NSF NSO, NSF NCAR HAO, and SwRI scientists have demonstrated a way to map the Sun’s 3D coronal magnetic field using existing ...

Using observations from both the SOLIS and GONG instruments, NISP produces a plethora of data products at a variety of levels. The most commonly used products are listed below. We are developing this ...

In an era when we receive our news in almost real-time —and often condensed in 140 characters— the National Solar Observatory is adapting its Newsletter to a new, more dynamic, blog format. In this ...

The Proposal Architect (PA) tool is used by proposers to prepare, validate, and submit proposals for the DKIST. The Proposal Architect tool is a web-based tool and ...

The DKIST Science Working Group works with and advises the Project Director. The membership of the DSWG includes scientists from PI and Co-I institutions as well as experts from the community. The ...

The Potential-field Source-surface (PFSS) model provides a simple and effective model for the large-scale features of the global coronal magnetic field. To capture large-scale field structure in a ...

Scientists using the U.S. National Science Foundation Daniel K. Inouye Solar Telescope have made a major breakthrough in solar physics, discovering Kelvin-Helmholtz Instability on the surface of the ...

The U.S. National Science Foundation’s (NSF’s) Daniel K. Inouye Solar Telescope (Inouye Solar Telescope) released eight new images of the Sun featuring a variety of sunspots and quiet regions of the ...

The GONG facility of NSO continually produces solar full-disk images centered on the H-αspectral line at a wavelength of 6562.8 Åin air. The image format is 2048 x 2048 pixels. The images are taken ...

Scientists from the U.S. National Science Foundation National Solar Observatory and New Jersey Institute of Technology produced the finest images of the Sun’s corona to date. To make these ...

Solar flares and coronal mass ejections are spectacular phenomena that are not only critical to the space weather environment of Earth, but reflect processes ubiquitous in astrophysical plasmas. The ...

The mission of the Cryo-NIRSP is to take advantage of the full coronagraphic capabilities of DKIST to observe both the near-limb and off-limb corona out to 1.5 Solar Radii, and, additionally, leverage ...