F-corona-experiment: Requirements for remote sensing of interplanetary dust

Details F-corona-experiment: Requirements for remote sensing of interplanetary dust F-corona-experiment: Requirements for remote sensing of interplanetary dust

Nov 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991esasp.317..335m&link_type=abstract

In ESA, 10th ESA Symposium on European Rocket and Balloon Programmes and Related Research p 335-337 (SEE N92-24589 15-12)

Other

Coronagraphs, F Region, Interplanetary Dust, Remote Sensing, Sky Brightness, Infrared Radiation, Optical Properties

Scientific paper

The near solar dust that produces the brightness of the F corona represents the central region of the interplanetary dust cloud. The structure of the inner dust cloud and the properties of the near solar dust contribute to the understanding of the meteoritic complex and its relation to other constituents of the interplanetary medium. The flux rates of these micrometeorites have to be considered for the concept of near solar missions. To investigate this complex a synoptical observation in different spectral ranges is needed. The concept of the dedicated rocket-borne experiment is outlined.

Affiliated with

Also associated with

No associations

Rating

F-corona-experiment: Requirements for remote sensing of interplanetary dust 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 F-corona-experiment: Requirements for remote sensing of interplanetary dust, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and F-corona-experiment: Requirements for remote sensing of interplanetary dust will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1717234