Events

The seventh European Space Weather Week will take place in Brugge, Belgium, from Monday 15th November to Friday 19th November 2009. This meeting is being jointly organised by the Solar-Terrestrial Centre of Excellence (STCE), ESA, the SWWT and the COST ES0803 communities. The local organisation is done by the STCE. This event will build on the advances made during previous European Space Weather Weeks and preceding ESA Space Weather Applications Workshops.

The seventh European Space Weather Week will take place in Brugge, Belgium, from Monday 15th November to Friday 19th November 2009. This meeting is being jointly organised by the Solar-Terrestrial Centre of Excellence (STCE), ESA, the SWWT and the COST ES0803 communities. The local organisation is done by the STCE. This event will build on the advances made during previous European Space Weather Weeks and preceding ESA Space Weather Applications Workshops.

The seventh European Space Weather Week will take place in Brugge, Belgium, from Monday 15th November to Friday 19th November 2009. This meeting is being jointly organised by the Solar-Terrestrial Centre of Excellence (STCE), ESA, the SWWT and the COST ES0803 communities. The local organisation is done by the STCE. This event will build on the advances made during previous European Space Weather Weeks and preceding ESA Space Weather Applications Workshops.

The seventh European Space Weather Week will take place in Brugge, Belgium, from Monday 15th November to Friday 19th November 2009. This meeting is being jointly organised by the Solar-Terrestrial Centre of Excellence (STCE), ESA, the SWWT and the COST ES0803 communities. The local organisation is done by the STCE. This event will build on the advances made during previous European Space Weather Weeks and preceding ESA Space Weather Applications Workshops.

The seventh European Space Weather Week will take place in Brugge, Belgium, from Monday 15th November to Friday 19th November 2009. This meeting is being jointly organised by the Solar-Terrestrial Centre of Excellence (STCE), ESA, the SWWT and the COST ES0803 communities. The local organisation is done by the STCE. This event will build on the advances made during previous European Space Weather Weeks and preceding ESA Space Weather Applications Workshops.

Remote polarization sensing has widely been applied in Astrophysics. Generally, the application focuses on extracting information on the magnetic fields which play a pervasive role in all astrophysical plasmas and govern most of the variability in the universe at intermediate time scales, in particular all activity phenomena on the Sun and stars.

Remote polarization sensing has widely been applied in Astrophysics. Generally, the application focuses on extracting information on the magnetic fields which play a pervasive role in all astrophysical plasmas and govern most of the variability in the universe at intermediate time scales, in particular all activity phenomena on the Sun and stars.

Remote polarization sensing has widely been applied in Astrophysics. Generally, the application focuses on extracting information on the magnetic fields which play a pervasive role in all astrophysical plasmas and govern most of the variability in the universe at intermediate time scales, in particular all activity phenomena on the Sun and stars.

The large success (and accompanying growth, both in attendance and in breadth of topics) of the SHINE workshop is due primarily to its uniqueness in style. Unlike many annual conferences (e.g., AGU, SPD, ICRC) SHINE sessions are not a series of talks interspersed with short discussion. The goal of a SHINE session is to generate involved and constructive discussion on a topic of keen interest to the participants.

Remote polarization sensing has widely been applied in Astrophysics. Generally, the application focuses on extracting information on the magnetic fields which play a pervasive role in all astrophysical plasmas and govern most of the variability in the universe at intermediate time scales, in particular all activity phenomena on the Sun and stars.

The large success (and accompanying growth, both in attendance and in breadth of topics) of the SHINE workshop is due primarily to its uniqueness in style. Unlike many annual conferences (e.g., AGU, SPD, ICRC) SHINE sessions are not a series of talks interspersed with short discussion. The goal of a SHINE session is to generate involved and constructive discussion on a topic of keen interest to the participants.

Remote polarization sensing has widely been applied in Astrophysics. Generally, the application focuses on extracting information on the magnetic fields which play a pervasive role in all astrophysical plasmas and govern most of the variability in the universe at intermediate time scales, in particular all activity phenomena on the Sun and stars.

The large success (and accompanying growth, both in attendance and in breadth of topics) of the SHINE workshop is due primarily to its uniqueness in style. Unlike many annual conferences (e.g., AGU, SPD, ICRC) SHINE sessions are not a series of talks interspersed with short discussion. The goal of a SHINE session is to generate involved and constructive discussion on a topic of keen interest to the participants.

Remote polarization sensing has widely been applied in Astrophysics. Generally, the application focuses on extracting information on the magnetic fields which play a pervasive role in all astrophysical plasmas and govern most of the variability in the universe at intermediate time scales, in particular all activity phenomena on the Sun and stars.

The large success (and accompanying growth, both in attendance and in breadth of topics) of the SHINE workshop is due primarily to its uniqueness in style. Unlike many annual conferences (e.g., AGU, SPD, ICRC) SHINE sessions are not a series of talks interspersed with short discussion. The goal of a SHINE session is to generate involved and constructive discussion on a topic of keen interest to the participants.

Remote polarization sensing has widely been applied in Astrophysics. Generally, the application focuses on extracting information on the magnetic fields which play a pervasive role in all astrophysical plasmas and govern most of the variability in the universe at intermediate time scales, in particular all activity phenomena on the Sun and stars.

The large success (and accompanying growth, both in attendance and in breadth of topics) of the SHINE workshop is due primarily to its uniqueness in style. Unlike many annual conferences (e.g., AGU, SPD, ICRC) SHINE sessions are not a series of talks interspersed with short discussion. The goal of a SHINE session is to generate involved and constructive discussion on a topic of keen interest to the participants.

Remote polarization sensing has widely been applied in Astrophysics. Generally, the application focuses on extracting information on the magnetic fields which play a pervasive role in all astrophysical plasmas and govern most of the variability in the universe at intermediate time scales, in particular all activity phenomena on the Sun and stars.

The large success (and accompanying growth, both in attendance and in breadth of topics) of the SHINE workshop is due primarily to its uniqueness in style. Unlike many annual conferences (e.g., AGU, SPD, ICRC) SHINE sessions are not a series of talks interspersed with short discussion. The goal of a SHINE session is to generate involved and constructive discussion on a topic of keen interest to the participants.

