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Solar Max Quick Guide. ODOT Surveyors Conference Salem, OR 19 March 2013 Ken Bays, PLS Lead Geodetic Surveyor Oregon Dept. of Transportation. Solar Weather Overview. Solar activity cycles & their cause 3 types of ionospheric disturbances NOAA Space Weather Scales used to quantify
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Solar Max Quick Guide ODOT Surveyors Conference Salem, OR 19 March 2013 Ken Bays, PLS Lead Geodetic Surveyor Oregon Dept. of Transportation
Solar Weather Overview • Solar activity cycles & their cause • 3 types of ionospheric disturbances • NOAA Space Weather Scales used to quantify • NGS recommendations for GPS surveying during solar activity • Where to obtain solar activity forecasts and reports • How to interpret in relation to NGS recommendations • Improved ORGN real-time correctors from Spider software • Specifically innovated to help GPS surveying during high solar activity
Solar Activity • Solar activity cycles • Approximate 11 year cycles • Observed variations from 9 to 14 years • Hard to predict • Solar max this year: 2013 • Original prediction: • Max would occur in 2010 or 2011 • Strongest cycle since 1958 • Lots of coverage in the media • Latest prediction as of January 2013: • Max will arrive in autumn of 2013 • Smallest cycle since 1906 • Very little media coverage • http://solarscience.msfc.nasa.gov/predict.shtml • Strong solar activity possible any time in any cycle.
Sun Spots • Sun spots (emerging strong magnetic fields) are the prime indicators of solar activity contributing to increased ionospheric disturbance
NGS “User Guidelines for Single Base Real Time GNSS Positioning” http://www.ngs.noaa.gov/PUBS_LIB/NGSRealTimeUserGuidelines.v1.1.pdf
Solar Flares • A solar flare is a sudden brightening observed over the Sun’s surface or solar limb, which is interpreted as a large energy release from twisted magnetic fields near sunspots. • The flare ejects clouds of electrons, ions, and atoms through the corona into space. • These clouds typically reach earth in a day or two. • Can trigger ionospheric disturbances.
NOAA Weather Scales forIonospheric Disturbances • Geomagnetic Storms (G 1- G 5 ratings) • Solar Radiation Storms (S 1- S 5 ratings) • Radio Blackouts (R 1- R 5 ratings)
Geomagnetic Storms • Geomagnetic Storms - disturbances in the geomagnetic field caused by gusts in the solar wind (the outward flux of solar particles and magnetic fields from the sun) that blows by Earth. • May affect satellite orientation, orbital information, broadcast ephemeris, communication. • May cause inability to initialize for the GNSS user and radio problems. • NGS Recommendation: Do not try to perform RT during level G3 – G5 storm events. • NGS “User Guidelines for Single Base Real Time GNSS Positioning”
Solar Radiation Storms • Elevated levels of radiation that occur when the numbers of energetic particles increase. • Strong to extreme storms may impact satellite operations, orientation and communication. • Degraded, intermittent or loss of radio communication in the northern regions are possible. • May impact the noise level at the receiver degrading precision. • NGS Recommendation: Do not try to perform RT during level S4 – S5 storm events. • NGS “User Guidelines for Single Base Real Time GNSS Positioning”
Radio Blackouts • Disturbances of the ionosphere caused by X-ray emissions from the Sun. • Strong to extreme storms may affect satellite signal reception. • May cause intermittent, degraded, or loss of radio communication. • May increase noise at the receiver causing degraded precision. • NGS Recommendations: Do not try to perform RT during level R3 – R5 storm events. • Be aware of possible radio problems even at level R2 storm events. • NGS “User Guidelines for Single Base Real Time GNSS Positioning”
The largest solar event of the period was a M1 event observed at 15/0658Z from Region 1692 (N09W03). There are currently 7 numbered sunspot regions on the disk.
Solar activity is likely to be low with a slight chance for an M-class flare on days one, two, and three (16 Mar, 17 Mar, 18 Mar).
Solar wind speed, as measured by the ACE spacecraft, reached a peak speed of 517 km/s at 15/0500Z. Total IMF reached 14 nT at 15/0719Z. The maximum southward component of Bz reached -10 nT at 15/0619Z.
Protons greater than 10 Mev have a slight chance of crossing threshold on days one and two (16 Mar, 17 Mar).
