61. University Of Newcastle Space Physics Research Group space physics Research Group in Australia. http://plasma.newcastle.edu.au/spwg/

62. WWW Space Physics Resources space physics Models. Geomagnetic Field Models space physics Models space physics Models @ SwRI Run These Models! space physics Data Systems http://spacephysics.space.swri.edu/resrc/www.space.htm

WWW Space Physics Resources Space Weather Latest Space Weather Geophysical Indices Space Physics Data Archives Solar Data Solar Flares Solar Images Solar Indices Solar Spectra ... Solar Links Experiments Imaging the Geospace Environment Ionospheric Radars Space Experiments Space Experiments @ SwRI Geospace Geospace Environment Middle Atmosphere Space Environment Effects Space Physics Models Geomagnetic Field Models Space Physics Models Space Physics Models @ SwRI Run These Models! Space Physics Data Systems Data Formats Data Systems Software Literature Educational Resources Current Journal Contents Resources Additional Resource Lists Resource Locators Organizations Space Agencies Etc Image Gallery Search Our Web Server! Questions or comments? e-mail: help15@swri.edu 1996, 1997 Southwest Research Institute Back to home page

63. Roger Smith Professor at the University of Alaska. Includes recent papers, and details on the GI space physics undergraduate intern program. http://www.gi.alaska.edu/space/roger_smith/index.htm

Roger Smith's Home Page I am a professor of physics and associate director of the Geophysical Institute at the University of Alaska, Fairbanks most of the time. At other times, I sing tenor in the Tanana Flats barbershop quartet, lead in the Greatland Sounds Barbershop Chorus and tenor in the University Community Presbyterian Church Choir. Isa Smith, my wife, is a fiber artist who can be found most Wednesdays and some other days working at Hands All Around. I am also a fan of historic cars, having two of my own. They are both in need of restoration, but the 1936 Riley Kestrel runs well enough to drive around town. My 1967 Morris Traveller is waiting until its owner retires and has more time to devote to it. My research interest is the study of the dynamics of the high latitude upper atmosphere and also the high latitude aurora. You can look at some of my recent research work at item 1 below. I also run a summer intern program for undergraduates funded by the National Science Foundation . More information can be found about that at item 2 below. Recent papers which are in preparation or have been submitted to journals.

64. Interplanetary Space Physics For interplanetary space missions see Solar space physics Missions. Also see; Studying the Earth s Magnetosphere / space physics in the Earth section. http://members.aol.com/gca7sky/planets/s_physics.htm

Interplanetary Space / Space Physics Astronomy Homework Research Help Compiled by Gary Agranat GCA7Sky@AOL.Com Up Home Astronomy Main Index Planetary Sciences Main Page Earth Magnetosphere ... Space Physics missions Solar System Menu Interplanetary Space / Space Physics Solar System Websites Solar System Specialized Websites The Sun Mercury ... Minor Objects: Interplanetary Space / Space Physics Miscelaneous : additional websites which carry Solar System information. Some Related Pages The Sun Earth Earth's Magnetosphere Aurora ... The ASTRONOMY CAFE by Sten Odenwald @ NASA GSFC The IMAGE K12 Education Site: What is space science? The IMAGE / POETRY K12 Space Science Site Primer on the Solar Space Environment @ NOAA NOAA- NESDIS- National Geophysical Data Center (NGDC) Home Page NASA Space Weather.Com Space Weather at Rice University University of Kansas Space Physics ... Space Weather Nat'l Academy of Sciences, Space Studies Board The Solar Wind The Exploration of the Earth's Magnetosphere Space Science Institute Cosmic and Heliospheric Learning Center associated with the ACE spacecraft: The Heliosphere SwRI Imager for Magnetopause-to-Aurora Global Exploration (IMAGE) Mission Web Site Includes a useful glossary , actually a mini-encyclopedia of magnetosphere-space physics terms.

65. 2005 Villa Olmo International Conference Astroparticle, Particle, space physics, Detectors and Medical Physics Applications. Instrumentation as a tool for detection of radiation and effects of http://villaolmo.mib.infn.it/Conference2005.html