MHD, which treats plasmas as a continuum medium, is a branch of plasma physics. It has been widely applied in solar physics, space physics and astrophysics. The summer school is designed especially for graduate students and young scientists, and the overall objective is to deepen the understanding of MHD theory and its applications in solar and space physics.

Remote polarization sensing has widely been applied in Astrophysics. Generally, the application focuses on extracting information on the magnetic fields which play a pervasive role in all astrophysical plasmas and govern most of the variability in the universe at intermediate time scales, in particular all activity phenomena on the Sun and stars.

MHD, which treats plasmas as a continuum medium, is a branch of plasma physics. It has been widely applied in solar physics, space physics and astrophysics. The summer school is designed especially for graduate students and young scientists, and the overall objective is to deepen the understanding of MHD theory and its applications in solar and space physics.

Remote polarization sensing has widely been applied in Astrophysics. Generally, the application focuses on extracting information on the magnetic fields which play a pervasive role in all astrophysical plasmas and govern most of the variability in the universe at intermediate time scales, in particular all activity phenomena on the Sun and stars.

MHD, which treats plasmas as a continuum medium, is a branch of plasma physics. It has been widely applied in solar physics, space physics and astrophysics. The summer school is designed especially for graduate students and young scientists, and the overall objective is to deepen the understanding of MHD theory and its applications in solar and space physics.

Remote polarization sensing has widely been applied in Astrophysics. Generally, the application focuses on extracting information on the magnetic fields which play a pervasive role in all astrophysical plasmas and govern most of the variability in the universe at intermediate time scales, in particular all activity phenomena on the Sun and stars.

MHD, which treats plasmas as a continuum medium, is a branch of plasma physics. It has been widely applied in solar physics, space physics and astrophysics. The summer school is designed especially for graduate students and young scientists, and the overall objective is to deepen the understanding of MHD theory and its applications in solar and space physics.

The CISM Summer School is intended to give students a comprehensive immersion in the subject of space weather: what it is, what it does, and what can be done about it. Space weather is many things: beautiful when seen through the eyes of a sun-viewing telescope, fascinating when studied for its alien worlds of magnetic structures and phenomena, awesome when witnessed as a solar eruption or auroral storm, and devastating to the users of services it disrupts. Space weather links the Sun, the Earth, and the space in between in a branching chain of consequences.

MHD, which treats plasmas as a continuum medium, is a branch of plasma physics. It has been widely applied in solar physics, space physics and astrophysics. The summer school is designed especially for graduate students and young scientists, and the overall objective is to deepen the understanding of MHD theory and its applications in solar and space physics.

The CISM Summer School is intended to give students a comprehensive immersion in the subject of space weather: what it is, what it does, and what can be done about it. Space weather is many things: beautiful when seen through the eyes of a sun-viewing telescope, fascinating when studied for its alien worlds of magnetic structures and phenomena, awesome when witnessed as a solar eruption or auroral storm, and devastating to the users of services it disrupts. Space weather links the Sun, the Earth, and the space in between in a branching chain of consequences.

MHD, which treats plasmas as a continuum medium, is a branch of plasma physics. It has been widely applied in solar physics, space physics and astrophysics. The summer school is designed especially for graduate students and young scientists, and the overall objective is to deepen the understanding of MHD theory and its applications in solar and space physics.

The CISM Summer School is intended to give students a comprehensive immersion in the subject of space weather: what it is, what it does, and what can be done about it. Space weather is many things: beautiful when seen through the eyes of a sun-viewing telescope, fascinating when studied for its alien worlds of magnetic structures and phenomena, awesome when witnessed as a solar eruption or auroral storm, and devastating to the users of services it disrupts. Space weather links the Sun, the Earth, and the space in between in a branching chain of consequences.

MHD, which treats plasmas as a continuum medium, is a branch of plasma physics. It has been widely applied in solar physics, space physics and astrophysics. The summer school is designed especially for graduate students and young scientists, and the overall objective is to deepen the understanding of MHD theory and its applications in solar and space physics.

The CISM Summer School is intended to give students a comprehensive immersion in the subject of space weather: what it is, what it does, and what can be done about it. Space weather is many things: beautiful when seen through the eyes of a sun-viewing telescope, fascinating when studied for its alien worlds of magnetic structures and phenomena, awesome when witnessed as a solar eruption or auroral storm, and devastating to the users of services it disrupts. Space weather links the Sun, the Earth, and the space in between in a branching chain of consequences.

The CISM Summer School is intended to give students a comprehensive immersion in the subject of space weather: what it is, what it does, and what can be done about it. Space weather is many things: beautiful when seen through the eyes of a sun-viewing telescope, fascinating when studied for its alien worlds of magnetic structures and phenomena, awesome when witnessed as a solar eruption or auroral storm, and devastating to the users of services it disrupts. Space weather links the Sun, the Earth, and the space in between in a branching chain of consequences.

The CISM Summer School is intended to give students a comprehensive immersion in the subject of space weather: what it is, what it does, and what can be done about it. Space weather is many things: beautiful when seen through the eyes of a sun-viewing telescope, fascinating when studied for its alien worlds of magnetic structures and phenomena, awesome when witnessed as a solar eruption or auroral storm, and devastating to the users of services it disrupts. Space weather links the Sun, the Earth, and the space in between in a branching chain of consequences.

The CISM Summer School is intended to give students a comprehensive immersion in the subject of space weather: what it is, what it does, and what can be done about it. Space weather is many things: beautiful when seen through the eyes of a sun-viewing telescope, fascinating when studied for its alien worlds of magnetic structures and phenomena, awesome when witnessed as a solar eruption or auroral storm, and devastating to the users of services it disrupts. Space weather links the Sun, the Earth, and the space in between in a branching chain of consequences.

The CISM Summer School is intended to give students a comprehensive immersion in the subject of space weather: what it is, what it does, and what can be done about it. Space weather is many things: beautiful when seen through the eyes of a sun-viewing telescope, fascinating when studied for its alien worlds of magnetic structures and phenomena, awesome when witnessed as a solar eruption or auroral storm, and devastating to the users of services it disrupts. Space weather links the Sun, the Earth, and the space in between in a branching chain of consequences.

In 2011 the two STEREO spacecraft will be separated by more than 90 degrees from the Earth. With the help of observations from SDO and SOHO, we will have a 360-degree view of the Sun for the first time. The objective of the workshop is to discuss a range of scientific topics, which are key to our current understanding of the global structure of the Sun and inner heliosphere.

