themis.igpp.ucla.edu

artemis.igpp.ucla.edu

ARTEMIS

http://artemis.igpp.ucla.edu/publications.shtml

Register your submitted, in press or accepted THEMIS/ARTEMIS Publication by email. Please visit the following links to access THEMIS/ARTEMIS Science Publications:. Nuggets (summaries of THEMIS research). Click here to order. First Results from the THEMIS Mission, GRL. First Results from the THEMIS Mission, JGR. Substorm Perspectives with Modern Magnetospheric and Ground Observatories, JGR. Auroral Phenomenology and Magnetospheric Processes: Earth and Other Planets. AGU Monograph Series. Data Files - All.

artemis.igpp.ucla.edu

ARTEMIS

http://artemis.igpp.ucla.edu/software.shtml

TDAS 9.0 (including SPEDAS framework version 1.00). THEMIS data can be accessed using TDAS: the THEMIS Data Analysis Software. The current release is TDAS 9.0. This release also includes version 1.00 of the SPEDAS framework, which is now required to run TDAS. SPEDAS stands for "Space Physics Environment Data Analysis Software". There is a blog. On the SPEDAS software. And can download data from dozens of NASA space missions. Read more about the relationship between TDAS and SPEDAS. For Linux, we also off...

artemis.igpp.ucla.edu

ARTEMIS

http://artemis.igpp.ucla.edu/instrument_efi.shtml

The THEMIS Electric Field Instrument (EFI) measures the electric fields in three directions. One pair of sensors is deployed to 20 meters, the other pair to 25 meters. Two stiff telescopic booms extend sensors perpendicular to the four spinning cables and along the probe's spin axis. Sensors - Space Sciences Laboratory, University of California, Berkeley. Data Processing - Laboratory for Atmospheric and Space Physics (LASP), University of Colorado, Boulder. Would you like to see:. Table of EFI Parameters.

artemis.igpp.ucla.edu

ARTEMIS

http://artemis.igpp.ucla.edu/instrument_asi.shtml

And an interactive map is available here. Thumbnail images are transmitted in almost real-time from the sites and corresponding overview plots and CDF-data-files are available about two days following data collection. The full-resolution 256x256 pixel images are transferred via hard-disk swap and become available approximately 3-5 months after data collection. University of California, Berkeley (UCB) and University of Calgary (UofC), Canada. S Mende (UCB) and Eric Donovan (UofC). Would you like to see:.

artemis.igpp.ucla.edu

ARTEMIS

http://artemis.igpp.ucla.edu/instrument_fit.shtml

On-board Spin FIT module. Given a spin rate of 3 seconds, the use of 128 Hz data for spin fitting puts an apparent phase shift of 360/(3*128) or roughly 0.9 degrees into the results. While this meets the 1.0 degree requirement, the phase shift correction can be determined on the ground using the spin pulse time data relative to the 1Hz tick which is the basis of the 128 Hz data. Detailed information on the FIT module and spin-fit processing is available in the Flight Software Documents [FIT Module].

artemis.igpp.ucla.edu

ARTEMIS

http://artemis.igpp.ucla.edu/spacecraft.shtml

ATK Space Systems manufactured the THEMIS spacecraft (probe bus). The five THEMIS probes are identical in design and are capable of being placed in any THEMIS orbit. This provided robustness to the constellation design and allowed for any one of the probes to be placed in any orbit. For more detailed information on the spacecraft design, please visit ATK Probe and Probe Carrier Subsystem (THEMIS). Data Policy and Credits. Data Files - All. Data Files - By Platform. Data Files - By Group.

artemis.igpp.ucla.edu

ARTEMIS

http://artemis.igpp.ucla.edu/instruments.shtml

The five spin-stabilized (spin period = 3 seconds) THEMIS probes carry the comprehensive packages of plasma and field instruments needed to determine the cause of geomagnetic substorms. The instruments being flown are:. Electric field instruments (EFI). Search coil magnetometers (SCM). Solid state telescopes (SST). All-sky white light imagers (ASI). Digital Fields Board (DFB)-Filter Bank (FBK)-Fourier Power Spectra (FFT). On-board Spin Fits (FIT) from EFI and FGM Instruments. Data Policy and Credits.

esp.igpp.ucla.edu

UCLA Experimental Space Physics - Angelopoulos Group

http://esp.igpp.ucla.edu/outreach.html

Learn More About Space Weather. Below are some educational tools and multimedia web resources that explain space weather and basic magnetospheric physics, including the aurora and radiation belts. Our team would love to give interactive presentations at your school or educational event, please contact us! UCLA Planeterrella Aurora Simulator: Space Weather in the Classroom. We can demonstrate the Planeterrella and the basic electric/magnetic principles of space weather for your class or education event!

artemis.igpp.ucla.edu

ARTEMIS

http://artemis.igpp.ucla.edu/instrument_gmags.shtml

THEMIS makes data available from 106 GMAG stations in the Northern United States, Canada, Denmark, Greenland, Norway, Sweden, Iceland, and Russia, and two stations in Antarctica. GMAG daily Availability, Map and information. Station names and data inventory. By year, pdf file). Detailed station data inventory. By month, 2007-2012, pdf file). On the data description page. Detailed station information and location spreadsheet. Instrument status updates are available here. C T Russell (UCLA).