International Conference on Advanced Technology and Particle Physics CENTRO DI CULTURA SCIENTIFICA A.VOLTA VILLA OLMO (COMO-ITALY) 9th ICATPP Conference on Astroparticle, Particle, Space Physics, Detectors and Medical Physics Applications Instrumentation as a tool for detection of radiation and effects of radiation in particle physics, astroparticle physics, space and medical applications Villa Olmo, Como 17-21 October 2005) 2005 Conference Schedule Preliminary Conference Programme Session Information Conference Poster ... Call for papers: Abstracts already agreed with the session organizers or organizing committee can be still submitted Exhibition Abstract Submission Article submission and Conference Proceedings Registration Hotel Reservation ... To contact Session Organizers Slides of Presented talks Companion Program Villa Olmo: Volta Centre Information Inside Villa Olmo How to reach Como and Villa Olmo Como Visitor Information links click to magnify Here you can find the locations of hotels and Villa Olmo: A special Covenant connects the "A.Volta" Centre for Scientific Culture to

66. Space Physics Group - Home Page Welcome to space physics Group. Our parent WWW pages; Department of Electronics and Vacuum Physics Faculty of Mathematics and Physics http://www.troja.mff.cuni.cz/fs_troja/kevf/kosmos/home.htm.en

Zmena kodu a jazyka / Change language and charset Welcome to Space Physics Group Our parent WWW pages: Department of Electronics and Vacuum Physics Faculty of Mathematics and Physics Charles University in Prague About Czech Republic News People ... Study Connections: e-mail: Dr. J. Safrankova (jana.safrankova@mff.cuni.cz) (head of the group) tel.: fax: address: KEVF MFF UK, V Holesovickach 2, 18000 Prague 8, Czech Republic News: People: Staff and students Science: The scientific research of our group is oriented to the experimental investigation of the space environment. Members of the group participate in a development of space plasma instruments, processing and interpretation of data collected during many international experiments, and are involved in a laboratory research as well. Scientific fields in our work Cooperating institutions List of launched and planned instruments Publications in Proceedings of the NATO Advanced Research Workshop "Coordinated Studies of the Solar Wind-Magnetosphere-Ionosphere Interaction: INTERBALL Observations", held in Košice, Slovakia, September 7-11, 1998. Our current mission - MAGION 4 subsatellite and INTERBALL-1 tail probe.

67. 400 Years Of "De Magnete" History of geomagnetism, and its relation to space physics and aurora. http://www.phy6.org/earthmag/demagint.htm

The Great Magnet, the Earth by David P. Stern A more technical historical review, overlapping some of the material of this web site, appeared in Reviews of Geophysics in September 2002. under the title A Millennium of Geomagnetism It can now be read here, titled A Millennium of Geomagnetism ...A Spanish translation ...also a French translation by Pascale Cambier with the Belgian Institute of Space Aeronomy. ...and a German translation by Sven Friedel of the University of Leipzig. Incomplete Translations: Polish Ziemia-wielki magnes We are seeking volunteer translators to produce versions in other languages . Please contact the author, Dr. David Stern, earthmag ("at" symbol) phy6.org This is part of a large family of websites. See: http://www.phy6.org/prospect.htm "tared and zipped" compressed version of this set (2 Mb) http://www.phy6.org/earthmg.tar.gz "tar" version joining all files (no compression, 3.8 Mb) at http://www.phy6.org/eartmg.tar (Best viewed in font #14, but print in #10 or #12 Page width=600, with any window width) William Gilbert In 1600, four hundred years ago William Gilbert, later physician to Queen Elizabeth I of England, published his great study of magnetism

68. Welcome To The NSSDC! Provides access to a wide variety of astrophysics, space physics, solar physics, lunar, and planetary data from NASA space flight missions, in addition to selected other data, models, and software. http://nssdc.gsfc.nasa.gov/

Visit the NASA Portal NSSDC Home NSSDC Home NSSDC Mission ... Contact Us Find it @NSSDC Universe Exploration Astrophysics data and mission information Earth-Sun Exploration Space and solar physics data and mission information ... Access to a variety of NASA image products General Services Obtaining Data Master Catalog Anonymous FTP Multimedia Catalog Archive Support NASA/Science Office of Standards and Technology (NOST) Common Data Format (CDF) Flexible Image Transport System (FITS) Guidelines for PDMPs (March 1993, Rich Text Format) White paper on NASA science data retention White paper on Resident archives Machine-dependent number representations Other Services World Data Center for Satellite Information Earth Science Legacy Data Publications Space Science Education Outreach Recent News in... Astrophysics Using NASA's Spitzer Space Telescope , a team of astronomers led by the University of Rochester has detected gaps ringing the dusty disks around two very young stars, which suggests that gas-giant planets have formed there. More...