The CISM Summer School is intended to give students a comprehensive immersion in the subject of space weather: what it is, what it does, and what can be done about it. Space weather is many things: beautiful when seen through the eyes of a sun-viewing telescope, fascinating when studied for its alien worlds of magnetic structures and phenomena, awesome when witnessed as a solar eruption or auroral storm, and devastating to the users of services it disrupts. Space weather links the Sun, the Earth, and the space in between in a branching chain of consequences.

In 2011 the two STEREO spacecraft will be separated by more than 90 degrees from the Earth. With the help of observations from SDO and SOHO, we will have a 360-degree view of the Sun for the first time. The objective of the workshop is to discuss a range of scientific topics, which are key to our current understanding of the global structure of the Sun and inner heliosphere.

The CISM Summer School is intended to give students a comprehensive immersion in the subject of space weather: what it is, what it does, and what can be done about it. Space weather is many things: beautiful when seen through the eyes of a sun-viewing telescope, fascinating when studied for its alien worlds of magnetic structures and phenomena, awesome when witnessed as a solar eruption or auroral storm, and devastating to the users of services it disrupts. Space weather links the Sun, the Earth, and the space in between in a branching chain of consequences.

In 2011 the two STEREO spacecraft will be separated by more than 90 degrees from the Earth. With the help of observations from SDO and SOHO, we will have a 360-degree view of the Sun for the first time. The objective of the workshop is to discuss a range of scientific topics, which are key to our current understanding of the global structure of the Sun and inner heliosphere.

Applications were invited for the 2011 Heliophysics Summer School, to be held in Boulder, Colorado. NASA Living with a Star sponsors the Heliophysics Summer Schools. The UCAR Visiting Scientist Programs office administers these schools for NASA. This series of summer schools helps graduate students and scientists learn and develop the science of heliophysics as a broad, coherent discipline that reaches in space from the Earth's troposphere to the depths of the Sun, and in time from the formation of the solar system to the distant future.

The CISM Summer School is intended to give students a comprehensive immersion in the subject of space weather: what it is, what it does, and what can be done about it. Space weather is many things: beautiful when seen through the eyes of a sun-viewing telescope, fascinating when studied for its alien worlds of magnetic structures and phenomena, awesome when witnessed as a solar eruption or auroral storm, and devastating to the users of services it disrupts. Space weather links the Sun, the Earth, and the space in between in a branching chain of consequences.

In 2011 the two STEREO spacecraft will be separated by more than 90 degrees from the Earth. With the help of observations from SDO and SOHO, we will have a 360-degree view of the Sun for the first time. The objective of the workshop is to discuss a range of scientific topics, which are key to our current understanding of the global structure of the Sun and inner heliosphere.

Applications were invited for the 2011 Heliophysics Summer School, to be held in Boulder, Colorado. NASA Living with a Star sponsors the Heliophysics Summer Schools. The UCAR Visiting Scientist Programs office administers these schools for NASA. This series of summer schools helps graduate students and scientists learn and develop the science of heliophysics as a broad, coherent discipline that reaches in space from the Earth's troposphere to the depths of the Sun, and in time from the formation of the solar system to the distant future.

The CISM Summer School is intended to give students a comprehensive immersion in the subject of space weather: what it is, what it does, and what can be done about it. Space weather is many things: beautiful when seen through the eyes of a sun-viewing telescope, fascinating when studied for its alien worlds of magnetic structures and phenomena, awesome when witnessed as a solar eruption or auroral storm, and devastating to the users of services it disrupts. Space weather links the Sun, the Earth, and the space in between in a branching chain of consequences.

In 2011 the two STEREO spacecraft will be separated by more than 90 degrees from the Earth. With the help of observations from SDO and SOHO, we will have a 360-degree view of the Sun for the first time. The objective of the workshop is to discuss a range of scientific topics, which are key to our current understanding of the global structure of the Sun and inner heliosphere.

Applications were invited for the 2011 Heliophysics Summer School, to be held in Boulder, Colorado. NASA Living with a Star sponsors the Heliophysics Summer Schools. The UCAR Visiting Scientist Programs office administers these schools for NASA. This series of summer schools helps graduate students and scientists learn and develop the science of heliophysics as a broad, coherent discipline that reaches in space from the Earth's troposphere to the depths of the Sun, and in time from the formation of the solar system to the distant future.

Applications were invited for the 2011 Heliophysics Summer School, to be held in Boulder, Colorado. NASA Living with a Star sponsors the Heliophysics Summer Schools. The UCAR Visiting Scientist Programs office administers these schools for NASA. This series of summer schools helps graduate students and scientists learn and develop the science of heliophysics as a broad, coherent discipline that reaches in space from the Earth's troposphere to the depths of the Sun, and in time from the formation of the solar system to the distant future.

Applications were invited for the 2011 Heliophysics Summer School, to be held in Boulder, Colorado. NASA Living with a Star sponsors the Heliophysics Summer Schools. The UCAR Visiting Scientist Programs office administers these schools for NASA. This series of summer schools helps graduate students and scientists learn and develop the science of heliophysics as a broad, coherent discipline that reaches in space from the Earth's troposphere to the depths of the Sun, and in time from the formation of the solar system to the distant future.

Applications were invited for the 2011 Heliophysics Summer School, to be held in Boulder, Colorado. NASA Living with a Star sponsors the Heliophysics Summer Schools. The UCAR Visiting Scientist Programs office administers these schools for NASA. This series of summer schools helps graduate students and scientists learn and develop the science of heliophysics as a broad, coherent discipline that reaches in space from the Earth's troposphere to the depths of the Sun, and in time from the formation of the solar system to the distant future.

Applications were invited for the 2011 Heliophysics Summer School, to be held in Boulder, Colorado. NASA Living with a Star sponsors the Heliophysics Summer Schools. The UCAR Visiting Scientist Programs office administers these schools for NASA. This series of summer schools helps graduate students and scientists learn and develop the science of heliophysics as a broad, coherent discipline that reaches in space from the Earth's troposphere to the depths of the Sun, and in time from the formation of the solar system to the distant future.

