Search

Your search keyword '"Lal, N."' showing total 27 results
Start Over Author "Lal, N." Publication Type Conference Materials
27 results on '"Lal, N."'

4. PV as an ancillary service provider – laboratory and field experiences from IEA PVPS countries

Author

Kraiczy, M., primary, Siegl, S., additional, Schütt, J., additional, Arnold, G., additional, Wende von Berg, S., additional, Mende, D., additional, Braun, M., additional, Bründlinger, R., additional, Heilscher, G., additional, Chen, S., additional, Cauz, M., additional, Perret, L., additional, Guerrero Lemus, R., additional, Lal, N., additional, Knobloch, A., additional, Premm, D., additional, Bucher, C., additional, MacGill, I., additional, Jäger-Waldau, A., additional, Adinolfi, G., additional, and Graditi, G., additional

Published
2021
Full Text
View/download PDF

10. Anomalous Cosmic Rays in the Heliosheath

Author

Cummings, A. C., primary, Stone, E. C., additional, McDonald, F. B., additional, Heikkila, B. C., additional, Lal, N., additional, Webber, W. R., additional, Li, Gang, additional, Hu, Qiang, additional, Verkhoglyadova, Olga, additional, Zank, Gary P., additional, Lin, R. P., additional, and Luhmann, J., additional

Published
2008
Full Text
View/download PDF

14. The Energetic Particle Populations of the Distant Heliosphere.

Author

McDonald, F. B., Cummings, A. C., Stone, E. C., Heikkila, B. C., Lal, N., and Webber, W. R.

Subjects
HELIOSPHERE, COSMIC rays, IONS, SOLAR activity, SPACE environment, SOLAR radiation
Abstract

In late 2003 as Voyager 1 moves beyond 90 AU in the recovery phase of solar cycle 23, the effects of the termination shock (TS) and the heliosheath on particle transport are becoming more evident. There are now detectable fluxes of 2.5 – 70 MeV electrons but at low intensity levels that suggest they are heavily modulated in the heliosheath. The modulation of galactic and anomalous cosmic rays is significant but much smaller than observed at 1 AU. At V1 a large increase of MeV ions was observed with a flat energy spectra which persisted over a period of 6.5 months. A second event has now been in progress for some eight months. These ions appear to originate at the TS. At V2, 17 AU behind V1, there are a series of 8 increases of low energy ions that occur approximately every 140 days starting in late 2000. Many of these increases can be related to specific periods of high solar activity that occurred some 6 months earlier. © 2004 American Institute of Physics [ABSTRACT FROM AUTHOR]

Published
2004
Full Text
View/download PDF

Catalog

Books, media, physical & digital resources
See catalog results