Dust Deflation by Dust Devils on Mars Derived from Optical Depth Measurements 
Using the Shadow Method in HiRISE Images

Reiss, Dennis; Hoekzema, Nick M.; Stenzel, Oliver J.

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

このアイテムの新しいバージョンが利用可能です:
https://pure.mpg.de/pubman/item/item_2535041_3

詳細要約

公開

ポスター

Dust Deflation by Dust Devils on Mars Derived from Optical Depth Measurements Using the Shadow Method in HiRISE Images

MPS-Authors

/persons/resource/persons103968

Hoekzema, Nick M.
Department Planets and Comets, Max Planck Institute for Solar System Research, Max Planck Society;

/persons/resource/persons104232

Stenzel, Oliver J.
Department Planets and Comets, Max Planck Institute for Solar System Research, Max Planck Society;

External Resource

Link
(全文テキスト（全般）)

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

Reiss, D., Hoekzema, N. M., & Stenzel, O. J. (2014). Dust Deflation by Dust Devils on Mars Derived from Optical Depth Measurements Using the Shadow Method in HiRISE Images. Poster presented at 45th Lunar and Planetary Science Conference, The Woodlands, Texas.

引用: https://hdl.handle.net/21.11116/0000-0000-40A5-D

要旨

要旨はありません