SOHO UltraViolet Coronagraph Spectrometer


DAS51 RELEASE


News


The final UVCS FITS files have been submitted to the SOHO Archives (as of Oct. 2013). These include uncalibrated (Level 1) and fully calibrated (Level 2) data for the LYA and OVI spectral channels, and the Visible Light channel. The latest Data Analysis Software (DAS51) program is able to read, display, and calibrate the new files. For more information about how to download and use the DAS51 package with the new UVCS FITS files, click on the "DAS51 RELEASE" link above.


For a short time, the old UVCS FITS files (created prior to 2013) can be found on the SOHO Archive here. These files can be read, displayed, and calibrated with the DAS40.

Past Meetings Observations
SOHO 23 Meeting (2009)
UVCS 2000 Science Meeting
UVCS/SOHO 1999 Science Meeting
SOHO 7 Workshop (Oct. 1998)
UVCS/SOHO 1998 Science Meeting
UVCS/SOHO 1997 Science Meeting, Monselice, Italy
UVCS/SOHO 1996 Science Meeting, Baltimore

Observations of the April 21, 2002 Event
Eclipse Support '99
Eclipse Support '98
Comet Observations
Events

Press Release (Feb. 2006): Steven Cranmer Receives 2006 Harvey Prize
Press Release (May 2004): The Sources of Solar Hazards in Interplanetary Space
Press Release (October 2003): Wildfires on the Sun
Press Release for the IUGG 2003 Conference
Press Release (March 2002): Scientists Predict Calmer Weather Ahead
Press Release (April 2001): SOHO 5th Anniversary Celebration
Press Release (July 1999): Surf's Up: Historic Glenn Mission and SOHO Make Major Solar Advance on 37-year old Mystery

UVCS Instrument Model on Display at Boston's Museum of Science

UVCS Reports for the SOHO Fifth Anniversary and Sun-Earth Day Celebrations
List of UVCS Events for the SOHO Fifth Anniversary and Sun-Earth Day Celebrations

The UVCS Data Analysis Software (DAS) and the calibration files are available now through the Solar SoftWare (SSW)

Whole-sun Ly-alpha fluxes measured by the SOLSTICE instrument on UARS may be helpful in analyzing scattered disk light in UVCS spectra. SOLSTICE fluxes are at ftp://laspftp.colorado.edu/pub/solstice/composite_lya.dat



WWW implementation by Peter L. Smith and Raid Suleiman

e-mail