Millimeter wavelength observations of solar flares for Max 1991

Details Millimeter wavelength observations of solar flares for Max 1991 Millimeter wavelength observations of solar flares for Max 1991

Nov 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988fnsm.work..107k&link_type=abstract

In NASA, Goddard Space Flight Center, Max 1991: Flare Research at the Next Solar Maximum. Workshop 1: Scientific Objectives p 10

Physics

Antenna Arrays, Equipment Specifications, Interferometry, Millimeter Waves, Solar Flares, Circular Polarization, Solar Maximum Mission, Spectrum Analysis

Scientific paper

The Hat Creek millimeter-wave interferometer (to be known as the Berkeley-Illinois-Maryland Array, BIMA) is being upgraded. The improved array will become available during the coming solar maximum, and will have guaranteed time for solar observing. The Hat Creek millimeter-wave interferometer is described along with the improvements. The scientific objectives are briefly discussed.

Affiliated with

Also associated with

No associations

Rating

Millimeter wavelength observations of solar flares for Max 1991 does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Millimeter wavelength observations of solar flares for Max 1991, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Millimeter wavelength observations of solar flares for Max 1991 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1825996