Home News About Us Contact Contributors Disclaimer Privacy Policy Help FAQ

Home
Search
Quick Search
Advanced
Fulltext
Browse
Collections
Persons
My eDoc
Session History
Login
Name:
Password:
Documentation
Help
Support Wiki
Direct access to
document ID:


          Institute: MPI für Sonnensystemforschung     Collection: Solar Studies     Display Documents



ID: 434291.0, MPI für Sonnensystemforschung / Solar Studies
Understanding magnetic structure in the solar corona through topological analysis
Authors:Maclean, R. C.; Parnell, C. E.; De Moortel, I.; Büchner, J.; Priest, E. R.
Research Context:Project(s) = TSSSP, THEORY, Solar
Publisher:ESA Publ. Div.
Place of Publication:Noordwijk
Date of Publication (YYYY-MM-DD):2006
Title of Proceedings:Proc. SOHO 17 - 10 Years of SOHO and beyond, Giardini Naxos, Sicily, Italy,
Start Page:156
End Page:159
Audience:Experts Only
Intended Educational Use:No
Comment of the Author/Creator:On CD
External Publication Status:published
Document Type:Conference-Paper
Affiliations:MPI f�r Sonnensystemforschung/Solar and Heliospheric Studies
Identifiers:LOCALID:Maclean:2006-296
URL:http://adsabs.harvard.edu/abs/2006ESASP.617E.156M
The scope and number of records on eDoc is subject to the collection policies defined by each institute - see "info" button in the collection browse view.