Applications were invited for the 2011 Heliophysics Summer School, to be held in Boulder, Colorado. NASA Living with a Star sponsors the Heliophysics Summer Schools. The UCAR Visiting Scientist Programs office administers these schools for NASA. This series of summer schools helps graduate students and scientists learn and develop the science of heliophysics as a broad, coherent discipline that reaches in space from the Earth's troposphere to the depths of the Sun, and in time from the formation of the solar system to the distant future.

Website: http://www.asiaoceania.org/aogs2011/public.asp?page=mars/confSessionList.asp

Website: http://www.asiaoceania.org/aogs2011/public.asp?page=mars/confSessionList.asp

Website: http://www.asiaoceania.org/aogs2011/public.asp?page=mars/confSessionList.asp

Website: http://www.asiaoceania.org/aogs2011/public.asp?page=mars/confSessionList.asp

Website: http://www.asiaoceania.org/aogs2011/public.asp?page=mars/confSessionList.asp

The XXX General Assembly and Scientific Symposium of the International Union of Radio Science (Union Radio Scientifique Internationale-URSI) will be held at Lütfi Kırdar Convention and Exhibition Centre in the beautiful historical center of Istanbul, Turkey on August 13-20, 2011. The XXX General Assembly and Scientific Symposium will have a scientific program consisting of plenary lectures, public lectures, tutorials, posters, invited and contributed papers organized around the ten Commissions of URSI.

The XXX General Assembly and Scientific Symposium of the International Union of Radio Science (Union Radio Scientifique Internationale-URSI) will be held at Lütfi Kırdar Convention and Exhibition Centre in the beautiful historical center of Istanbul, Turkey on August 13-20, 2011. The XXX General Assembly and Scientific Symposium will have a scientific program consisting of plenary lectures, public lectures, tutorials, posters, invited and contributed papers organized around the ten Commissions of URSI.

The XXX General Assembly and Scientific Symposium of the International Union of Radio Science (Union Radio Scientifique Internationale-URSI) will be held at Lütfi Kırdar Convention and Exhibition Centre in the beautiful historical center of Istanbul, Turkey on August 13-20, 2011. The XXX General Assembly and Scientific Symposium will have a scientific program consisting of plenary lectures, public lectures, tutorials, posters, invited and contributed papers organized around the ten Commissions of URSI.

The XXX General Assembly and Scientific Symposium of the International Union of Radio Science (Union Radio Scientifique Internationale-URSI) will be held at Lütfi Kırdar Convention and Exhibition Centre in the beautiful historical center of Istanbul, Turkey on August 13-20, 2011. The XXX General Assembly and Scientific Symposium will have a scientific program consisting of plenary lectures, public lectures, tutorials, posters, invited and contributed papers organized around the ten Commissions of URSI.

The XXX General Assembly and Scientific Symposium of the International Union of Radio Science (Union Radio Scientifique Internationale-URSI) will be held at Lütfi Kırdar Convention and Exhibition Centre in the beautiful historical center of Istanbul, Turkey on August 13-20, 2011. The XXX General Assembly and Scientific Symposium will have a scientific program consisting of plenary lectures, public lectures, tutorials, posters, invited and contributed papers organized around the ten Commissions of URSI.

The XXX General Assembly and Scientific Symposium of the International Union of Radio Science (Union Radio Scientifique Internationale-URSI) will be held at Lütfi Kırdar Convention and Exhibition Centre in the beautiful historical center of Istanbul, Turkey on August 13-20, 2011. The XXX General Assembly and Scientific Symposium will have a scientific program consisting of plenary lectures, public lectures, tutorials, posters, invited and contributed papers organized around the ten Commissions of URSI.

The XXX General Assembly and Scientific Symposium of the International Union of Radio Science (Union Radio Scientifique Internationale-URSI) will be held at Lütfi Kırdar Convention and Exhibition Centre in the beautiful historical center of Istanbul, Turkey on August 13-20, 2011. The XXX General Assembly and Scientific Symposium will have a scientific program consisting of plenary lectures, public lectures, tutorials, posters, invited and contributed papers organized around the ten Commissions of URSI.

The XXX General Assembly and Scientific Symposium of the International Union of Radio Science (Union Radio Scientifique Internationale-URSI) will be held at Lütfi Kırdar Convention and Exhibition Centre in the beautiful historical center of Istanbul, Turkey on August 13-20, 2011. The XXX General Assembly and Scientific Symposium will have a scientific program consisting of plenary lectures, public lectures, tutorials, posters, invited and contributed papers organized around the ten Commissions of URSI.

The ISWI is a follow-up activity to the successful IHY 2007 (that conducted many programs not only to popularise space science all over the world but also to create favorable conditions for joint research and training in some sort of global framework), but focusing exclusively on space weather. European scientists are successfully participating in the ISWI and many research level scientific instruments have been installed in many parts of Europe in the framework of the IHY and ISWI.

The ISWI is a follow-up activity to the successful IHY 2007 (that conducted many programs not only to popularise space science all over the world but also to create favorable conditions for joint research and training in some sort of global framework), but focusing exclusively on space weather. European scientists are successfully participating in the ISWI and many research level scientific instruments have been installed in many parts of Europe in the framework of the IHY and ISWI.

The ISWI is a follow-up activity to the successful IHY 2007 (that conducted many programs not only to popularise space science all over the world but also to create favorable conditions for joint research and training in some sort of global framework), but focusing exclusively on space weather. European scientists are successfully participating in the ISWI and many research level scientific instruments have been installed in many parts of Europe in the framework of the IHY and ISWI.

The ISWI is a follow-up activity to the successful IHY 2007 (that conducted many programs not only to popularise space science all over the world but also to create favorable conditions for joint research and training in some sort of global framework), but focusing exclusively on space weather. European scientists are successfully participating in the ISWI and many research level scientific instruments have been installed in many parts of Europe in the framework of the IHY and ISWI.

The ISWI is a follow-up activity to the successful IHY 2007 (that conducted many programs not only to popularise space science all over the world but also to create favorable conditions for joint research and training in some sort of global framework), but focusing exclusively on space weather. European scientists are successfully participating in the ISWI and many research level scientific instruments have been installed in many parts of Europe in the framework of the IHY and ISWI.

The ISWI is a follow-up activity to the successful IHY 2007 (that conducted many programs not only to popularise space science all over the world but also to create favorable conditions for joint research and training in some sort of global framework), but focusing exclusively on space weather. European scientists are successfully participating in the ISWI and many research level scientific instruments have been installed in many parts of Europe in the framework of the IHY and ISWI.

