Resource Detailed View
Open access to near-real-time images, and calibrated Lyman alpha intensities in ASCII table form
The Solar Wind Anisotropy instrument SWAN on board SOHO is monitoring the Lyman alpha radiation of the whole sky once in 24 hours. By subtracting background and constant light sources like stars, subsequent images reveal moving targets, most likely comets. There water orbit parameters and production rates can be derived from the data sets
Calibrated
active
The summary image table gives access to daily full solar system UV images processed for:
- Space weather forecast (radiation on the Sun's far side in spheric coordinates and as Carrington rotation maps)
- Lyman-alpha background maps of the solar system (solar wind distribution)
- Static background removed images to highlight comets
Keywords (4):
Science Cases (4):
SC4.1 - Relative contributions of asteroidal dust, cometary dust... to the structure of zodiacal cloud
SC4.3 - Distant activity, outbursts, splitting and disruption of cometary nuclei
SC4.4 - Comet Churyumov-Gerasimenko outgassing
SC4.5 - Solar wind-comet surface interaction
SC4.3 - Distant activity, outbursts, splitting and disruption of cometary nuclei
SC4.4 - Comet Churyumov-Gerasimenko outgassing
SC4.5 - Solar wind-comet surface interaction




