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Kadi Sarva Vishwavidyalaya KSV University, Gandhinagar near AhmedabadIndia is a private university, which runs courses in engineering, sciences, pharmacy, commerce and management. Sc Physics with a special paper on Space and Astrophysics. For this program we are planning to establish a lab with some good experiments related to space and astrophysics. In this context, we are planning to set-up a modest observatory with one telescope to observe the Sun and other to observe the night time celestial objects to teach and train the students with observational techniques and data analysis etc.

We also seek help and appreciate receiving gift of Celeostat, good quality lenses, associated optics and other accessories to build spectrographs etc. Electric currents are fundamental to the structure and dynamics of cetneno plasmas. New developments in observations, simulations and theory make it timely to collect new research studies on electric currents.

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Hence, this special issue of JGR-Space Physics solicits research papers on electric currents in the ionospheres and magnetospheres of the Earth and other planets, in the heliosphere, and on the Sun. Studies are welcome addressing not only current system robert and dynamics but also the impacts and ramifications on the local space environment. Many naciinal the collected papers will be based on presentations and discussions at a recent AGU Chapman conference held in Dubrovnik, Croatia, in May Papers relevant to the scope but not presented at the conference are also solicited.

Manuscripts should be submitted through the website: For additional information please contact: As indicated in the NOI, scoping comments may be submitted to the National Science Foundation during the public comment period, which extends through August 5,via email at envcomp-AST-sacpeak nsf.

Comments may also be provided during the public scoping meeting scheduled for July 21, at the following location:. July 21,6: Sacramento Peak Notice of Intent at www. Please note that comments must be submitted via the mechanisms described above in order to be considered. The F-CHROMA consortium would like to announce the availability of a large number of solar flare datasets, obtained from ground-based solar facilities during the two most recent solar cycles.

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A few of these datasets are currently available online through a simple wiki interface, and more will be made available in the next months.

For each flare entry links to corresponding space-based observations are also provided. Among the main questions which the project seeks to answer, are: If not, what is the expectation for cycle 25? For the next few decades, what can we expect in terms of extreme solar flares and storms, and also absence of activity? What is the expectation for periods with absence of activity? A special issue of the Journal of Atmospheric and Solar-Terrestrial Physics will include papers based on the presentations at this forum, as well as other contributions related to its topics www.

Sep 1st, Submission Deadline: Feb 1st, Acceptance Deadline: Our current fleet of space-based solar observatories offer us a wealth of opportunities to study solar flares over a range of wavelengths, and the greatest advances in our understanding of flare physics often come from coordinated observations between different instruments.

However, finding or keeping track of which flares have been observed by specific combinations of instruments can be cumbersome and time consuming. After selecting a time range it defaults to the beginning of the SDO mission to the present dayand which combination of instruments you require to address a given science question, along with options for GOES class, maximum energy observed by RHESSI, and flare location disk or limbetc, click the Search button.


This will return a list of flares that conform to your search criteria. Clicking on a given flare in this list will call up a plot that containing 1 the GOES X-ray lightcurves with the timing of your chosen observations overlaid, 2 the RHESSI lightcurves up to the maximum recorded energy, and 3 a RHESSI full-disk quicklook image with the fields of view of the different instruments overlaid.

The option exists to also download a copy of this. Future improvements to this service will include adding flares that were not observed by RHESSI, adding additional instruments e.

Please address any questions, comments or requests to r. In addition to the various research activities in the area of Space Weather, the Royal Observatory of Belgium, as a federal Belgian institute, provides services to citizens, industry and government by means of alerts and predictions for space weather. To assure the successful continuation of our operations in this context, the Royal Observatory of Belgium seeks a collaborator for the further development and support of its Space Weather Services.

Applicants must maximally combine the following criteria: The offered position is immediately available and will be scaled according to the applicable scales for Belgian federal institutes depending on the qualifications of the candidate. To apply, please send your CV and an accompanying motivation letter as soon as possible to jesse. Applications are welcome till August 15 included.

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For further enquiries contact jesse. The aim of these fellowships is to provide young scientists, holding a PhD or the equivalent degree, with the means of performing space science research in fields related to the ESA Science and Robotic Exploration Programmes. Areas of research include planetary science, astronomy and astrophysics, solar and solar-terrestrial science, plasma physics and fundamental physics.

Applications are now solicited for fellowships in space science to begin in the fall of Preference will be given to applications submitted by candidates within five years of receiving their PhD.

Candidates not holding a PhD yet are encouraged to apply, but they must provide evidence of receiving their degree disoarate starting the fellowship. A monthly deduction covers these short-term and long-term risks. More information on the ESA Research Fellowship programme in Space Science, on the conditions and eligibility, as well nqcional the application form can retrieved from cosmos.

