Evolutionary signatures in complex ejecta and their driven shocks
We examine interplanetary signatures of ejecta-ejecta interactions. To this end, two time intervals of inner-heliospheric (≤1AU) observations separated by 2 solar cycles are chosen where ejecta/magnetic clouds are in the process of interacting to form complex ejecta. At the Sun, both int...
Main Authors: | C. J. Farrugia, D. B. Berdichevsky |
---|---|
Format: | Article |
Language: | English |
Published: |
Copernicus Publications
2004-11-01
|
Series: | Annales Geophysicae |
Online Access: | https://www.ann-geophys.net/22/3679/2004/angeo-22-3679-2004.pdf |
Similar Items
-
Optical techniques for characterising shock ejecta
by: Bell, David James
Published: (2011) -
Dust formation in supernova ejecta
by: Shmeld I.
Published: (1994-03-01) -
The ν process in the innermost supernova ejecta
by: Sieverding Andre, et al.
Published: (2017-01-01) -
High-energy X-ray radiography investigation on the ejecta physics of laser shock-loaded tin
by: Weihua He, et al.
Published: (2019-08-01) -
Ejecta velocities in twice-shocked liquid metals under extreme conditions: A
hydrodynamic approach
by: V. Karkhanis, et al.
Published: (2019-07-01)