The solar wind during STIP II interval: stream structures, boundaries, shocks 
and other features as observed on Helios-1 and Helios-2

Schwenn, R.; Rosenbauer, H.; Mühlhäuser, K.-H.

アイテム詳細

登録内容を編集ファイル形式で保存

一時保存へ追加

タグ情報を表示リリース履歴を表示詳細要約

公開

会議論文

The solar wind during STIP II interval: stream structures, boundaries, shocks and other features as observed on Helios-1 and Helios-2

MPS-Authors

/persons/resource/persons104200

Schwenn, R.
Department Sun and Heliosphere, Max Planck Institute for Solar System Research, Max Planck Society;
MPI for Aeronomy, Max Planck Institute for Solar System Research, Max Planck Society;

/persons/resource/persons104165

Rosenbauer, H.
MPI for Aeronomy, Max Planck Institute for Solar System Research, Max Planck Society;

External Resource

There are no locators available

Fulltext (restricted access)

There are currently no full texts shared for your IP range.

フルテキスト (公開)

公開されているフルテキストはありません

付随資料 (公開)

There is no public supplementary material available

引用

Schwenn, R., Rosenbauer, H., & Mühlhäuser, K.-H. (1977). The solar wind during STIP II interval: stream structures, boundaries, shocks and other features as observed on Helios-1 and Helios-2. In M. A., Shea, D. F., Smart, & S. T., Wu (Eds.), Contributed Papers to the Study of Travelling Interplanetary Phenomena/77 (pp. 351-361). Hanscom AFB, MA, U.S.A.: Air Force Geophysics Laboratory.

引用: https://hdl.handle.net/11858/00-001M-0000-0014-E8BF-5

要旨

要旨はありません