69. RAL Space Physics Division The space physics Division is concerned with the development and use of space Contact Prof Richard Harrison MBE Head of space physics Division http://www.sstd.rl.ac.uk/Divisions/Space_Physics.htm

Home Overview Contacts  CCLRC Space Physics An overview of the Space Physics Division The Space Physics Division is concerned with the development and use of space instrumentation for space research, specifically in the areas of solar physics, solar terrestrial physics, planetary and magnetospheric physics, astronomy and fundamental physics - and these areas make up the group structure of the Division. The Division operates a scientific, operations and mission development and management programme that is at the very heart of the UK's space programme - and in many ways provides a leading and coordinating role in UK space research, collaborating with many university groups and national and international partners. The Division operates on a world-class level having gained a high reputation through its long heritage of space missions, ground-based systems and facilities and scientific research. Contact: Prof Richard Harrison MBE Head of Space Physics Division Research Areas Astronomy Roger Emery Solar Physics Richard Harrison Solar Terrestral Physics Ian McCrea Manuel Grande Fundamental Physics Bob Bingham Space and Groundbased Research Projects The Space Physics Division is involved in over fifty major space projects. A full list of these can be seen on the Projects page.

70. Radio And Space Physics Group, Aberystwyth Radio and space physics Group, University of Wales, Aberystwyth. http://www.aber.ac.uk/propag/

Radio and Space Physics Group Introduction to the Group Group Members Current Experimental Facilities Theoretical Projects ... Data Maintained by Helen Middleton ( e-mail Last updated 01 August 2003

71. Poetry Includes classroom activities and study guides related to space physics. http://image.gsfc.nasa.gov/poetry/

P. O. E. T. R. Y P ublic O utreach, E ducation, T eaching and R eaching Y outh. This web site provides teachers, students and the interested public with the latest information about auroral science, and the study of Earth's magnetic field. The goal of the IMAGE mission's education and public outreach program (POETRY) is to explain how solar storms affect the Earth, and to correct misconceptions about Earth's magnetic field, its radiation belts, and why we have aurora. Here are some questions that you may have encountered in your textbooks: What causes aurora? Answer What is the solar wind? Answer What is space weather? Answer What is a magnetic field? Answer What are the Van Allen Belts? Answer IMAGE Discoveries Educator Resources Multimedia Gallery ... Warning!!

72. Space Physics Explore theoretical space physics using the latest computational tools. http://www.physics.auburn.edu/research/space.htm

Space Physics Space Plasma Physics Space plasma physics , as opposed to astrophysics, typically addresses the physics of our local solar-system. It deals with the sun, the solar wind, planetary magnetospheres, aurora, and importantly, their interrelationship. Our faculty and students are currently engaged in satellite observation, computational modeling of earth's magnetosphere and its specific features, in the study of our sun, and in the study of magnetic reconnection and other properties of space plasmas through laboratory experiments. Faculty Hinata Lin Perez Thomas

73. Atmospheric Chemistry And Space Physics SRI s research in Atmospheric Chemistry and space physics contributes to understanding of atmospheric processes through active programs in all three http://www-mpl.sri.com/topics/atmspace.html

Atmospheric Chemistry and Space Physics During the past three decades there has developed a growing public awareness of the interrelation between human activity and the atmosphere. In recent years this has evolved an urgency that is leading to major international research efforts to prepare for the political and economic decisions that need to be made. SRI's research in Atmospheric Chemistry and Space Physics contributes to understanding of atmospheric processes through active programs in all three cornerstone areas: field observations, modeling and simulation, and laboratory measurements. Table of Contents Atmospheric Fate of Anthropogenic Substances Heterogeneous Atmospheric Chemistry Reliable Models of Ozone-Depletion Chemistry Aeronomy: Photochemistry of Terrestrial and Planetary Atmospheres ... Ionospheric and Space Sciences Atmospheric Fate of Anthropogenic Substances Industrial activity results in release of wide variety of chemicals to the atmosphere. Some of these chemicals are benign, others are effectively destroyed by natural processes in the atmosphere, and some result in damaging air pollution, acid rain, ozone depletion, or are implicated as promoting potential global climate changes. Increasingly restrictive regulations motivate careful assessment of atmospheric impact and development of new technologies with reduced emissions. SRI scientists and engineers assist clients through testing and monitoring protocols that track pollutants in the environment. Laboratory experimental procedures are used to understand chemical transformations. Optical and sampling techniques are developed for remote and point monitoring of pollutants and transport through the atmosphere.

