This service contributes to the International Service of Geomagnetic Indices (ISGI) of the IAGA . ... The Kp numbers of the previous month are available in tabular format . ... There are available also historical and current Kp and derived indices per anonoymos FTP (see below). ... U.S.A. FTP server: ftp://ftp.ngdc.noaa.gov/STP/GEOMAGNETIC_DATA/INDICES/KP_AP/ . monthly update) . ... contains the monthly Kp / ap tables in a simple text format readable for both humans and computers (*.tab). ...

Since the light from galaxies represents the integrated contribution of its consitutient stars, then we can learn about stellar populations in galaxies by modelling their light by summing up individual stellar spectra for different kinds of stars. ... The data cover the wavelength range 3500 - 9000 angstroms. ... Retrieve Digital Stellar Spectra Click on the appropriate spectral type. ... Note that the designation V means main sequence, IV means subgiants, III means giants, I means supergiant. ...

I'm glad you're interested in collaborating on the ConcepTests for Astronomy WWW database project! ... I'm looking forward to your contributions! ... a) high luminosity, high temperature to low luminosity, low temperature . b) high luminosity, low temperature to low luminosity, low temperature . c) high luminosity, low temperature to low luminosity, high temperature . d) high luminosity, high temperature to low luminosity high temperature. ... Back to Paul Green's Peer Instruction page. ...

Permitted Context: SELECT . ... The OPTION element can only occur within a SELECT element. ... When the form is submitted, the NAME of the enclosing SELECT element is paired with the OPTION's VALUE attribute to contribute a name/value pair for the selection. ... CLASS . ... The string to be used together with the name attribute of the enclosing select element, when submitting the form. ... SELECTED . ... This attribute is used within menus to define shaped hotzones associated with this option's value. ...

... Programme . ... Abstract: As the nearest early-type galaxy, Centaurus A contains a treasure trove of information about X-ray binaries. With over 700 ks of Chandra observations spread over 10 years, the Centaurus A Very Large Project provides the deepest look at X-ray binaries in an early-type galaxy. ... Preliminary results have already shed light on the low-mass X-ray binary connection to globular clusters and the discovery of a remarkable transient ultra-luminous X-ray source. ...

... Section 1: Astrometry and Celestial Mechanics Section 2: Solar Physics and Solar-Terrestrial Coupling Section 3: Galaxies and Cosmology Section 4: Physics of the Stars and Interstellar Medium Section 5: Planetary Systems Section 6: The History of Astronomy Section 7: Problems of Astronomical Education . ... no need travel accommodation waiving of the registration fee . ...

Proceedings of the XXVIIth Young European Radio Astronomers Conference (YERAC). ... Please Note: e-mail addresses and external links in these contributions were correct when these papers were written in 1995, but may no longer be valid. ... In addition to the hypertext version of each paper, indicated by the link from the title of the paper, there are links to postscript versions of each paper, which are suitable for printing if you want a hardcopy of a given paper. ... Sandor Frey (or postscript ) . ...

The information contained in this Handbook represents the cumulative experience and contributions of many members of the STScI community, including the WFPC2, WFC3, ACS, NICMOS and STIS instrument groups, the Observatory Support Group and the Science Software Branch. The drizzle code, which underlies all the analysis routines described here, was originally developed by Richard Hook and Andy Fruchter. ... http://www.stsci.edu . ... help@stsci.edu . ...

... Lyngby, Denmark The flux-flow oscillator (FFO) is a long Josephson junction in which a unidirectional flow of magnetic flux quanta (fluxons) generates millimeter and submillimeter electromagnetic radiation. ... The FFO voltage and thus its frequency is controlled independently by the overlap bias current, Ib, and the so called "control line" inline current, Icl, which creates the magnetic field at the ends of the FFO. ...

Next: Acknowledgements Up: A Database of Optical Previous: Hydrogenated amorphous carbon . We have presented recent developments in the Jena-Petersburg Database of Optical Constants (JPDOC) and have demonstrated examples for application of the optical constants contained for purposes of comparison with astronomical spectroscopic observations. ... The authors will highly acknowledge any contribution to the database such as references, data files and links to be included in the database. ...