The ISWI is a follow-up activity to the successful IHY 2007 (that conducted many programs not only to popularise space science all over the world but also to create favorable conditions for joint research and training in some sort of global framework), but focusing exclusively on space weather. European scientists are successfully participating in the ISWI and many research level scientific instruments have been installed in many parts of Europe in the framework of the IHY and ISWI.

As the impact of space weather and climate on daily life is becoming more important, it is timely to discuss the latest reseach on the solar origin of these phenomena. Recent advances in helioseismology have demonstrated that subsurface dynamics are closely associated with aspects of solar activity from the long-term timing of the solar cycle to the short-term eruption of solar flares. The advent of synoptic vector magnetic field measurements is opening up a new path for research on active regions, flares and CME's.

The meeting will cover a broad range of aspects of solar physics, space science and solar-terrestrial relations. We aim to include every side of solar and space research, including observations, theory, and numerical modelling. The main idea behind the meeting is to treat the entire solar-terrestrial domain as one system, rather than treating each region independently, so speakers with interdisciplinary expertise are particularly welcome.

The academic reason for us to gather here is to participating the International Living With a Star Program (ILWS) Science Workshop. The ILWS program is an international organization in the field of solar-terrestrial physics, heliophysics and space weather. As the name of the organization indicated, if the human beings want to continuously survive on the Earth, we must live with the Sun, a star. This is particularly true in the modern society where we are already so much dependent on the technical infrastructures in the space and on the ground.

As the impact of space weather and climate on daily life is becoming more important, it is timely to discuss the latest reseach on the solar origin of these phenomena. Recent advances in helioseismology have demonstrated that subsurface dynamics are closely associated with aspects of solar activity from the long-term timing of the solar cycle to the short-term eruption of solar flares. The advent of synoptic vector magnetic field measurements is opening up a new path for research on active regions, flares and CME's.

The meeting will cover a broad range of aspects of solar physics, space science and solar-terrestrial relations. We aim to include every side of solar and space research, including observations, theory, and numerical modelling. The main idea behind the meeting is to treat the entire solar-terrestrial domain as one system, rather than treating each region independently, so speakers with interdisciplinary expertise are particularly welcome.

The academic reason for us to gather here is to participating the International Living With a Star Program (ILWS) Science Workshop. The ILWS program is an international organization in the field of solar-terrestrial physics, heliophysics and space weather. As the name of the organization indicated, if the human beings want to continuously survive on the Earth, we must live with the Sun, a star. This is particularly true in the modern society where we are already so much dependent on the technical infrastructures in the space and on the ground.

As the impact of space weather and climate on daily life is becoming more important, it is timely to discuss the latest reseach on the solar origin of these phenomena. Recent advances in helioseismology have demonstrated that subsurface dynamics are closely associated with aspects of solar activity from the long-term timing of the solar cycle to the short-term eruption of solar flares. The advent of synoptic vector magnetic field measurements is opening up a new path for research on active regions, flares and CME's.

The meeting will cover a broad range of aspects of solar physics, space science and solar-terrestrial relations. We aim to include every side of solar and space research, including observations, theory, and numerical modelling. The main idea behind the meeting is to treat the entire solar-terrestrial domain as one system, rather than treating each region independently, so speakers with interdisciplinary expertise are particularly welcome.

The academic reason for us to gather here is to participating the International Living With a Star Program (ILWS) Science Workshop. The ILWS program is an international organization in the field of solar-terrestrial physics, heliophysics and space weather. As the name of the organization indicated, if the human beings want to continuously survive on the Earth, we must live with the Sun, a star. This is particularly true in the modern society where we are already so much dependent on the technical infrastructures in the space and on the ground.

As the impact of space weather and climate on daily life is becoming more important, it is timely to discuss the latest reseach on the solar origin of these phenomena. Recent advances in helioseismology have demonstrated that subsurface dynamics are closely associated with aspects of solar activity from the long-term timing of the solar cycle to the short-term eruption of solar flares. The advent of synoptic vector magnetic field measurements is opening up a new path for research on active regions, flares and CME's.

The meeting will cover a broad range of aspects of solar physics, space science and solar-terrestrial relations. We aim to include every side of solar and space research, including observations, theory, and numerical modelling. The main idea behind the meeting is to treat the entire solar-terrestrial domain as one system, rather than treating each region independently, so speakers with interdisciplinary expertise are particularly welcome.

The academic reason for us to gather here is to participating the International Living With a Star Program (ILWS) Science Workshop. The ILWS program is an international organization in the field of solar-terrestrial physics, heliophysics and space weather. As the name of the organization indicated, if the human beings want to continuously survive on the Earth, we must live with the Sun, a star. This is particularly true in the modern society where we are already so much dependent on the technical infrastructures in the space and on the ground.

As the impact of space weather and climate on daily life is becoming more important, it is timely to discuss the latest reseach on the solar origin of these phenomena. Recent advances in helioseismology have demonstrated that subsurface dynamics are closely associated with aspects of solar activity from the long-term timing of the solar cycle to the short-term eruption of solar flares. The advent of synoptic vector magnetic field measurements is opening up a new path for research on active regions, flares and CME's.

The meeting will cover a broad range of aspects of solar physics, space science and solar-terrestrial relations. We aim to include every side of solar and space research, including observations, theory, and numerical modelling. The main idea behind the meeting is to treat the entire solar-terrestrial domain as one system, rather than treating each region independently, so speakers with interdisciplinary expertise are particularly welcome.

The academic reason for us to gather here is to participating the International Living With a Star Program (ILWS) Science Workshop. The ILWS program is an international organization in the field of solar-terrestrial physics, heliophysics and space weather. As the name of the organization indicated, if the human beings want to continuously survive on the Earth, we must live with the Sun, a star. This is particularly true in the modern society where we are already so much dependent on the technical infrastructures in the space and on the ground.

This is the 13th general meeting in Solar Physics in Europe, a tri-annual event that covers and welcomes contributions from all aspects of contemporary solar physics. The conference's Science Program is a non-exhaustive list of topics designed to expose the breadth and diversity of current research undertaken by the international solar physics community, but more general contributions not necessarily falling into these research categories will also be accommodated.

