![]() ![]() Solar activity monitoring and forecasting capabilities at Big Bear Solar Observatoryĭirectory of Open Access Journals (Sweden)įull Text Available The availability of full-disk, high-resolution Ha images from Big Bear Solar Observatory (USA, Kanzelhöhe Solar Observatory (Austria, and Yunnan Astronomical Observatory (China allows for the continual monitoring of solar activity with unprecedented spatial and temporal resolution. We examine some of the challenges and potential of such a "meta-VO." Over the next few years, this integration will be especially obvious as the NASA Heliophysics division sponsors the development of a heliophysics-wide virtual observatory (VO), based on existing VO's in heliospheric, magnetospheric, and ionospheric physics as well as the VSO. The solar physics community can use a Web interface or an Application Programming Interface (API) that allows integrating VSO searches into other software, including other Web services. The Virtual Solar Observatory (VSO) is now able to search for solar data ranging from the radio to gamma rays, obtained from space and groundbased observatories, from 26 sources at 12 data providers, and from 1915 to the present. WiPPL and its leadership are fully committed to a diverse, equitable and inclusive research community and follow the policies of the UW Physics Department DEI plan.The Virtual Solar Observatory and the Heliophysics Meta-Virtual Observatory Exploiting the flexibility of the Big Red Ball and Madison Symmetric Torus devices to address the breadth of topics in energy flow as part of a coordinated multi-investigator Wisconsin Plasma Physics Laboratory (WiPPL) operating as a versatile user facility.Promoting collaborative and outreach activities with space and astro physicists through strong connections between astronomy and physics,.Creating and diagnosing plasmas with unique and wide ranging dimensionless parameters and geometries capable of studying energy transformation between forms that are inspired by astrophysical and space plasma phenomena. ![]() Strategy: Carry out this mission and vision by Mission: Push the frontier of experimental plasma physics research, backed by theory and computation, to improve our understanding of natural plasma phenomena while providing an environment for the very best education that only first generation research projects allow. Vision: Experimentally advance our understanding of how energy flows between fields and particles in a plasma and thereby advance a major physics frontier while providing an experimental plasma facility with unprecedented range and scope of parameters and operating conditions. The vision, mission and strategy of WiPPL Scientific and technical staff operate the two devices on behalf of all users. The combined capabilities of these two devices and their associated infrastructure creates a unique opportunity to lead the world in expanding the basic plasma frontier and to fully realize the extraordinary potential of laboratory experiments to transform space and astrophysical plasma science.įor external users, WiPPL provides a suite of plasma source and diagnostic capabilities on the BRB and MST that manipulate and probe fundamental plasma processes in a variety of geometries. WiPPL coordinates the joint operation of the Big Red Plasma Ball (BRB) and Madison Symmetric Torus (MST) devices with a focus on frontier basic plasma science. WiPPL serves both UW and external users, and supports the core of a broad research program to understand the flow of energy between fields and particles in plasmas. ![]() The Wisconsin Plasma Physics Laboratory (WiPPL) is funded by the DoE Office of Fusion Energy Sciences to operate several multi-investigator, intermediate-scale plasma physics devices, and represents the Plasma Physics efforts within the University of Wisconsin Physics Department. ![]()
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