased Cycle 24

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October 28, 2008 NAV 08/ILA 37, Church House, Westminster, London 12

And in the other direction….

 Would big cycle proponents concede?

 What they said approx. one year ago

 A clear demonstration of how polar fields can produce sunspots at latitudes below 30º just a few years later  The already historically weak meridional flow may weaken by yet another factor of two and produce a small cycle 24  No evidence of new cycle spots by mid-2008

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October 28, 2008 NAV 08/ILA 37, Church House, Westminster, London 13

Space Weather Effects

 Issues include:

 High latitude users (aviation, maritime, geophysical)  Middle latitude radio impacts

 Evolving (during solar minimum) technologies

 GIOVE A & B, GPS L2C  FAA ADS-B

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October 28, 2008 NAV 08/ILA 37, Church House, Westminster, London 14

In 2008, the Department of Homeland Security was named Executive Agent for development of a national backup for critical systems used in position, navigation and

  • timing. Enhanced LORAN (eLORAN) has

been identified as the primary candidate for this backup.

Solar flares, radiation storms, and geomagnetic storms all impact the performance of LORAN

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October 28, 2008 NAV 08/ILA 37, Church House, Westminster, London 15

Navigation at High Latitudes

 Global warming causes polar ice melt  Less ice means more sea lanes  GPS coverage poor at high latitudes  eLoran primary there?  (Space weather hot spot!)

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October 28, 2008 NAV 08/ILA 37, Church House, Westminster, London 16

Off Shore Oil Exploration

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October 28, 2008 NAV 08/ILA 37, Church House, Westminster, London 18

Earth System Models

Radiation Dose Rates: AIR (parametric) HZETRN (physics-based) Near-Earth Space Environment

  • Badhwar/O’Neill GCR Model
  • Empirical Cutoff Rigidity

( IGRF+T05)

  • Physics-based Cutoff Rigidity

(LFM/CMIT+SEP-trajectory)

Value & Benefits to Society

Improvements in the decision- making, decisions, and actions First-ever, data-driven, real-time prediction of biologically harmful radiation exposure levels at commercial airline altitudes Quantitative and qualitative benefits from the improved decisions Comprehensive database of radiation dose rates to formulate recommended annual and career limits to ionizing radiation exposure Comprehensive database of radiation dose rates for airlines to assess cost/risk of polar routes

Real-time prediction of radiation exposure levels to enable optimal balance between airline cost and air traveler health risk during solar storm (SEP) events Improve understanding of biological effects of atmospheric ionizing radiation

  • n aircrew and passengers

through collaboration of epidemiological studies by NIOSH

Predictions/Forecasts Observations, Parameters & Products

Earth Observations

Near-Earth Space Environment NASA/ACE NASA/HEAO-3 NOAA/GOES Assimilated Atmospheric Atmospheric Depth (NCAR/NCEP) Ground-Based Neutron Count Monitors

Nowcast of Atmospheric Ionizing Radiation for Aviation Safety (NAIRAS)

Ionizing Radiation Nowcast 3-D Dose Equivalent 3-D Differential Flux NAIRAS Distributed Network System High-Performance Computer Systems Server Interface Operational and Archival Databases Differential Particle Flux HZE Particles (Z=5-26) Light-Ions (Z=1-4) Neutrons Pions and Muons Electromagnetic Cascasde Particles

Decision Support Systems, Assessments, Management Actions

NAIRAS decision support tool for NOAA/SEC space weather forecasts, warnings, and advisories NAIRAS available at NOAA/ ADD experimental aviation- related weather forecasts,

  • bservations, and analysis

Specific analyses to support the decision making Predict real-time radiation exposure at commercial airline altitudes (includes background GCR and SEP events) Provide accumulated radiation exposures for representative set of domestic, international, and polar routes Specific Decisions / Actions Limit aircrew flight hours to within recommended annual and career limits Alter route and/or altitude during SEP events

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repeat of previous cycle

Photo by Gary Palmer

Radio noise level

  • n GPS frequency

Owens Valley Solar Array

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Solar Radio Burst Of December 6, 2006: Observed by the Global GPS Network

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Galapagos: Sunlit during SRB GUAM: Nighttime during SRB

GUAM GLPS

  • Ultra-precise positioning (10-20 cm)
  • Global coverage: Land, Air, Space
  • Used by satellites in orbit

Global GPS Network Applications

Positioning Fails Positioning fails

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October 28, 2008 NAV 08/ILA 37, Church House, Westminster, London 21

Solar Radio Bursts on GPS

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October 28, 2008 NAV 08/ILA 37, Church House, Westminster, London 22

International Space Environment Service (ISES) Regional Warning Centers

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October 28, 2008 NAV 08/ILA 37, Church House, Westminster, London 23

WMO Initiative

 The Potential Role

  • f WMO in Space

Weather

 A REPORT ON THE POTENTIAL SCOPE, COST AND BENEFIT OF A WMO ACTIVITY IN SUPPORT OF INTERNATIONAL COORDINATION OF SPACE WEATHER SERVICES, PREPARED FOR THE SIXTIETH EXECUTIVE COUNCIL

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October 28, 2008 NAV 08/ILA 37, Church House, Westminster, London 24

Conclusion

 The problem – space weather looms  The question – Cycle 24: How strong? TBD  The issues

 Science -- shaky  Users -- needy

 The outlook

 Activity picking up; get space weather services from ISES