The main purpose of the International Symposium on Recent Observations and Simulations of the Sun-Earth System II (ISROSES-II) is to bring together cross-disciplinary scientists from around the globe to have focused discussions on fundamental problems related to the space environment of the Earth. It is a continuation of the highly successful ISROSES symposium held in Varna, Bulgaria, during 17-22 September 2006 (http://www.isroses.org).

This is the 13th general meeting in Solar Physics in Europe, a tri-annual event that covers and welcomes contributions from all aspects of contemporary solar physics. The conference's Science Program is a non-exhaustive list of topics designed to expose the breadth and diversity of current research undertaken by the international solar physics community, but more general contributions not necessarily falling into these research categories will also be accommodated.

The main purpose of the International Symposium on Recent Observations and Simulations of the Sun-Earth System II (ISROSES-II) is to bring together cross-disciplinary scientists from around the globe to have focused discussions on fundamental problems related to the space environment of the Earth. It is a continuation of the highly successful ISROSES symposium held in Varna, Bulgaria, during 17-22 September 2006 (http://www.isroses.org).

This workshop will facilitate our quest for a deeper understanding of solar cycle variations, Sun-like star variability, solar influences on climate change, and decadal climate variations. This workshop is especially timely as we anticipate an upcoming solar cycle that will likely differ significantly from the past three cycles. Sessions are organized around the following science questions:

This is the 13th general meeting in Solar Physics in Europe, a tri-annual event that covers and welcomes contributions from all aspects of contemporary solar physics. The conference's Science Program is a non-exhaustive list of topics designed to expose the breadth and diversity of current research undertaken by the international solar physics community, but more general contributions not necessarily falling into these research categories will also be accommodated.

The main purpose of the International Symposium on Recent Observations and Simulations of the Sun-Earth System II (ISROSES-II) is to bring together cross-disciplinary scientists from around the globe to have focused discussions on fundamental problems related to the space environment of the Earth. It is a continuation of the highly successful ISROSES symposium held in Varna, Bulgaria, during 17-22 September 2006 (http://www.isroses.org).

This workshop will facilitate our quest for a deeper understanding of solar cycle variations, Sun-like star variability, solar influences on climate change, and decadal climate variations. This workshop is especially timely as we anticipate an upcoming solar cycle that will likely differ significantly from the past three cycles. Sessions are organized around the following science questions:

This is the 13th general meeting in Solar Physics in Europe, a tri-annual event that covers and welcomes contributions from all aspects of contemporary solar physics. The conference's Science Program is a non-exhaustive list of topics designed to expose the breadth and diversity of current research undertaken by the international solar physics community, but more general contributions not necessarily falling into these research categories will also be accommodated.

The main purpose of the International Symposium on Recent Observations and Simulations of the Sun-Earth System II (ISROSES-II) is to bring together cross-disciplinary scientists from around the globe to have focused discussions on fundamental problems related to the space environment of the Earth. It is a continuation of the highly successful ISROSES symposium held in Varna, Bulgaria, during 17-22 September 2006 (http://www.isroses.org).

This workshop will facilitate our quest for a deeper understanding of solar cycle variations, Sun-like star variability, solar influences on climate change, and decadal climate variations. This workshop is especially timely as we anticipate an upcoming solar cycle that will likely differ significantly from the past three cycles. Sessions are organized around the following science questions:

This is the 13th general meeting in Solar Physics in Europe, a tri-annual event that covers and welcomes contributions from all aspects of contemporary solar physics. The conference's Science Program is a non-exhaustive list of topics designed to expose the breadth and diversity of current research undertaken by the international solar physics community, but more general contributions not necessarily falling into these research categories will also be accommodated.

The main purpose of the International Symposium on Recent Observations and Simulations of the Sun-Earth System II (ISROSES-II) is to bring together cross-disciplinary scientists from around the globe to have focused discussions on fundamental problems related to the space environment of the Earth. It is a continuation of the highly successful ISROSES symposium held in Varna, Bulgaria, during 17-22 September 2006 (http://www.isroses.org).

This workshop will facilitate our quest for a deeper understanding of solar cycle variations, Sun-like star variability, solar influences on climate change, and decadal climate variations. This workshop is especially timely as we anticipate an upcoming solar cycle that will likely differ significantly from the past three cycles. Sessions are organized around the following science questions:

Our actions are defined around four vectors: 1. High Quality Technical Contents, 2. it is Multidisciplinary, 3. Worldwide Participants and 4. it is a People-oriented Conference. By organising a very attractive Conference we expect to increase the number of contributors, as well as the quality of the selected papers. Our aim is to have three different “worlds” converge and be present in the area of radiation effects on components and systems, namely: Academia, Public Institutions and Industry.

ESLAB is an annual meeting organised by the European Space Agency's Directorate of Science and Robotic Exploration's Research and Scientific Support Department. This year it will be combined with the 21st Cluster workshop with broad themes focusing on the nature of space plasma physics as sampled from in-situ and remote sensing instruments.

Our actions are defined around four vectors: 1. High Quality Technical Contents, 2. it is Multidisciplinary, 3. Worldwide Participants and 4. it is a People-oriented Conference. By organising a very attractive Conference we expect to increase the number of contributors, as well as the quality of the selected papers. Our aim is to have three different “worlds” converge and be present in the area of radiation effects on components and systems, namely: Academia, Public Institutions and Industry.

ESLAB is an annual meeting organised by the European Space Agency's Directorate of Science and Robotic Exploration's Research and Scientific Support Department. This year it will be combined with the 21st Cluster workshop with broad themes focusing on the nature of space plasma physics as sampled from in-situ and remote sensing instruments.

Our actions are defined around four vectors: 1. High Quality Technical Contents, 2. it is Multidisciplinary, 3. Worldwide Participants and 4. it is a People-oriented Conference. By organising a very attractive Conference we expect to increase the number of contributors, as well as the quality of the selected papers. Our aim is to have three different “worlds” converge and be present in the area of radiation effects on components and systems, namely: Academia, Public Institutions and Industry.

ESLAB is an annual meeting organised by the European Space Agency's Directorate of Science and Robotic Exploration's Research and Scientific Support Department. This year it will be combined with the 21st Cluster workshop with broad themes focusing on the nature of space plasma physics as sampled from in-situ and remote sensing instruments.

