語系:
繁體中文
English
說明(常見問題)
回圖書館首頁
手機版館藏查詢
登入
回首頁
切換:
標籤
|
MARC模式
|
ISBD
Design and application of a PC inter...
~
Franke, Danny R.
FindBook
Google Book
Amazon
博客來
Design and application of a PC interfaced cosmic ray detection system for secondary school physics programs.
紀錄類型:
書目-電子資源 : Monograph/item
正題名/作者:
Design and application of a PC interfaced cosmic ray detection system for secondary school physics programs./
作者:
Franke, Danny R.
面頁冊數:
72 p.
附註:
Source: Masters Abstracts International, Volume: 44-01, page: 0375.
Contained By:
Masters Abstracts International44-01.
標題:
Physics, Elementary Particles and High Energy. -
電子資源:
http://pqdd.sinica.edu.tw/twdaoapp/servlet/advanced?query=1427583
ISBN:
9780542187889
Design and application of a PC interfaced cosmic ray detection system for secondary school physics programs.
Franke, Danny R.
Design and application of a PC interfaced cosmic ray detection system for secondary school physics programs.
- 72 p.
Source: Masters Abstracts International, Volume: 44-01, page: 0375.
Thesis (M.S.)--University of Missouri - Saint Louis, 2005.
A great deal of current cosmic ray research focuses on those in the ultra high energy regime (>1018 eV). Though interesting in their own right, they also have implications in astronomy and cosmology. The arrival frequency of these particles is on the order of one per square kilometer per century. Such a low number of arrivals requires the construction of detectors that are capable of uninterrupted observation over an area of hundreds of square kilometers. Several detectors already exist, such as AUGER, and AGASA. One proposed detection system involves placing a large number of small detectors in high schools located across large distances. The construction and operation of these detectors is to be part of educational outreach intended to generate interest in physics and science. While this makes labor and finding locations easy, it introduces several new complications such as the training of staff at a pre-college level. Despite being small and robust as compared to their commercial counterparts, these detectors can be fairly imposing to a high school level audience. This project aims to build an intermediate detection system by which high school teachers and students can learn the basics of cosmic ray research without significant commitment of time or capital. Ideally this detection system would be offered as a kit which, under the supervision of a teacher, a high school student could build and test themselves. The main piece of technology that facilitates such a detector to be offered at low cost is the use of an embedded microcontroller such as PICmicro RTM Microcontrollers [1]. This allows for most of the engineering to be done on the software level which can be freely distributed over the Internet.
ISBN: 9780542187889Subjects--Topical Terms:
1019488
Physics, Elementary Particles and High Energy.
Design and application of a PC interfaced cosmic ray detection system for secondary school physics programs.
LDR
:02653nmm 2200289 4500
001
1826294
005
20061211120337.5
008
130610s2005 eng d
020
$a
9780542187889
035
$a
(UnM)AAI1427583
035
$a
AAI1427583
040
$a
UnM
$c
UnM
100
1
$a
Franke, Danny R.
$3
1915265
245
1 0
$a
Design and application of a PC interfaced cosmic ray detection system for secondary school physics programs.
300
$a
72 p.
500
$a
Source: Masters Abstracts International, Volume: 44-01, page: 0375.
500
$a
Adviser: David Kraus.
502
$a
Thesis (M.S.)--University of Missouri - Saint Louis, 2005.
520
$a
A great deal of current cosmic ray research focuses on those in the ultra high energy regime (>1018 eV). Though interesting in their own right, they also have implications in astronomy and cosmology. The arrival frequency of these particles is on the order of one per square kilometer per century. Such a low number of arrivals requires the construction of detectors that are capable of uninterrupted observation over an area of hundreds of square kilometers. Several detectors already exist, such as AUGER, and AGASA. One proposed detection system involves placing a large number of small detectors in high schools located across large distances. The construction and operation of these detectors is to be part of educational outreach intended to generate interest in physics and science. While this makes labor and finding locations easy, it introduces several new complications such as the training of staff at a pre-college level. Despite being small and robust as compared to their commercial counterparts, these detectors can be fairly imposing to a high school level audience. This project aims to build an intermediate detection system by which high school teachers and students can learn the basics of cosmic ray research without significant commitment of time or capital. Ideally this detection system would be offered as a kit which, under the supervision of a teacher, a high school student could build and test themselves. The main piece of technology that facilitates such a detector to be offered at low cost is the use of an embedded microcontroller such as PICmicro RTM Microcontrollers [1]. This allows for most of the engineering to be done on the software level which can be freely distributed over the Internet.
590
$a
School code: 0481.
650
4
$a
Physics, Elementary Particles and High Energy.
$3
1019488
650
4
$a
Education, Sciences.
$3
1017897
650
4
$a
Education, Secondary.
$3
539262
690
$a
0798
690
$a
0714
690
$a
0533
710
2 0
$a
University of Missouri - Saint Louis.
$3
1017796
773
0
$t
Masters Abstracts International
$g
44-01.
790
1 0
$a
Kraus, David,
$e
advisor
790
$a
0481
791
$a
M.S.
792
$a
2005
856
4 0
$u
http://pqdd.sinica.edu.tw/twdaoapp/servlet/advanced?query=1427583
筆 0 讀者評論
館藏地:
全部
電子資源
出版年:
卷號:
館藏
1 筆 • 頁數 1 •
1
條碼號
典藏地名稱
館藏流通類別
資料類型
索書號
使用類型
借閱狀態
預約狀態
備註欄
附件
W9217157
電子資源
11.線上閱覽_V
電子書
EB
一般使用(Normal)
在架
0
1 筆 • 頁數 1 •
1
多媒體
評論
新增評論
分享你的心得
Export
取書館
處理中
...
變更密碼
登入