PPT-The Solar-Stellar Spectrograph (SSS) Project Review

JEFFREY HALL LOWELL OBSERVATORY FLAGSTAFF AZ Project Timeline 1988 1992 1996 2000 2004 2008 2012 Constructionearly observing Rebuild 1 Broad survey Solar analog survey Rebuild 2 AD boundary. Total Number of Passenger Coaches . 62,924 . , Surface area per coach : 40 . Sq. Meter. T. rain’s . roof top has a total surface area of 40 square . meters. Which can be used to install over 6 kW Solar system.. versus convective . blueshifts. , and wavelength variations across stellar disks. Dainis Dravins. – Lund . Observatory. , Sweden. www.astro.lu.se. /~. dainis. KVA. IAU Comm.30, IAU XXVIII GA Beijing, August 2012. Larry J. Paxton. GUVI co-PI. SSUSI PI. Why spectrograph mode?. Spectrograph mode returns the entire spectrum. When SSUSI was designed the data rate was . set as spare words in the OLD data stream – about . ?. Implications from observations of solar-type stars . and historical records. Hiroaki Isobe. Graduate School of Integrated Advanced Studies . in Human Survivability, Kyoto University. Aknowledgements. Dainis . Dravins. – Lund . Observatory. , Sweden. www.astro.lu.se. /~. dainis. KVA. Towards the science case for E-ELT . HIRES. , Cambridge UK, September 2012. STELLAR SURFACES. … where starlight and stellar spectra originate. Steven R. . Cranmer. Harvard-Smithsonian Center for . Astrophysics. . with A. van . Ballegooijen. , S. Saar, A. Dupree, N. . Brickhouse. , et al.. Stellar winds across the H-R Diagram. Massive stars: radiation-driven winds. Public Interest Groups advocated for a community solar project. Analysis performed in the Collaborative showed a surprising number of retail customers identify as green. A goal of EKPC’s Strategic Plan is to diversify its generation portfolio. Organization. Presentation Date. What is Community Solar?. Community solar refers to local solar facilities shared by individual community members, who receive credits on their electricity bills for their portion of the power produced. Can also be called a Solar Garden or Solar Farm. Three particles. Nucleus. Electrostatic Force. Strong nuclear force. Exploring Solar - 1/23/17 - ©The NEED Project . Radiant Energy. Nuclear Fusion. Exploring Solar - 1/23/17 - ©The NEED Project . Variances in Solar Radiation. Larry J. Paxton. GUVI co-PI. SSUSI PI. Why spectrograph mode?. Spectrograph mode returns the entire spectrum. When SSUSI was designed the data rate was . set as spare words in the OLD data stream – about . Angel Suarez| Open Universiteit. WAPLA Workshop| 16 September 2016. #. laceproject. , . angel.suarez@ou.nl. Presentation Outline. LACE introduction. Vision of LACE. Goals and objectives. Who we are . Commissioning, Upgrades and Future. Wenda . Cao & NST Team. BBSO was built by Caltech in 1969.. Observatory . was transferred from Caltech to NJIT in July 1997. . The dome sits at the end of a 1000 ft. causeway on Big Bear Lake’s north shore at 6,750 foot elevation.. Jeffrey . Linsky. JILA and APAS. Solar Focus Group. April 12, 2019. Why are the Lyman-α and EUV fluxes important?. Lyman-α is the brightest line in the solar UV spectrum.. Lyman-α is as bright as the entire UV spectra of M dwarf stars.. N. . Prantzos. Lecturer:. . Hans-Jürgen . Wollersheim. e-mail: . h.j.wollersheim@gsi.de. web-page: . https://web-docs.gsi.de/~. wolle/. and click on . thermodynamics. subatomic physics. Sun´s energy.