Our actions are defined around four vectors: 1. High Quality Technical Contents, 2. it is Multidisciplinary, 3. Worldwide Participants and 4. it is a People-oriented Conference. By organising a very attractive Conference we expect to increase the number of contributors, as well as the quality of the selected papers. Our aim is to have three different “worlds” converge and be present in the area of radiation effects on components and systems, namely: Academia, Public Institutions and Industry.

ESLAB is an annual meeting organised by the European Space Agency's Directorate of Science and Robotic Exploration's Research and Scientific Support Department. This year it will be combined with the 21st Cluster workshop with broad themes focusing on the nature of space plasma physics as sampled from in-situ and remote sensing instruments.

Our actions are defined around four vectors: 1. High Quality Technical Contents, 2. it is Multidisciplinary, 3. Worldwide Participants and 4. it is a People-oriented Conference. By organising a very attractive Conference we expect to increase the number of contributors, as well as the quality of the selected papers. Our aim is to have three different “worlds” converge and be present in the area of radiation effects on components and systems, namely: Academia, Public Institutions and Industry.

ESLAB is an annual meeting organised by the European Space Agency's Directorate of Science and Robotic Exploration's Research and Scientific Support Department. This year it will be combined with the 21st Cluster workshop with broad themes focusing on the nature of space plasma physics as sampled from in-situ and remote sensing instruments.

The goal of IAU S286 will be to consider solar and stellar minima, from generative dynamo mechanisms, to in-depth analyses from Sun to Earth for recent well-observed and modeled minima, to the range in stellar cyclic activity, to outlier "grand minima". Solar, heliospheric, geospace, atmospheric, stellar, and planetary science are included in the meeting's scope. The meeting will be held in Mendoza, Argentina, at the foot of the Andes Mountains: "The land of Sun and good wine". Website: http://iaus286.iafe.uba.ar/

The goal of IAU S286 will be to consider solar and stellar minima, from generative dynamo mechanisms, to in-depth analyses from Sun to Earth for recent well-observed and modeled minima, to the range in stellar cyclic activity, to outlier "grand minima". Solar, heliospheric, geospace, atmospheric, stellar, and planetary science are included in the meeting's scope. The meeting will be held in Mendoza, Argentina, at the foot of the Andes Mountains: "The land of Sun and good wine". Website: http://iaus286.iafe.uba.ar/

The goal of IAU S286 will be to consider solar and stellar minima, from generative dynamo mechanisms, to in-depth analyses from Sun to Earth for recent well-observed and modeled minima, to the range in stellar cyclic activity, to outlier "grand minima". Solar, heliospheric, geospace, atmospheric, stellar, and planetary science are included in the meeting's scope. The meeting will be held in Mendoza, Argentina, at the foot of the Andes Mountains: "The land of Sun and good wine". Website: http://iaus286.iafe.uba.ar/

The goal of IAU S286 will be to consider solar and stellar minima, from generative dynamo mechanisms, to in-depth analyses from Sun to Earth for recent well-observed and modeled minima, to the range in stellar cyclic activity, to outlier "grand minima". Solar, heliospheric, geospace, atmospheric, stellar, and planetary science are included in the meeting's scope. The meeting will be held in Mendoza, Argentina, at the foot of the Andes Mountains: "The land of Sun and good wine". Website: http://iaus286.iafe.uba.ar/

The goal of IAU S286 will be to consider solar and stellar minima, from generative dynamo mechanisms, to in-depth analyses from Sun to Earth for recent well-observed and modeled minima, to the range in stellar cyclic activity, to outlier "grand minima". Solar, heliospheric, geospace, atmospheric, stellar, and planetary science are included in the meeting's scope. The meeting will be held in Mendoza, Argentina, at the foot of the Andes Mountains: "The land of Sun and good wine". Website: http://iaus286.iafe.uba.ar/

Hinode, the 3rd Japanese led international solar mission, is improving our understanding of the mechanisms that power the solar atmosphere and drive solar eruptions. Launched in 2006, the Hinode satellite is an international collaboration of space agencies, industry and research organizations dedicated to measuring solar magnetic fields. The Hinode-5 meeting will bring scientists from all over the world together to discuss breakthroughs in our understanding of the Sun and the origins of space weather events as we approach the next maximum in solar activity.

Hinode, the 3rd Japanese led international solar mission, is improving our understanding of the mechanisms that power the solar atmosphere and drive solar eruptions. Launched in 2006, the Hinode satellite is an international collaboration of space agencies, industry and research organizations dedicated to measuring solar magnetic fields. The Hinode-5 meeting will bring scientists from all over the world together to discuss breakthroughs in our understanding of the Sun and the origins of space weather events as we approach the next maximum in solar activity.

Hinode, the 3rd Japanese led international solar mission, is improving our understanding of the mechanisms that power the solar atmosphere and drive solar eruptions. Launched in 2006, the Hinode satellite is an international collaboration of space agencies, industry and research organizations dedicated to measuring solar magnetic fields. The Hinode-5 meeting will bring scientists from all over the world together to discuss breakthroughs in our understanding of the Sun and the origins of space weather events as we approach the next maximum in solar activity.

Hinode, the 3rd Japanese led international solar mission, is improving our understanding of the mechanisms that power the solar atmosphere and drive solar eruptions. Launched in 2006, the Hinode satellite is an international collaboration of space agencies, industry and research organizations dedicated to measuring solar magnetic fields. The Hinode-5 meeting will bring scientists from all over the world together to discuss breakthroughs in our understanding of the Sun and the origins of space weather events as we approach the next maximum in solar activity.