NOAA Space Weather Alerts Description and Criteriahttp://www.swpc.noaa.gov/alerts/description.html • Good page to start understanding NOAA alerts • Many alert service products correspond with the NOAA Space Weather Scales thresholds. • 4 types of Space Weather Alert Messages • Watch messages are issued for long-lead-time geomagnetic activity predictions • Warning messages are issued when some condition is expected • Alert messages are issued when an event threshold is crossed • Summary messages are issued after the event ends
NOAA Space Weather Alerts Description and Criteriahttp://www.swpc.noaa.gov/alerts/description.html • Space Weather Alerts are issued for these categories: • X-ray Flux Alert and Event Summaries • Radio Burst Alerts and Summary • Geomagnetic Sudden Impulse Warning and Alert • Geomagnetic K-index Watches, Warnings, and Alerts • Electron Flux Alert • Proton 10MeV and 100MeV Flux Warnings, Event Alerts and Summaries
Geomagnetic Stormshttp://www.swpc.noaa.gov/NOAAscales/index.html#GeomagneticStorms
Solar Radiation Stormshttp://www.swpc.noaa.gov/NOAAscales/index.html#SolarRadiationStorms
Radio Blackoutshttp://www.swpc.noaa.gov/NOAAscales/index.html#RadioBlackouts
NOAA Space Weather Data and Products • NOAA Space Weather Advisory Outlooks • http://www.swpc.noaa.gov/advisories/outlooks.html • Issued every Monday • Summary of solar activity for previous week • Forecast of expected activity for coming week • Geomagnetic K-indices • http://www.swpc.noaa.gov/alerts/k-index.html • A report of geomagnetic activity in blocks of time. • Need a “secret decoder” chart to convert to NOAA scale. • NOAA SWPC Product Subscription • https://pss.swpc.noaa.gov/LoginWebForm.aspx?ReturnUrl=%2fproductsubscriptionservice%2f • Space Weather Outlook (weekly) • Report of Solar Geophysical Activity (daily)
NOAA Space Weather Advisory Outlookshttp://www.swpc.noaa.gov/advisories/outlooks.html Monday
NOAA Space Weather Advisory Outlookshttp://www.swpc.noaa.gov/advisories/outlooks.html
NOAA Space Weather Advisory Outlookshttp://www.swpc.noaa.gov/advisories/outlooks.html
Geomagnetic K-indices • This chart is updated every 15 minutes. http://www.swpc.noaa.gov/alerts/k-index.html
Geomagnetic K-indices http://www.swpc.noaa.gov/alerts/k-index.html
Geomagnetic K-indices http://www.swpc.noaa.gov/alerts/k-index.html
Relationship between the NOAA G-scale and Kphttp://www.swpc.noaa.gov/info/Kindex.html • “The Kp scale is a reasonable way to summarize the global level of geomagnetic activity” • “It has not always been easy for those affected by the space environment to understand its significance.” • “The NOAA G-scale was designed to correspond, in a straight forward way, to the significance of effects of geomagnetic storms.”
Relationship between the NOAA G-scale and Kphttp://www.swpc.noaa.gov/info/Kindex.html “Estimates of the planetary average Kp index is used to determine Geomagnetic Storm (NOAA Space Weather Scale) level: Kp of 0 to 4 is below storm level and labeled G0
NOAA SWPC Product Subscriptionhttps://pss.swpc.noaa.gov/LoginWebForm.aspx?ReturnUrl=%2fproductsubscriptionservice%2f
Two NOAA Subscription Products • “Space Weather Outlook” • Weekly • Same as NOAA Space Weather Advisory Outlooks at http://www.swpc.noaa.gov/advisories/outlooks.html • Understandable in terms of NGS GPS guidelines. • “Solar Geophysical Activity Report and Forecast” • Daily with a three day forecast • Not as useful when using NGS GPS guidelines or predicting how it will affect your GPS surveying or when. • Solar flares • Electron flux • Proton Events • But does have general prediction for geomagnetic activity.
Space Weather Outlook Subscription Same as NOAA Space Weather Outlook web page but sent to your E-mail:
Spider 4.3 Improved Network Processing during Solar Max • Automated FTP file downloads by Spider: • Precise Emphemeris files • DCB (Differential Code Bias) files • IONEX (IONsphere Map EXchange) files • These files are used to improve Spider real-time correctors
TEC • The charged particles in the ionosphere affect radio waves proportional to the "total electron content" (TEC) along the wave path. • TEC is the total number of free electrons along the path between the satellite and GNSS receiver. • TEC varies with the changes of solar and geomagnetic conditions during the day, with geographic location and with season.
Spider 4.3 Improved Network Processing:IONEX Files • IONosphereMapEXchange format • Contain info on Total Electron Content (TEC) of the ionosphere • Radio propagation depends on electron density in the ionosphere • IONEX files exchange geographic grid of 2-D & 3-D TEC maps • Generated on a daily basis using data from about 150 GPS sites of the IGS and other institutions. • Spider v 4.3 automatically downloads IONEX files daily from FTP sites and uses this predicted ionosphere TEC to improve processing of network RTK correctors.
Solar Weather Review • Solar activity cycles & their cause • 3 types of ionospheric disturbances • NOAA space weather scales • NGS recommendations for GPS surveying • Where to get solar activity forecasts and reports • How to interpret in relation to NGS recommendations • Improved ORGN real-time correctors from Spider software • How they help GPS surveying during high solar activity
Solar Flare Classifications • X-class flares are big; they are major events that can trigger planet-wide radio blackouts and long-lasting radiation storms. • M-class flares are medium-sized; they can cause brief radio blackouts that affect Earth's polar regions. Minor radiation storms sometimes follow an M-class flare. Compared to X- and M-class events, • C-class flares are small with few noticeable consequences here on Earth.
Precise Orbits: prior to late 2009 http://igscb.jpl.nasa.gov/components/prods.html
Improved precise orbits: after late 2009 http://igscb.jpl.nasa.gov/components/prods.html
DCB FilesDifferential Code Bias files • The time dependent bias between C1 and P1 code pseudoranges, or, the P1 and P2 code pseudoranges. • or • What part of : • http://www.navipedia.net/index.php/Combining_pairs_of_signals_and_clock_definition • don’t you understand?