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Showing 1 to 8 of 8 for “"National Solar Observatory"”.

  1. High resolution solar observations from first principles to applications

    The expression "high-resolution observations" in Solar Physics refers to the spatial, temporal and spectral domains in their entirety. High-resolution observations of solar fine structure are a necessity to answer many of the intriguing questions related to solar activity. However, a researcher …

    njit Repository record for High resolution solar observations from first principles to applications (opens in a new tab)

  2. Magnetic reconnection in small and large scales on the sun

    Almost all solar activities observed are related to the solar magnetic field, especially the topological restructuring of magnetic fields, the so-called magnetic reconnection in solar physics. They are occurring at different scales related to various phenomena, during minimum or maximum of the …

    njit Repository record for Magnetic reconnection in small and large scales on the sun (opens in a new tab)

  3. Comparing Different Methods for Estimating Total Open Heliospheric Magnetic Flux

    <p>There are extended periods over the solar cycle where significant discrepancies occur between the observed open magnetic flux (i.e., those based on spacecraft observations) and that determined from coronal models. One explanation for the source of these discrepancies is the magnetic fields in …

    embry-riddle Repository record for Comparing Different Methods for Estimating Total Open Heliospheric Magnetic Flux (opens in a new tab)

  4. The Lunar Exosphere: Spatial and Temporal Variations of Sodium and Potassium Emissions from November 2013 to May 2014

    … and velocities. Observations were made from the National Solar Observatory (MMP) at Kitt Peak, Arizona from November 2013 to May 2014, with the exception of March 2014. Data collection was centered of full moon and spanned several nights with lunar phase angle coverage ranging from 65.6° (waxing) …

    embry-riddle Repository record for The Lunar Exosphere: Spatial and Temporal Variations of Sodium and Potassium Emissions from November 2013 to May 2014 (opens in a new tab)

  5. Design and application of near infrared tunable filter for ATST and NST

    … Tunable Filter (NIRTF) of Advanced Technology Solar Telescope (ATST) project and the Near Infrared Imaging Magnetograph (IRIM) of the New Solar Telescope (NST), the design of achromatic waveplates, the narrowband continuum observation of a Sunspot at 1.56 um using IRIM instruments, and the …

    njit Repository record for Design and application of near infrared tunable filter for ATST and NST (opens in a new tab)

  6. Setting Constraints on the Lunar Exosphere: A Comprehensive Analysis of Velocity Resolved Sodium and Potassium Line Profile Measurements

    … lunar exosphere. Observations were made at the National Solar Observatory McMath – Pierce Telescope, Kitt Peak, Arizona where I personally collected both sodium and potassium data over about a dozen observing runs. This work builds on the initial velocity resolved measurement analysis of sodium …

    embry-riddle Repository record for Setting Constraints on the Lunar Exosphere: A Comprehensive Analysis of Velocity Resolved Sodium and Potassium Line Profile Measurements (opens in a new tab)

  7. Studies of solar white-light flares and small-scale magnetic structures observed in the near infrared

    … as developed by NJIT, detailed study of solar white-light flares and small magnetic structures, such as faculae and pores, are presented in this dissertation. The investigations focus on near-infrared observations at 1.56 um, which are good proxy of the deepest layer of the solar

    njit Repository record for Studies of solar white-light flares and small-scale magnetic structures observed in the near infrared (opens in a new tab)

  8. Estimation of the vertical wavelength of atmospheric gravity waves from airglow imagery

    Abstract In the summer of 2010, two imagers were installed in New Mexico with the objective of making stereoscopic observations of atmospheric gravity waves (AGWs). As AGWs propagate vertically, they spatially perturb the airglow emission layers in all three dimensions. Estimates of the vertical …

    uiuc Repository record for Estimation of the vertical wavelength of atmospheric gravity waves from airglow imagery (opens in a new tab)