The 12th RHESSI workshop will be held at the Purple Mountain Observatory in Nanjing, P.R.China on 17-21 Oct. 2011. This Workshop will be hosted by the Purple Mountain Observatory (PMO) and sponsored by the National Natural Science Foundation of China (NSFC) and Chinese Academy of Sciences (CAS). Website: http://12th-rhessi.csp.escience.cn/dct/page/1

The 12th RHESSI workshop will be held at the Purple Mountain Observatory in Nanjing, P.R.China on 17-21 Oct. 2011. This Workshop will be hosted by the Purple Mountain Observatory (PMO) and sponsored by the National Natural Science Foundation of China (NSFC) and Chinese Academy of Sciences (CAS). Website: http://12th-rhessi.csp.escience.cn/dct/page/1

The 12th RHESSI workshop will be held at the Purple Mountain Observatory in Nanjing, P.R.China on 17-21 Oct. 2011. This Workshop will be hosted by the Purple Mountain Observatory (PMO) and sponsored by the National Natural Science Foundation of China (NSFC) and Chinese Academy of Sciences (CAS). Website: http://12th-rhessi.csp.escience.cn/dct/page/1

The 12th RHESSI workshop will be held at the Purple Mountain Observatory in Nanjing, P.R.China on 17-21 Oct. 2011. This Workshop will be hosted by the Purple Mountain Observatory (PMO) and sponsored by the National Natural Science Foundation of China (NSFC) and Chinese Academy of Sciences (CAS). Website: http://12th-rhessi.csp.escience.cn/dct/page/1

The 12th RHESSI workshop will be held at the Purple Mountain Observatory in Nanjing, P.R.China on 17-21 Oct. 2011. This Workshop will be hosted by the Purple Mountain Observatory (PMO) and sponsored by the National Natural Science Foundation of China (NSFC) and Chinese Academy of Sciences (CAS). Website: http://12th-rhessi.csp.escience.cn/dct/page/1

Extreme space-weather events such as geomagnetic storms are natural phenomena caused by solar activity that can have a serious impact on modern technological infrastructures such as electrical power grids, telecommunication, global satellite navigation (GNSS) and banking. In view of the upcoming solar maximum expected in 2013 the “Space-Weather Awareness Dialogue” aims at raising awareness of the potential impact of space weather on critical infrastructures in view of the growing risk of technological catastrophic events.

Extreme space-weather events such as geomagnetic storms are natural phenomena caused by solar activity that can have a serious impact on modern technological infrastructures such as electrical power grids, telecommunication, global satellite navigation (GNSS) and banking. In view of the upcoming solar maximum expected in 2013 the “Space-Weather Awareness Dialogue” aims at raising awareness of the potential impact of space weather on critical infrastructures in view of the growing risk of technological catastrophic events.

The LWS/SDO-3/GONG-2011 Workshop "Solar Dynamics and Magnetism from the Interior to the Atmosphere" will be held on Oct.31-Nov.4, 2011, at the NASA/Ames Conf. Center, Moffett Field, CA. The goal of the workshop is to discuss recent advances in our understanding of the solar dynamics and magnetism, and to explore links between the interior and the atmosphere. The Workshop will focus on new results from the Solar Dynamics Observatory, GONG, other space missions and ground-based observatories, as well as on numerical simulations and theoretical modeling.

The LWS/SDO-3/GONG-2011 Workshop "Solar Dynamics and Magnetism from the Interior to the Atmosphere" will be held on Oct.31-Nov.4, 2011, at the NASA/Ames Conf. Center, Moffett Field, CA. The goal of the workshop is to discuss recent advances in our understanding of the solar dynamics and magnetism, and to explore links between the interior and the atmosphere. The Workshop will focus on new results from the Solar Dynamics Observatory, GONG, other space missions and ground-based observatories, as well as on numerical simulations and theoretical modeling.

The LWS/SDO-3/GONG-2011 Workshop "Solar Dynamics and Magnetism from the Interior to the Atmosphere" will be held on Oct.31-Nov.4, 2011, at the NASA/Ames Conf. Center, Moffett Field, CA. The goal of the workshop is to discuss recent advances in our understanding of the solar dynamics and magnetism, and to explore links between the interior and the atmosphere. The Workshop will focus on new results from the Solar Dynamics Observatory, GONG, other space missions and ground-based observatories, as well as on numerical simulations and theoretical modeling.

The LWS/SDO-3/GONG-2011 Workshop "Solar Dynamics and Magnetism from the Interior to the Atmosphere" will be held on Oct.31-Nov.4, 2011, at the NASA/Ames Conf. Center, Moffett Field, CA. The goal of the workshop is to discuss recent advances in our understanding of the solar dynamics and magnetism, and to explore links between the interior and the atmosphere. The Workshop will focus on new results from the Solar Dynamics Observatory, GONG, other space missions and ground-based observatories, as well as on numerical simulations and theoretical modeling.

The LWS/SDO-3/GONG-2011 Workshop "Solar Dynamics and Magnetism from the Interior to the Atmosphere" will be held on Oct.31-Nov.4, 2011, at the NASA/Ames Conf. Center, Moffett Field, CA. The goal of the workshop is to discuss recent advances in our understanding of the solar dynamics and magnetism, and to explore links between the interior and the atmosphere. The Workshop will focus on new results from the Solar Dynamics Observatory, GONG, other space missions and ground-based observatories, as well as on numerical simulations and theoretical modeling.

This workshop focuses on connectivity science that looks at the solar atmosphere as a systemconnected by solar magnetic fields. Particular emphasis will be on discussing the new capabilities that large aperture solar telescopes will provide for observing and measuring magnetic fields and their dynamic behavior from the photosphere to the corona. This 2nd joint ATST-EAST workshop continues to demonstrate the common interests of the European and US solar physics community toward next-generation, large-aperture solar telescopes.

This workshop focuses on connectivity science that looks at the solar atmosphere as a systemconnected by solar magnetic fields. Particular emphasis will be on discussing the new capabilities that large aperture solar telescopes will provide for observing and measuring magnetic fields and their dynamic behavior from the photosphere to the corona. This 2nd joint ATST-EAST workshop continues to demonstrate the common interests of the European and US solar physics community toward next-generation, large-aperture solar telescopes.

This workshop focuses on connectivity science that looks at the solar atmosphere as a systemconnected by solar magnetic fields. Particular emphasis will be on discussing the new capabilities that large aperture solar telescopes will provide for observing and measuring magnetic fields and their dynamic behavior from the photosphere to the corona. This 2nd joint ATST-EAST workshop continues to demonstrate the common interests of the European and US solar physics community toward next-generation, large-aperture solar telescopes.

Potential topics:

Potential topics:

Potential topics:

The 4th French-Chinese meeting on solar physics, to be held in Nice (France), in November 2011, is aimed at stimulating scientific collaborations between groups and Institutes of our two countries, by discussing projects of common interest. French and Chinese solar scientists have been pursuing a long-term collaboration, since the first French-Chinese meeting held in Xi'an (1999). The 3rd, and so far last, French-Chinese meeting was held in Shanghaï in November 2005, and a SMESE workshop was organised in Paris in March 2008.