74. Martindale's Astronomy, Astrophysics & Space Center: Space Physics For more information see space physics Data Facility (SPDF) or the Goddard Space WHAT IS THE MAGNETOSPHERE space physics Plasma Branch, Space Science http://www.martindalecenter.com/GradSpace_5_SPhy.html

M ARTINDALE'S T HE "VIRTUAL" ~ A STRONOMY A S PACE C ENTER SPACE PHYSICS COURSES, TEXTBOOKS TUTORIALS, DATABASES, MOVIES US/Pacific: Saturday, September 17, 2005 Sydney, Australia: Sunday, September 18, 2005 File Download Time Calculator Author, ... Space Radiation Databases SPACE PHYSICS DATABASES - Space Physics Data Facility (SPDF), Goddard Space Flight Center, NASA Space Physics Data Facility (SPDF) or the Goddard Space Flight Center SPACE PHYSICS TEXTBOOK - Space Physics Group, Department of Physical Sciences, University of Oulu, Finland Multimedia Course (Text and Images). Includes: Introduction, Regions of interest (Sun, Earth, Solar System, Solar wind and interplanetary magnetic fields, Cosmic rays, Magnetospher and Ionosphere), Phenomena of interest (Plasma waves, Plasma instabilities, Auroras, Magnetosphere Storms and Substorms, and Plasma Convection), Space Physics instrumentation and Appendixes. For more information see Space Physics Group, Department of Physical Sciences, or the University of Oulu Home Page in English For a complete overview see Text Book page listing (alphabetic order) Some examples from the over "90" Tutorials include Bow shock Cusp Magnetic Field Models (Earth) Pc 4 Pulsations ... Waves in Cold Plasma SEE MATHEMATICS CALCULATORS AND/OR THE SOME EXAMPLES INCLUDE ASTR0-PHYSICAL CALCULATOR - C. Dolan, Department of Astronomy, University of Wisconsin, Madison, Wisconsin

75. Section Of Astrophysics And Space Physics, Physics Dept, Univ. Of Crete http://astrophysics.physics.uoc.gr/

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76. Space Physics Data System: Climax And Haleakala Neutron Monitor Datasets through funding by the National Aeronautics and Space Administration. Go to the space physics Data System home page. Go to the LASR home page. http://ulysses.sr.unh.edu/NeutronMonitor/neutron_mon.html

Would you like to receive update notices every month? Send email HERE Climax and Haleakala neutron monitor operations and research activities are supported by the National Science Foundation (Grant ATM-9912341). This SPDS node was made possible through funding by the National Aeronautics and Space Administration. Principal Investigator: Clifford Lopate . Send email HERE if you need more recent data. Datasets available here are from our monitors at Haleakala, Hawaii (IGY and Supermonitor, 1991-present) [Photo] Huancayo, Peru (IGY, 1953-1992), Climax (IGY, 1951-present) [Photo] Neutron Monitor Locations around the world, plus a Text File with station info. What is a neutron monitor and why should I care? Other cosmic ray sites: Indices of Global Geomagnetic Activity University of Delaware Neutron Monitors Moscow Neutron Monitor! (Near-real-time data) . Other recent neutron monitor rates and a short description of Cosmic Rays at World Data Center A, Boulder. SPIDR, a new neutron monitor data archive , funded by NOAA and NASA/SPDS; over 1700 station-years of hourly value data from more than 117 stations for the years 1953 to the present. If you use our Neutron Monitor data in a scientific publication, please acknowledge us, "National Science Foundation Grant ATM-9912341". We would be interested in receiving a copy of any publication resulting from your use of these data. We welcome any suggestions for improvement, and any "testimonials" would be appreciated!

77. Space Physics And Atmospheric Research Center The space physics and Atmospheric Research Center (SPARC) was established at the Air Force Academy in March 2003 to study the physics of space and upper http://atlas.usafa.af.mil/dfp/dfp_site/sparc.cfm

Space Physics and Atmospheric Research Center DFP Home PEOPLE Joining the Faculty Contact Us RESEARCH Overview Space Physics and Atmospheric Research Physics Education Research ... Cadet Research ACADEMICS Physics Major Meteorology Major LINKS USAFA Academy Admissions Cool Physics Links Background The Space Physics and Atmospheric Research Center (SPARC) was established at the Air Force Academy in March 2003 to study the physics of space and upper atmosphere environments. Over the past ten years the Department of Physics has developed extensive faculty expertise to promote excellence in cadet space physics education and Air Force related space research. The majority of the faculty expertise has resided in military sequential tour officers. From 2000 to the present faculty research efforts have functioned under the Physics Department's Solar Terrestrial Interactions Group (STInG). STInG members individually have proposed for research funding of projects aligned with Air Force needs from a variety of sources such as NASA, NSF and AFOSR. Establishment of the SPARC, with its new civilian manpower, will stabilize the research and allow the Academy to continue providing excellence in space physics education and enhance our research contributions to the Air Force space mission. Areas of Interest Our core area of expertise is the study of how stellar and near-earth-environment plasmas affect the Earth in general and Air Force systems in particular. This expertise ranges from theory and modeling to designing and building instruments for measuring plasma characteristics and integrating our instruments into satellite payloads. SPARC members engage in three main activities: developing payloads for the Academy's small satellite program, applied physics and modeling upper atmospheric response to solar and space weather events. Beyond these main activities, our interests extend from the surface of the Earth to outer space.

