The Extreme Ultraviolet Imager. The Extreme Ultraviolet Imager. Is a suite of three EUV telescopes that will fly onboard the Solar Orbiter mission and will observe the Sun in four bandpasses. The suite is equipped with a single-band and a dual-band High Resolution Imager. That will observe the Sun at high spatial resolution and cadence, along with a dual-band Full Sun Imager. That will continuously monitor the Sun.
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EUI - Extreme Ultraviolet Imager | eui.sidc.be Reviews
https://eui.sidc.be
The Extreme Ultraviolet Imager. The Extreme Ultraviolet Imager. Is a suite of three EUV telescopes that will fly onboard the Solar Orbiter mission and will observe the Sun in four bandpasses. The suite is equipped with a single-band and a dual-band High Resolution Imager. That will observe the Sun at high spatial resolution and cadence, along with a dual-band Full Sun Imager. That will continuously monitor the Sun.
eui.sidc.be
EUI - Extreme Ultraviolet Imager
http://eui.sidc.be/public/allnews.php
11th EUI Consortium Meeting. The 11th EUI consortium meeting will take place at PMOD, starting the 12th March and finishing on 14th March, 2013. Science and technical splinters. 2d day:. [more]. 5th Solar Orbiter Workshop. The 5th Solar Orbiter Workshop will take place in Brugge, Belgium, from Monday September 13 to Thursday September 13, 2012. Friday September 14 will be dedicated to a Science Working Team (SWT) meeting. The worksh. [more]. 10th EUI Consortium Meeting. 9th EUI Consortium Meeting. The Fo...
EUI - Extreme Ultraviolet Imager
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III Solar Orbiter Workshop. Living with a star Sentinels Mission. Solar Probe Plus mission. Homepages of the Institutes/groups belonging to the. Max-Planck-Institut für Sonnensystemforschung. Centre Spatiale de Liège. Mullard Space Science Laboratory. Solar Influence Data analysis Center. Update: 14 May 2014.
EUI File Repository
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Please choose an institute - -. Centre Spatial de Liège. P N Lebedev Physical Institute of the Russian Academy of Sciences. Max Planck Intitute for Solar System Research. Mullard Space Science Laboratory. Physikalisch Meteorologisches Observatorium Davos. Royal Observatory of Belgium. University of Saint Andrews. Send me an e-mail when a new file is uploaded? Your Email or Login:. You will receive soon an email with a link.
EUI - Extreme Ultraviolet Imager
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Prioritized Flags for Science Cases. As explained in the. Sections, the observations are driven by the mission profile in sinergy with the instruments onboard Solar Orbiter. In order to provide a handy toolkit for planning the operations, with the drawback of some unavoidable simplifications, seven main observing modes are foreseen:. Their main features are summarized in the following table. 1) Which physical conditions and processes govern the plasma, fields, and particles in the Sun-Heliosphere system?
EUI - Extreme Ultraviolet Imager
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An Overview On The. Extreme Ultraviolet Imager (. Put the mouse over the image to enlarge it). The Extreme Ultraviolet Imager (. At perihelion, while the maximum aphelion is located at about 0.95. Further more, about 3 years after the launch, the spacecraft will begin an out-of ecliptic phase, with an inclination which increases toward the maximum value of about 30º with respect to the equatorial plane. The suite is composed of 1 Full Solar Imager (. And 2 High Resolution Imagers (. HArr; 15% Sun ∅).
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SIDC - Solar Influences Data Analysis Center - Homepage
http://www.sidc.be/products/quieta
SIDC - Solar Influences Data Center. People and phone numbers. How to get there. AR and CH extraction. Start/End of all quiet alert from the SIDC/RWC Belgium. ASAP, when conditions warrant. Start/End of all quiet alert from the SIDC/RWC Belgium. This message is of the Fast Alert type. It contains a standard text announcing begin and end of periods of very low space weather activity. Check the ISES code book. For information on ISES codes.
SIDC - Solar Influences Data Analysis Center - Homepage
http://sidc.oma.be/products/mobu
SIDC - Solar Influences Data Center. People and phone numbers. How to get there. AR and CH extraction. SIDC Monthly Bulletin of Solar and Geomagnetic Activity. Summary of the Sunspot Bulletin and an overview ofthe solar and geomagnetic activity of last month. SIDC Monthly Bulletin of Solar and Geomagnetic Activity. This report is sent once a month, typically around the 10th. The Sunspot bulletin includes the provisional daily sunspot numbers(total and hemispheric),. Check the ISES code book.
