Sun-Quakes
The Advanced Technology Solar Telescope The ATST Project is funded by the National Science Foundation through the National Solar Observatory which is operated.
C.V.V. Prasad et al- Fourier Transform Jet Emission Spectroscopy of the B^2-Sigma^+-X^2-Sigma^+ Transition of CN
FOURIER TRANSFORM EMISSION SPECTROSCOPY AND AB INITIO CALCULATIONS ON WO R. S. Ram, Department of Chemistry, University of Arizona J. Liévin, Université.
Introduction By the 1950s, the biggest and best astronomy tools in the US were concentrated in a handful of universities. AURA national observatories.
From Static to Dynamic: Choosing and Implementing a CMS Ruth Kneale, [email protected] National Solar Observatory, Advanced Technology Solar Telescope.
Farside Helioseismic Holography: Recent Advances I. González Hernández (1), D. Braun (2), S. M. Hanasoge(3), F. Hill (1), C. Lindsey (2), P. Scherrer (3)
Jonathan A. Constable University of St Andrews Solar REU Presentation 2009 A flux rope model for CME initiation over solar cycle 23 Jonathan Constable.
Mapping active regions in the Far Side of the Sun using helioseismology I. González Hernández, F. Hill (1) C. Lindsey and D. Braun (2) (1) National Solar.
What coronal parameters determine solar wind speed? M. Kojima, M. Tokumaru, K. Fujiki, H. Itoh and T. Murakami Solar-Terrestrial Environment Laboratory,
F. I. Suárez-Sol á 1, E. González-Suárez 1, I. González-Hernández 1, A.R. Davey 2,J. Hourcl é 3, VSO Team 1 National Solar Observatory, Tucson AZ – 2 Harvard-Smithsonian.
Magnetogram Users Group Role of the MUG –Charge –Functioning –Agenda Scientific Objectives & Functional Requirements –One person's noise is another’s signal.
