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Form to reserve hotel accommodations for the symposium in Davos, Switzerland from March 11 to 15, 2002.
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How to fill out SoHO-11 / The Sun From Solar Minimum Through Solar Maximum

01
Obtain the SoHO-11 form from the appropriate source.
02
Begin with the general information section, filling in the date, location, and your name.
03
Indicate the solar minimum and maximum dates based on historical sunspot data.
04
Document significant solar events that occurred during this cycle, such as solar flares and coronal mass ejections.
05
Fill out the sections regarding solar observations, noting any anomalies or notable patterns.
06
Ensure that you reference all calculations or data sources used in your form.
07
Review the completed form for consistency and clarity.
08
Submit the form to the specified authority or repository.

Who needs SoHO-11 / The Sun From Solar Minimum Through Solar Maximum?

01
Solar physicists and researchers studying solar activity.
02
Space weather forecasters and analysts.
03
Educational institutions and students involved in solar studies.
04
Governments and agencies monitoring solar impact on technology.
05
Organizations involved in satellite operations and communications.
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Strongest solar flare of 2025 erupts from sun, sparking radio blackouts across Europe, Asia and the Middle East (video) X2. 7-class eruption from sunspot AR4087 disrupts radio signals as the active region rotates toward Earth, raising the risk of more flares ahead.
Solar maximum is the regular period of greatest solar activity during the Sun's 11-year solar cycle. During solar maximum, large numbers of sunspots appear, and the solar irradiance output grows by about 0.07%.
The beginning of a solar cycle is a solar minimum, or when the Sun has the least sunspots. Over time, solar activity — and the number of sunspots — increases. The middle of the solar cycle is the solar maximum, or when the Sun has the most sunspots.
The Solar cycle, also known as the solar magnetic activity cycle, sunspot cycle, or Schwabe cycle, is a periodic 11-year change in the Sun's activity measured in terms of variations in the number of observed sunspots on the Sun's surface.

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SoHO-11 is a comprehensive report that analyzes the solar activity from solar minimum to solar maximum, detailing various phenomena associated with the solar cycle such as sunspots, solar flares, and coronal mass ejections.
Individuals or organizations involved in solar research, including solar physicists and researchers from space agencies, are required to file the SoHO-11 report to contribute to the understanding of solar behavior and its impacts.
To fill out SoHO-11, participants must collect data on solar activity, including observations and measurements, and organize this data according to the specified format outlined in the filing guidelines, ensuring accurate and comprehensive reporting.
The purpose of SoHO-11 is to provide a clear and detailed overview of solar activity over the solar cycle, which helps in predicting and understanding the impacts of solar phenomena on space weather and Earth.
The report must include data on solar irradiance, sunspot counts, solar flare occurrences, and other relevant solar activity metrics, as well as any observed effects on space weather and terrestrial conditions.
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