SIDC - Solar Influences Data Center
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People and phone numbers. How to get there. AR and CH extraction. People at SIDC and phone list. Country code for Belgium:. 02 / 790 3 969. 02 / 373 0 276. 02 / 790 3 949. 02 / 373 0 344. 02 / 890 9 829. Frédéric Clette. 02 / 373 0 233. 02 / 790 3 959. 02 / 790 3 938. 02 / 373 0 925. 02 / 790 3 996. 02 / 890 9 845. 02 / 790 3 882. 02 / 373 0 289. 02 / 373 0 305 (or 307 or 910). 02 / 790 3 947. 02 / 373 0 514. 02 / 373 0 237. 02 / 373 0 310. 02 / 790 3 956. 02 / 373 0 208. 02 / 790 3 923. 02 / 373 0 277.
User guide from SIDC - Royal Observatory of Belgium
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SIDC - Solar Influences Data Center. People and phone numbers. How to get there. AR and CH extraction. CODES, TERMINOLOGY AND CLASSIFICATIONS. Mount Wilson Magnetic Classifications. Levels of geomagnetic activity. The 3 component McIntosh classification (McIntosh, Sol. Phys. 125, 251-267,1990) is based on the general form 'Zpc', where 'Z' is the modified Zurich Class, 'p' describes the penumbra of the principal spot, and 'c' describes the distribution of spots in the interior of the group. 247 2400 4 X9.
SIDC - Solar Influences Data Analysis Center - Homepage
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SIDC - Solar Influences Data Center. People and phone numbers. How to get there. AR and CH extraction. GOES X-ray flare detection alert from the SIDC/RWC Belgium. Large flare detection alert automatically produced by SIDC software. ASAP, when a large flare has been reliably detected. GOES X-ray flare detection alert from the SIDC/RWC Belgium. This message is of the Fast Alert type. Check the ISES code book. For information on ISES codes.
SIDC - Solar Influences Data Analysis Center - Homepage
http://www.sidc.be/products/mobu
SIDC - Solar Influences Data Center. People and phone numbers. How to get there. AR and CH extraction. SIDC Monthly Bulletin of Solar and Geomagnetic Activity. Summary of the Sunspot Bulletin and an overview ofthe solar and geomagnetic activity of last month. SIDC Monthly Bulletin of Solar and Geomagnetic Activity. This report is sent once a month, typically around the 10th. The Sunspot bulletin includes the provisional daily sunspot numbers(total and hemispheric),. Check the ISES code book.
SIDC - Solar Influences Data Analysis Center - Homepage
http://www.sidc.be/products/bul
SIDC - Solar Influences Data Center. People and phone numbers. How to get there. AR and CH extraction. Review of past solar and geomagnetic activity. This report is sent once a week, typically on a monday. The weekly bulletin gives an overview of solar and geomagnetic activity of the past week and includes a noticeable solar events list. Check the ISES code book. For information on ISES codes.
SIDC - Solar Influences Data Analysis Center
http://www.sidc.be/jobs
SIDC - Solar Influences Data Center. People and phone numbers. How to get there. AR and CH extraction. We currently have no job vacancies available.
SIDC - Solar Influences Data Analysis Center - Homepage
http://www.sidc.be/EIT
SIDC - Solar Influences Data Center. People and phone numbers. How to get there. AR and CH extraction. The Solar Physics Department of the Royal Observatory of Belgium is a member of the EIT/SoHO consortium. EIT is an instrument on board of the Solar and Heliospheric Observatory, a joint ESA/NASA mission. See also the EIT pages at GSFC. This web pages contain:. The EIT high-cadence synoptic program (' Shutterless' ). Probing the solar corona with the EIT experiment: Belgian science programs and archive.
SIDC - Solar Influences Data Analysis Center - Homepage
http://www.sidc.be/products/meu
SIDC - Solar Influences Data Center. People and phone numbers. How to get there. AR and CH extraction. 3-day-forecast of solar and geomagnetic activity. The SIDC ursigram starts with the code SIDC URSIGRAM YMMDD, where. Y is the last digit of the year number,. MM is the number of the month,. DD is the day of the month. A forecast is given on:. The global flare probability,. PREDICTIONS FOR "today" : 10CM FLUX: xxx / AP: xxx. PREDICTIONS FOR "today 1": 10CM FLUX: xxx / AP: xxx. 10CM SOLAR FLUX : xxx,.
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EUI - Extreme Ultraviolet Imager
The Extreme Ultraviolet Imager. The Extreme Ultraviolet Imager. Is a suite of three EUV telescopes that will fly onboard the Solar Orbiter mission and will observe the Sun in four bandpasses. The suite is equipped with a single-band and a dual-band High Resolution Imager. That will observe the Sun at high spatial resolution and cadence, along with a dual-band Full Sun Imager. That will continuously monitor the Sun.
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