78. JHU/APL's Auroral Particles And Imagery Page This site contains information regarding the Aurora Borealis, (aka. The Northern Lights), space physics, and the Earth s magnetosphere. http://sd-www.jhuapl.edu/Aurora/

Click on to enlarge. T he Auroral Particles and Imagery Group at The Johns Hopkins University Applied Physics Laboratory (JHU/APL) has made significant advances in quantitatively understanding certain space physics processes, while uncovering some new mysteries. OVATION: A multi-institutional effort to define the position (and ultimately the intensity) of the auroral oval using multiple data sets cross-calibrated to a single standard. Data from the DMSP satellites, from NASA's Polar UVI imager, and from the University of Alaska, Fairbanks Meridian Scanning Photometer are all incorporated. Only the latter is currently available real-time. The size and position of the auroral oval can be plotted for any time from December 1983 to present. Go To OVATION Real-Time Page GOES derived nowcast Kp and b2i: When the GOES satellites are on the nightside of the Earth, the extent to which the Earth's magnetic field has been stretched from its natural dipole inclination into a long magnetotail is measured by the GOES magnetometers. The more stretched the Earth's magnetic field, the more active is the state of the magnetosphere. GOES magnetometer data is available real-time from NOAA's space data center and from this data, the present values of Kp and b2i can be derived. Current Forecasts of Kp and Dst: As technology advances, space weather prediction has become increasingly important to many human activities, e.g., communications, navigation systems, satellites, power grid, space travel, etc. Kp and Dst are two of the most common indices used to indicate the severity of disturbances in near-Earth space. For the past few years, the ACE spacecraft, located at the L1 point, has been reliably providing solar wind measurements up to approximately 45-60 minutes in advance of its arrival at Earth. Kp and Dst models based on solar wind input can use ACE observations to make short-term forecasts of these two indices.

79. Swedish Institute Of Space Physics Research institute carrying out research in space physics and technology. Research, data, popular science and publications. http://www.irf.se/

Overview Topical Popular Science Research ... Contact Kiruna Umeå Uppsala Lund Latest news Solar Activity Workshop , Lund, 19-21 Sept. Postal address: Box 812, SE-981 28 Kiruna, Sweden Telephone: Fax number: E-mail: irf*irf.se Latest update: 2005-09-05 Webmaster*irf.se The Swedish Institute of Space Physics (Institutet för rymdfysik, IRF) is a governmental research institute with 110 employees. Its primary task is to carry out basic research, education and associated observatory activities in space physics, space technology and atmospheric physics. IRF has employees in Kiruna, Umeå, Uppsala and Lund. The main office is located in Kiruna (geographic coordinates 67.84° N, 20.41° E).

80. JHU/APL's Auroral Particles And Imagery - Interwoven Space Physics Stories Interwoven space physics Stories. about the solar wind striking the Earth, the aurora, and the halo around both of the Earth s magnetic poles http://sd-www.jhuapl.edu/Aurora/stories/hp.eng.html

Interwoven Space Physics Stories about the solar wind striking the Earth, the aurora, and the halo around both of the Earth's magnetic poles Presented bilingually. Click to toggle: Scientific Presentation Plain English Top Story: Solar Cycle and the Aurora After the 11-year solar cycle was established in the 18th century, efforts began to find out if the terrestrial environment was affected. The first relationship which seemed clear is that more aurora occur following solar maximum that minimum. We re-examined this question to test a controversial theory of auroral arc formation, with surprising results. Story 1: Is the aurora there when no one is looking? The aurora has been studied for centuries by scientists and enjoyed by others for much longer. The northern lights can only be seen at nighttime, but it has always been assumed that, like the stars, the aurora was still there after the sun came out. New research by the auroral particles and images group at JHU/APL shows that aurora which are intense enough to be seen with the unaided eye are in fact comparatively rare when the sun is above the horizon. The northern lights are present much more often when they can be seen (when the sun is down). Story 2: Barring the Earth's Halo.

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