Underneath coronal loops: MSDP observations coordinated with SERTS 4 and NIXT flights

Details Underneath coronal loops: MSDP observations coordinated with SERTS 4 and NIXT flights Underneath coronal loops: MSDP observations coordinated with SERTS 4 and NIXT flights

Nov 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992esasp.348..257s&link_type=abstract

In ESA, Proceedings of the First SOHO Workshop: Coronal Streamers, Coronal Loops, and Coronal and Solar Wind Composition p 257-2

Computer Science

Sound

2

Chromosphere, Coronal Loops, Rocket-Borne Instruments, Spectrographs, Velocity Distribution, Flux Density, Sounding Rockets, Spectroheliographs, X Ray Telescopes

Scientific paper

Ground based coordinated observations with the Multichannel Subtractive Double Mass spectrograph (MSDP) allowed the chromospheric intensity and velocity fields below coronal structures during recent launchs of sounding rockets to be portrayed. During SERTS 4 observations (7 May 1991), two different active regions (AR 6615, AR 6608) presenting flare and filament were coaligned with UV structures. On 11 Jul. 1991 (eclipse day) large H alpha ejection material in AR 6713 (N38 W 42) was detected during the NIXT (Normal Incidence X-ray Telescope) flight. Preliminary results are displayed.

Affiliated with

Also associated with

No associations

Rating

Underneath coronal loops: MSDP observations coordinated with SERTS 4 and NIXT flights 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 Underneath coronal loops: MSDP observations coordinated with SERTS 4 and NIXT flights, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Underneath coronal loops: MSDP observations coordinated with SERTS 4 and NIXT flights will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1552343