Questions on the scientific aspects of the ESA Fellowship in Space Science not answered in the above pages can be sent by e-mail to the fellowship coordinators, Dr. Oliver Rkberto or Dr. Bruno Altieri at the address fellowship cosmos. The research fields covered by the PhD program are: The poster is available at: Examples of PhD projects available can be found at: Application forms and instructions can be found at: September 9th, Interviews will starts on September 12th,at 9 am.

Any possible question on the selection modes must be addressed to pasquale. The incumbent will manage major research and analysis and advanced technology programs, as well as represent the scientific interests of several current and future NASA missions within SMD.

The incumbent will participate in developing budgets for major agency initiatives, program plans for data analysis and science operations, and long-range strategic plans for SMD. This position is an excellent opportunity for an experienced scientist to affect positively the future of heliophysics in the U. Applicants are expected to centen able to succeed in a demanding work environment cemteno to demonstrate a high degree of initiative.

Applicants should be familiar with the U.

Secondary Bibliography A-Z

Open to all U. This session will investigate the conditions under which the most geo-effective coronal mass ejections CMEs form and propagate in the corona and interplanetary space. Abstracts are invited that discuss topics such as the identification and characterization of the solar source region of the eruption, preconditioning of the corona and heliosphere for CME propagation, interactions of CMEs with the ambient solar wind structures and other CMEs, transformation of the CME flux rope, and geo-effective plasma and magnetic field characteristics at the Earth.


Contributions that discuss multi-point observations and modeling that address these questions are especially welcome. Wednesday, 3 August We will discuss mission progress and the exciting scientific preparations going on to be ready for the data these exciting missions will return!

Understanding coronal heating and solar wind acceleration, unveiling the mechanisms of coronal mass ejections and energetic particle acceleration, linking the magnetic field evolution from the solar interior to its consequences in terms of solar variability and space weather are at the core of heliophysics exploration in the next decade with Solar Probe Plus and Solar Orbiter.

While each mission will achieve its own important science objectives, taken together they will be capable of doing simultaneous and synergized observations to best address these questions. This session focuses on opportunities and capabilities for coordinated science studies with advanced instrumentation on multiple spacecraft, assets at Earth and beyond, and sophisticated modeling of basic plasma physical processes on multiple scales that will be key to understand the dynamics of the solar atmosphere from the base of the corona into the inner heliosphere, the origins of the solar wind and its evolution from the sun.

Space weather events are driven by eruptive activity originating on the Sun. The plasma dynamics and radiation signatures depend on the magnetic field configuration in the lower solar atmosphere, whereas the magnetic environment in the intervening heliospheric volume determines its geo-effectiveness.

This session focuses on the complex magnetic environment from the Sun to 1 AU, knowledge of which is crucial to understanding and forecasting solar eruptions and their impact on Earth. We invite contributions that preferably combine theoretical and observational knowledge taken from two or more of the following themes: The early abstract deadline is July 27th, and the final deadline is August 3.

We look forward to seeing you in San Francisco this December! The description of the session is given below. Abstracts may be submitted here.

The Sun influences the Earth through a complex set of interactions across interplanetary space. The behavior of this system is measured by many different instruments that produce many varied data. In the near future, the Daniel K. These disparate data are essentially different views of nafional same Sun-Earth system.

Maximizing the scientific output from these variegated data is the key to progress, and the subject of this session. We solicit contributions covering the following topics: This session will provide a venue for discussion on these two closely related, but traditionally separated phenomena, and thus facilitate cross-disciplinary collaboration.

Important dates for abstracts submission: The solar corona is hot and tenuous. Yet, it hosts a variety of mysteriously cool and dense plasma nadional, primarily in two distinct forms – prominences and coronal rain.

Their importance has been increasingly recognized, especially with the advent of the IRIS mission since They can involve a radiative cooling instability that causes hot coronal mass to condense and fall back to the chromosphere, closing the loop of the corona-chromosphere mass cycle and providing implications for the fundamental coronal heating problem.

Some prominences form the nacionla of Nacioanl that are major drivers of space-weather disturbances. We invite contributions on such topics as observational and modeling investigations of the formation and dynamics of prominences and coronal rain, their magnetic and plasma environments, their relevant physical processes such as ion-neutral coupling and magnetic reconnection in partially ionized plasmas, their diagnostic applications, disparatw their space-weather consequences and predictive potential.

The full session description, and a link to submit an abstract, can be found here: We look forward to welcoming you. A first announcement with more details will follow in September In the meantime, please save the date to your diary, bookmark and register your dizparate at www.