... Armagh Observatory, College Hill, Armagh BT61 9DG, +44 (0)28 3752 2928 . ... Sample fits to the SB2 observations of HD 22128 (top two frames) and HD 56495 (bottom two frames). Fits (smooth lines) to the observations (points) show the combined synthetic spectra, as well as the two component synthetic spectra. ... HD 22128 and HD 56495 are both double-lined spectroscopic binary systems with short orbital periods, which have been proposed to host magnetic Ap stars. ...

... 30, 2006 . ... If you retrieve these files via a Web browser, please note that you need to use the browser's "Save As..." facility. ... Figures must be provided as Encapsulated PostScript files and should be incorporated in your contribution using the standard Latex2e "graphicx" package as demonstrated in the demo file author.tex. ... Please submit the LaTeX source file of your contribution, and PostScript/PDF files of any figures, via email (!!!) to Iris Bronnert ( ibronner@eso.org ). ...

Next: Enabling Technologies for Astronomy . ... Astronomical Data Analysis Software and Systems X . ... The ADASS Conference Series provides a forum for scientists and computer specialists concerned with development of software for enabling technologies for Astronomy, sky surveys, science data pipelines, software development methodologies and technologies, education and public outreach, and software history. ... The conference was hosted by the Smithsonian Astrophysical Observatory (SAO). ...

... 8, ``Celestial Mechanics'', 2002 Two problems in solar systems dynamics, possible solutions and future A. Fienga IMCCE­Observatoire de Paris, Paris, France In this contribution, two major aspects of the new challenges of the solar system dynamics are presented. ... As it was demonstrated by (Standish and Fienga [4]), the perturbations of the Mars orbit by the asteroids are difficult to modelize and they present now the main limitation of the present theory of Mars motion. ...

The CHIANTI database consists of 4 primary ASCII files for each ion in the database. contains the energy levels in cm^(-1) It includes both experimental data and theoretical values of the levels energies. ... ADNDT, 1987, 37, 17 % produced as part of the Arcetri/Cambridge/NRL 'CHIANTI' atomic data base collaboration % % E. Landi - Mar 2005 . ... 1987, ADNDT, 37, 17 %produced as part of the Arcetri/Cambridge/NRL 'CHIANTI' atomic data base collaboration % % E. Landi 2000 . ...

... Song PLRFC File ---- ---------- 17 Days prflips 1999 1999 2 Nigs United 4 West Compton black.album 2 Sexy instrumental 2 The Wire instrumental 2 Whom It May Concern draft_1 200 Balloons batman 3 Chains o' Gold o+v 4 the Tears in Your Eyes around.the.world.in.a.day 7 o+v A Better Place 2 Die draft A Place in Heaven draft A-U-T-O-matic 1999 Adore sign.o.the.times Alexa De Paris instrumental All the Critics Love U in New York 1999 Alphabet Street ...

Astronotes Armagh Planetarium's Stellar Blog! ... Space Flight . ... January . ... By admin January 3, 2011 Posted in: Armagh Planetarium . ... Hosted by Professor Brian Cox (science advisor to the movie тАЬ Sunshine тАЭ, but we wonтАЩt hold that against him) and comedian Dara O Briain (who trained as a physicist), BBC Stargazing Live will include live observing featuring epic images from observatories around the globe on 3 ? ... Tweets that mention BBC Stargazing Live at Armagh Planetarium | ...

PENTICTON SOLAR RADIO FLUX VALUES (from SGD Explanation of Data Reports) Daily Solar Flux Values - Penticton -- Daily measurements of the integrated emission from the solar disc at 2800MHz (10.7cm wavelength) have been made by the National Research Council of Canada since 1947. ... The data are tabulated in two forms: the "observed flux" (S), and the "adjusted flux" (Sa). ... The "observed flux" values are useful in ionospheric physics and other terrestrial consequences of solar activity. ...

First Name . Last Name . ... A contributed talk . A poster . ... Tentative title of your oral contribution/poster . Required if ask for a Poster or Talk . ... Required if you are member of a collaboration . Short abstract of your oral contribution/poster . Required if you ask for a Poster or Talk . Options . ... Please select additional options . ... Please check the required fields. Powered by jqueryform.com . ...