'High cadence' presentation slideshows

LYRA and SWAP on board PROBA2 Heralding future solar UV observations

LYRA and SWAP on board PROBA2 Heralding future solar UV observations. J.-F. Hochedez & D. Berghmans (SIDC-ROB) J.-M. Defise (CSL-ULg) + the LYRA and SWAP teams. Where to go, with solar UV observations?. (Long-term) temporal coverage. Temperature range/coverage (spectral resolution).

456 views • 45 slides

Solar-B XRT

Solar-B XRT. Initial Science Observations. Ed DeLuca for the XRT Team. X-Ray Telescope Mirror inner diameter: 35 cm Focal Length: 2700 cm Geometric Area: 5 cm 2 Shutter/Analysis Filters t exp : 2ms to 10s 9 X-ray, 1 WL filter Camera 2K ? 2K back-illuminated CCD

316 views • 20 slides

Solar-B XRT

Solar-B XRT. Initial Science Observations. Ed DeLuca for the XRT Team. X-Ray Telescope Mirror inner diameter: 35 cm Focal Length: 2700 cm Geometric Area: 5 cm 2 Shutter/Analysis Filters t exp : 2ms to 10s 9 X-ray, 1 WL filter Camera 2K ? 2K back-illuminated CCD

202 views • 20 slides

Observing Sequences in View of the SECCHI Science Goals From the EUVI Perspective

226 views • 11 slides

The SECCHI Campaign

The SECCHI Campaign. Jean-Pierre Wuelser SECCHI Consortium Meeting Orsay. Outline. What is a SECCHI Campaign? The first SECCHI Campaign: May 2007 Campaign features and constraints Science objectives A possible campaign observing program Discussion Science focus Observational approach.

255 views • 8 slides

Synchronised High-Cadence Imaging of the Solar Chromosphere: The Rapid Dual Imager (RDI)

123 views • 1 slides